WEBVTT

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[SQUEAKING]

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[RUSTLING]

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[CLICKING]

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JOHN SOUTHARD: And this is where
we are, cross-stratification.

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As I remember, this
is what we got to--

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very useful for depositional
interpretations.

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Here's the official definition,
and just make sense.

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That's the official definition
of cross-stratification.

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I think that it's
probably the best

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way of making interpretations
from looking at Strata.

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So it's caused by the action
of bed configurations in a flow

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during aggradation.

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And we typically see sets
of conformable laminae,

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called sets, separated
by truncation surfaces.

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Or maybe not-- Maybe no
truncation surfaces in there.

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You're going to see
what I mean by that.

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So the basic idea
is pretty simple.

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There's a flow over a sediment
bed, and there's deposition.

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And then at a certain time
later, the flow changes.

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Flows change all the time.

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It erodes downward
into that deposit.

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And then it starts
to deposit again.

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And you're left with two sets
separated by a truncation

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surface.

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That's the basic idea.

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And I don't think I'm
telling you anything new.

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But there's a problem,
because if you have erosion,

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there's a certain amount of
time that's not recorded.

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Only when there's
aggradation enough

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so there's never
any truncation do

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you have a complete record
of the time involved

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in the process, which is
unfortunate, but that's the way

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it is.

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So the way you can
get around that is

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to run the flow over
a bed of sediment

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over a wide range of conditions,
either in the laboratory

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or in the natural
environment, and keep

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track of what's happening,
because then you do

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have a record of it.

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Even there's some
erosion later on,

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you know what's
happening through time.

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But the problem is only
in certain situations

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can you actually do
that, unfortunately.

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So I've been
interested, fascinated,

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by cross-stratification since I
was a grad student in the early

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'60s, and not a lot was
known about it then.

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We've made a lot of
advances since then.

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Oh, look at this.

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Oh, thank you.

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And so in the old textbooks
you'd see diagrams like this

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and like this.

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They're sets separated
by laminae, separated

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by truncation surfaces.

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But when you look more closely,
if you look at a block diagram,

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you often see
something like this--

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I'll be getting to this--
in which these are not

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really different
from each other,

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they're just different sections
through a unified deposit.

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I was looking at
this upside down once

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and, holy mackerel,
large scale trough

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classification in a cookbook.

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Isn't that amazing?

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You're going to
get the impression

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that I see cross-stratification
wherever I look.

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OK, so if you're lucky, you
have two angles like that,

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two right angles, or at least
at a considerable angle.

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So you can get different views.

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Just on the face, it
can be difficult to tell

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what's going on.

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If you want to try to back
out paleoflow directions,

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you really need more
than one face to look at.

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And sometimes we have
it, but often we don't.

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So let's start with ripples.

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I told you all about ripples,
ripple bed configurations

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and what they look like
and how they behave.

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And even with a
single ripple train,

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that's just one train
of current ripples,

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technically it's
cross-stratification,

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but typically the ripples
are climbing because there's

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deposition going on
while the ripples are

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doing their thing on the bed.

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And so that leads us to
what's called climbing

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bedform cross-stratification.

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And I have to tell you a little
bit of how bedforms climb.

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And we're dealing with
unidirectional flow now.

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So here's my
favorite terminology.

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You won't see this
much in the literature.

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Erosional-stoss,
climbing ripples,

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the stoss side is the
upstream side and the lee side

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is the downstream side.

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So erosional stoss,
angles climb low

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enough so that a given
ripple cuts partway

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into the next ripple downstream
and produces a set of laminae

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that's separated
from later deposits

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by a truncation surface.

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But sometimes the angle
of climb is large enough

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to produce to preserve
the entire ripple profile.

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And then there are no
truncation surfaces,

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and you can see the whole
thing, which is nice,

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but it's not nearly as common
as low angle erosional stoss.

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Oh, and I should mention that.

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In the official terminology,
in the literature,

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people call it subcritical
klein versus supercritical,

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but that doesn't tell you much.

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So I prefer erosional stoss
and depositional stoss.

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So let's start out.

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But here's a little
train of ripples.

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And here's one
ripple in the train.

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We cut the ripple with an
imaginary vertical section

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parallel to flow.

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And do that for a large
number of sections,

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and all those points where the
low point was in the trough

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are connected with a rather
sinuous, snaky-looking

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little surface, connecting
all the low points

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all along the trough,
which varies considerably

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in its depth and its shape.

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You keep that in mind.

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And that leads to
what I could call

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a cheesewire effect, because
cheese wires are straight,

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linears.

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But this is a snaky cheese wire
that moves down with the ripple

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and changes its shape as it goes
like this, this kind of thing,

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and eats into the next
ripple downstream.

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Every ripple is doing it to
every ripple just downstream.

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And that gives you the
key to what you will get.

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Here's an old profile and
here's a new later profile.

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This is a rotor from the stoss
side, and it's deposited.

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I mean, this is ho-hum stuff.

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I mean, you're aware of that.

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But that's what's going on
when the ripple climb is low.

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So this is the preserved
part of the laminae.

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This is now eroded completely
and gone down that way.

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And that's just what--

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every ripple comes along
and leaves another set

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of what are called four sets.

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And in your copies
of the PowerPoint,

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I wrote it not
fourth, but forests.

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Forests-- I left out an E. A
spell checker won't catch that.

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I corrected it on
the slide that's

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coming along that you have.

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I spent a long time making this
block diagram once long ago.

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Here's a rather garden
variety set of sinuous,

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crested, and variably
deep trough across.

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And it's climbing at
a fairly low angle.

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And we have all these foresets
separated by trunking services.

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Because remember, I told
you how varied ripples are.

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They change their shape.

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They change their size.

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Some of them get formed,
others disappear.

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And so these are
not quite straight,

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regular, tabular
sets of foresets.

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And then if you
look at the cross,

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vertical cross flow
direction sets,

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you can see how trophy it is.

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You get sets of concave upward
laminae separated by one,

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or usually two,
truncation surfaces.

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And we call those
truncation cross sets.

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And I'll be talking
later about what

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we see on a stratification
parallel section.

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But just keep that in mind.

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I'll be talking about
that when the time comes.

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Now, that was for a
low angle of climb.

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At a high angle of climb--

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Now, I'd like to redo this
because it's too regular.

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Even though they're
climbing at a large angle,

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they're still fairly regular.

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Although it's clear to me that
the higher the angle of climb,

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the more regular
the ripples are.

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And I don't know why
that is, but that's

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been my experience and
the experience of others.

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So there are no
truncation surfaces-- so

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maybe occasionally, when
ripples act up and do something

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a little bit different
from their surroundings.

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And this should be a
somewhat more sinuous.

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But there wouldn't be
any truncations in here

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for the reasons that I think
should be clear to you.

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Now, here's my
favorite ripple again.

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And you can see that this
ripple, it's classic.

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It has foreset laminae
faring out into the trough.

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And it has been--
not now-- it has been

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eroding, the ripple underneath.

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So here are the
preserved foresets

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underneath the
truncation surface.

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This is an unusual
ripple-- not unusual,

00:08:50.320 --> 00:08:54.020 align:middle line:84%
but it's irregular in the
sense that early on, when

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the crust was here, the
upstream side, the stoss side,

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was being eroded.

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But then more sediment
came in somehow,

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and now the stoss side is
aggrading, rather than cutting

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down into the underlying stuff.

00:09:10.800 --> 00:09:12.000 align:middle line:90%
So these come and go.

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Things change because of the
irregularity of the ripples.

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Here's a single ripple train.

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And maybe I shouldn't have
put it in here at this point,

00:09:20.920 --> 00:09:23.840 align:middle line:84%
because they don't look
like the one I showed first

00:09:23.840 --> 00:09:26.020 align:middle line:84%
because they're more
nearly symmetrical,

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and they do have
internal laminae.

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You can see vaguely
internal laminae.

00:09:30.260 --> 00:09:35.180 align:middle line:84%
This is more likely to be
oscillatory, oscillation

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ripples, starved or semi-starved
oscillation ripples, rather than

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current ripples.

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And we'll be dealing with
the differences presently.

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Here's a close up of a single
ripple in a ripple train.

00:09:49.310 --> 00:09:51.170 align:middle line:90%
And there is some asymmetry.

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This is more gently
sloping than this side.

00:09:53.890 --> 00:09:55.810 align:middle line:84%
And you can see the
internal lamination.

00:09:55.810 --> 00:09:59.170 align:middle line:84%
But again, this is likely
to be oscillation ripples.

00:09:59.170 --> 00:10:02.190 align:middle line:84%
And I may be arguing-- maybe
I'm going to show you this again

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when we get to talking
about oscillation ripples.

00:10:04.470 --> 00:10:08.170 align:middle line:84%
This is more like a
train of current ripples.

00:10:08.170 --> 00:10:11.030 align:middle line:84%
But there's a tip-off
here that maybe it's

00:10:11.030 --> 00:10:13.350 align:middle line:84%
oscillation influence,
because you see,

00:10:13.350 --> 00:10:16.510 align:middle line:90%
the stoss surface is arched.

00:10:16.510 --> 00:10:18.350 align:middle line:84%
And that suggests
to me they have

00:10:18.350 --> 00:10:22.430 align:middle line:84%
an element of being like
oscillation ripples.

00:10:22.430 --> 00:10:25.430 align:middle line:84%
And toward the end, if I
get a chance to get there,

00:10:25.430 --> 00:10:27.550 align:middle line:84%
there'll be a section
on combined flow

00:10:27.550 --> 00:10:32.350 align:middle line:84%
cross-stratification, which is
a difficult topic to manage,

00:10:32.350 --> 00:10:34.350 align:middle line:90%
and I hope I get there.

00:10:34.350 --> 00:10:37.470 align:middle line:84%
Now-- oh, Kristen
is not here today.

00:10:37.470 --> 00:10:41.570 align:middle line:84%
This is a photo
of a plate I have

00:10:41.570 --> 00:10:44.430 align:middle line:84%
that was made in
modern sediments.

00:10:44.430 --> 00:10:46.410 align:middle line:84%
They cut a surface
with a machete--

00:10:46.410 --> 00:10:48.470 align:middle line:84%
all sedimentary
geologists use a machete.

00:10:48.470 --> 00:10:49.490 align:middle line:90%
I own a machete.

00:10:49.490 --> 00:10:54.010 align:middle line:84%
And you take an epoxy plate and
you put it up against there.

00:10:54.010 --> 00:10:56.370 align:middle line:84%
And because the
differing permeability

00:10:56.370 --> 00:11:00.470 align:middle line:84%
of the various laminae,
you get a relief surface.

00:11:00.470 --> 00:11:01.870 align:middle line:90%
And this is a photo of it.

00:11:01.870 --> 00:11:05.130 align:middle line:84%
All right, so this is
classic erosional stoss

00:11:05.130 --> 00:11:06.430 align:middle line:90%
cross-stratification.

00:11:06.430 --> 00:11:09.090 align:middle line:84%
But it's not entirely
so, because here a ripple

00:11:09.090 --> 00:11:12.690 align:middle line:84%
got especially
vigorous and ended up

00:11:12.690 --> 00:11:14.390 align:middle line:90%
with depositional stuff.

00:11:14.390 --> 00:11:15.950 align:middle line:90%
But it's mainly erosional stoss.

00:11:15.950 --> 00:11:20.970 align:middle line:84%
And we know from
where he made this--

00:11:20.970 --> 00:11:24.050 align:middle line:84%
my colleague, Dick Mayall
from Mobile Research,

00:11:24.050 --> 00:11:25.430 align:middle line:90%
gave me this thing as a gift.

00:11:25.430 --> 00:11:28.970 align:middle line:84%
I really, really
loved to have it.

00:11:28.970 --> 00:11:31.090 align:middle line:90%
This is a flow parallel section.

00:11:31.090 --> 00:11:35.910 align:middle line:84%
And we're not showing what it
would look like at right angles.

00:11:35.910 --> 00:11:37.920 align:middle line:90%
OK, now here's a chunk.

00:11:37.920 --> 00:11:39.880 align:middle line:90%
And this is in Kristen's lab.

00:11:39.880 --> 00:11:43.520 align:middle line:84%
And I'm showing you one
way and then the other way.

00:11:43.520 --> 00:11:45.300 align:middle line:90%
And I want you to look at this.

00:11:45.300 --> 00:11:47.440 align:middle line:84%
I'll give you maybe
almost half a minute here.

00:11:47.440 --> 00:11:48.860 align:middle line:90%
Maybe you don't need that long.

00:11:48.860 --> 00:11:51.860 align:middle line:84%
You have to tell
me which way is up.

00:11:51.860 --> 00:11:54.040 align:middle line:90%
Is this upright or upside down?

00:11:54.040 --> 00:11:56.980 align:middle line:90%
Is this upright or upside down?

00:11:56.980 --> 00:11:58.340 align:middle line:90%
You don't need to tell me now.

00:11:58.340 --> 00:12:00.320 align:middle line:90%
We're going to take a vote.

00:12:00.320 --> 00:12:01.880 align:middle line:90%
So look at it carefully.

00:12:01.880 --> 00:12:03.520 align:middle line:90%
See if you can spot a feature.

00:12:03.520 --> 00:12:04.960 align:middle line:84%
And it's a little
bit complicated.

00:12:04.960 --> 00:12:07.502 align:middle line:84%
Can you spot any feature that
would tell you which way is up?

00:12:07.502 --> 00:12:10.220 align:middle line:90%


00:12:10.220 --> 00:12:11.760 align:middle line:90%
So let's take a vote.

00:12:11.760 --> 00:12:16.860 align:middle line:84%
You can vote-- you can vote the
top is up or the bottom is up,

00:12:16.860 --> 00:12:20.140 align:middle line:84%
or you don't know,
or you can abstain.

00:12:20.140 --> 00:12:25.420 align:middle line:84%
How many people that the
top shows that it's upright?

00:12:25.420 --> 00:12:28.370 align:middle line:84%
How many people the
bottom is upright?

00:12:28.370 --> 00:12:30.120 align:middle line:84%
One, two, three, four--
almost all of you.

00:12:30.120 --> 00:12:33.740 align:middle line:84%
How many people aren't
sure, don't know.

00:12:33.740 --> 00:12:37.260 align:middle line:84%
OK, this is clearly, when
you look at it carefully,

00:12:37.260 --> 00:12:40.200 align:middle line:84%
you see a set of four sets
tailing off into the trough

00:12:40.200 --> 00:12:42.058 align:middle line:84%
and being cut by a
truncation surface.

00:12:42.058 --> 00:12:43.600 align:middle line:84%
And there are some
other places right

00:12:43.600 --> 00:12:47.180 align:middle line:84%
in here, which are less obvious
here and here and right in here.

00:12:47.180 --> 00:12:48.580 align:middle line:90%
But you'll have to look closely.

00:12:48.580 --> 00:12:50.860 align:middle line:84%
See, it doesn't jump
right out at you.

00:12:50.860 --> 00:12:52.100 align:middle line:90%
But you did really well.

00:12:52.100 --> 00:12:56.280 align:middle line:90%


00:12:56.280 --> 00:12:58.380 align:middle line:84%
This is a cut through
modern sediments.

00:12:58.380 --> 00:13:01.660 align:middle line:84%
My valued colleague, senior
colleague, John Harms,

00:13:01.660 --> 00:13:04.180 align:middle line:84%
one of my mentors
early in my career,

00:13:04.180 --> 00:13:08.160 align:middle line:84%
cut this through unconsolidated
sediment, a view perpendicular

00:13:08.160 --> 00:13:08.980 align:middle line:90%
to flow.

00:13:08.980 --> 00:13:10.980 align:middle line:90%
And you can see the troughiness.

00:13:10.980 --> 00:13:12.680 align:middle line:90%
I like that word, troughiness.

00:13:12.680 --> 00:13:16.500 align:middle line:84%
All these little troughy
sets here with convex,

00:13:16.500 --> 00:13:20.000 align:middle line:84%
concave upward laminae
cut by one or two

00:13:20.000 --> 00:13:22.480 align:middle line:84%
or sometimes even three
truncation surfaces.

00:13:22.480 --> 00:13:25.140 align:middle line:84%
In the scale here, these
are inches over here.

00:13:25.140 --> 00:13:29.720 align:middle line:84%
So you see it's like a few
centimeter scale, small scale

00:13:29.720 --> 00:13:31.400 align:middle line:90%
trough cross-stratification.

00:13:31.400 --> 00:13:33.020 align:middle line:90%
Now, tell me about this.

00:13:33.020 --> 00:13:34.690 align:middle line:90%
What do you think about that?

00:13:34.690 --> 00:13:36.970 align:middle line:84%
Does that look
right to you or not?

00:13:36.970 --> 00:13:39.190 align:middle line:90%
I see a shaking head.

00:13:39.190 --> 00:13:43.150 align:middle line:84%
OK, well, the next slide
shows it in the other way.

00:13:43.150 --> 00:13:46.090 align:middle line:84%
And that's clearly small
scale trough cross-strat.

00:13:46.090 --> 00:13:48.330 align:middle line:90%
So you have to make sure--

00:13:48.330 --> 00:13:49.612 align:middle line:90%
troughiness, I like that word.

00:13:49.612 --> 00:13:51.570 align:middle line:84%
I'm not sure how to spell
it, and it's probably

00:13:51.570 --> 00:13:54.690 align:middle line:90%
not a real word anyway.

00:13:54.690 --> 00:13:58.250 align:middle line:90%
OK, so here's some examples--

00:13:58.250 --> 00:14:03.170 align:middle line:84%
erosional stoss, but
there's some places where

00:14:03.170 --> 00:14:05.310 align:middle line:90%
it's almost depositional stoss.

00:14:05.310 --> 00:14:09.290 align:middle line:84%
And the ripple profiles don't
quite look like current ripples.

00:14:09.290 --> 00:14:12.430 align:middle line:84%
So I'm figuring this may
be a combined flow feature.

00:14:12.430 --> 00:14:16.130 align:middle line:84%
Maybe there's an
oscillation influenced,

00:14:16.130 --> 00:14:17.850 align:middle line:90%
largely unidirectional flow.

00:14:17.850 --> 00:14:20.610 align:middle line:84%
And you have to
look close to guess

00:14:20.610 --> 00:14:23.130 align:middle line:84%
whether it's purely
unidirectional

00:14:23.130 --> 00:14:24.790 align:middle line:84%
or whether it's
oscillation influence.

00:14:24.790 --> 00:14:26.310 align:middle line:90%
It's often a problem.

00:14:26.310 --> 00:14:28.498 align:middle line:84%
A matter of fact, it's
a much bigger problem

00:14:28.498 --> 00:14:30.290 align:middle line:84%
if you're dealing with--
this is something,

00:14:30.290 --> 00:14:33.430 align:middle line:84%
I don't know how this got in
here in this particular place.

00:14:33.430 --> 00:14:37.210 align:middle line:84%
This is the thing I showed
you, except not as nice.

00:14:37.210 --> 00:14:39.130 align:middle line:84%
But you see all the
troughiness in here.

00:14:39.130 --> 00:14:42.950 align:middle line:84%
So it's a face that's largely
perpendicular to flow.

00:14:42.950 --> 00:14:45.470 align:middle line:84%
It gets a little
messier down in here.

00:14:45.470 --> 00:14:47.810 align:middle line:84%
I'll talk more about
messiness when we get there.

00:14:47.810 --> 00:14:51.110 align:middle line:90%


00:14:51.110 --> 00:14:53.837 align:middle line:84%
My wife wanted to put this
in the church yard sale.

00:14:53.837 --> 00:14:56.170 align:middle line:84%
And it was sitting on the
table and looking at it, says,

00:14:56.170 --> 00:14:58.750 align:middle line:84%
that's erosional stoss
cross-stratification right

00:14:58.750 --> 00:14:59.510 align:middle line:90%
there.

00:14:59.510 --> 00:15:00.170 align:middle line:90%
We kept it.

00:15:00.170 --> 00:15:02.550 align:middle line:90%
We didn't give it up.

00:15:02.550 --> 00:15:06.150 align:middle line:84%
I see cross-stratification
everywhere.

00:15:06.150 --> 00:15:09.650 align:middle line:84%
This is a messier example,
a real life kind of example.

00:15:09.650 --> 00:15:11.630 align:middle line:84%
But it's clear that
there's climbing ripples

00:15:11.630 --> 00:15:13.510 align:middle line:90%
and there's ripple drift.

00:15:13.510 --> 00:15:16.430 align:middle line:84%
Incidentally, some people
use the term ripple

00:15:16.430 --> 00:15:18.650 align:middle line:90%
drift cross-stratification.

00:15:18.650 --> 00:15:19.810 align:middle line:90%
But I don't like that term.

00:15:19.810 --> 00:15:21.430 align:middle line:90%
But it's in the literature.

00:15:21.430 --> 00:15:24.230 align:middle line:90%


00:15:24.230 --> 00:15:26.670 align:middle line:90%
This is an interesting slide.

00:15:26.670 --> 00:15:30.840 align:middle line:84%
This is a surface
in a turbidite that

00:15:30.840 --> 00:15:32.560 align:middle line:90%
was deposited with Normanskill.

00:15:32.560 --> 00:15:35.480 align:middle line:84%
It's a deep basin
turbidite-- big, thick stack

00:15:35.480 --> 00:15:39.840 align:middle line:84%
of sand, sandstone, shale,
interbedded sandstone and shale.

00:15:39.840 --> 00:15:42.340 align:middle line:84%
And the ripples are
climbing depositionally.

00:15:42.340 --> 00:15:44.680 align:middle line:90%
But look at their shapes.

00:15:44.680 --> 00:15:46.640 align:middle line:90%
They're very undulatory.

00:15:46.640 --> 00:15:49.240 align:middle line:84%
And if I'd looked at that
without knowing where

00:15:49.240 --> 00:15:51.400 align:middle line:84%
it came from, I'd say,
well, that's a combined

00:15:51.400 --> 00:15:53.160 align:middle line:90%
flow, a combined flow.

00:15:53.160 --> 00:15:54.140 align:middle line:90%
But it isn't.

00:15:54.140 --> 00:15:55.000 align:middle line:90%
It's in a turbidite.

00:15:55.000 --> 00:15:56.680 align:middle line:90%
And I don't understand it.

00:15:56.680 --> 00:16:02.000 align:middle line:84%
So I certainly don't
have all the answers.

00:16:02.000 --> 00:16:03.240 align:middle line:90%
John Harms gave me this, too.

00:16:03.240 --> 00:16:06.180 align:middle line:84%
This is a cut in the
Chaco river, New Mexico,

00:16:06.180 --> 00:16:07.200 align:middle line:90%
parallel to flow.

00:16:07.200 --> 00:16:08.920 align:middle line:90%
There's a sidebar.

00:16:08.920 --> 00:16:11.480 align:middle line:84%
And you can see there's
lots of climbing ripples.

00:16:11.480 --> 00:16:13.400 align:middle line:84%
Down here, they're
climbing at a low angle.

00:16:13.400 --> 00:16:15.140 align:middle line:90%
And they climb higher or higher.

00:16:15.140 --> 00:16:17.780 align:middle line:84%
And there's some kind
of hiatus in there.

00:16:17.780 --> 00:16:20.700 align:middle line:84%
Then they start to climb again,
and they go up to vertical.

00:16:20.700 --> 00:16:22.740 align:middle line:84%
And at the top,
they're being draped.

00:16:22.740 --> 00:16:25.640 align:middle line:84%
The ripples start moving,
but sediment is still

00:16:25.640 --> 00:16:26.340 align:middle line:90%
showering down.

00:16:26.340 --> 00:16:29.130 align:middle line:90%
So you're draping the ripples.

00:16:29.130 --> 00:16:32.510 align:middle line:84%
This is maybe one event
bed or two event beds.

00:16:32.510 --> 00:16:35.450 align:middle line:84%
But things change during the
deposition of an event bed.

00:16:35.450 --> 00:16:38.210 align:middle line:84%
So you have to look
at it layer by layer

00:16:38.210 --> 00:16:41.730 align:middle line:84%
to try to make sense of how
the flow changed with time.

00:16:41.730 --> 00:16:42.750 align:middle line:90%
Here's another example.

00:16:42.750 --> 00:16:45.010 align:middle line:84%
This is from glacial
Lake Hitchcock.

00:16:45.010 --> 00:16:46.730 align:middle line:84%
My valued colleague,
Gail Ashley,

00:16:46.730 --> 00:16:50.490 align:middle line:84%
took me out and showed me
the stuff, a flow parallel

00:16:50.490 --> 00:16:54.450 align:middle line:84%
section of erosional
source, rock climbers

00:16:54.450 --> 00:16:56.650 align:middle line:84%
going into depositional
source and then

00:16:56.650 --> 00:17:02.130 align:middle line:84%
into drapes, a waning
flow kind of situation.

00:17:02.130 --> 00:17:04.349 align:middle line:84%
And we got together and
made some experiments,

00:17:04.349 --> 00:17:05.450 align:middle line:90%
the lab got it--

00:17:05.450 --> 00:17:08.010 align:middle line:84%
paper out of it long ago,
in the '70s sometime.

00:17:08.010 --> 00:17:11.250 align:middle line:84%
So we started out with a
preexisting rippled bed.

00:17:11.250 --> 00:17:13.349 align:middle line:84%
And then we were
showering sediment.

00:17:13.349 --> 00:17:17.250 align:middle line:84%
This was a narrow, long
flume, about 5 meters long.

00:17:17.250 --> 00:17:22.130 align:middle line:84%
And we set up a shaker
apparatus all along above,

00:17:22.130 --> 00:17:24.829 align:middle line:90%
which would shake sand in.

00:17:24.829 --> 00:17:26.630 align:middle line:84%
And so it would
gradually upgrade the bed

00:17:26.630 --> 00:17:28.610 align:middle line:90%
while the ripples were working.

00:17:28.610 --> 00:17:30.750 align:middle line:84%
And we arranged it
so that we gradually

00:17:30.750 --> 00:17:33.890 align:middle line:84%
decreased the flow velocity
while the sediment was falling

00:17:33.890 --> 00:17:37.110 align:middle line:84%
and so just the same way we go
from low angle to high angle

00:17:37.110 --> 00:17:38.790 align:middle line:90%
to drape.

00:17:38.790 --> 00:17:41.910 align:middle line:84%
So you do see that
in various places.

00:17:41.910 --> 00:17:47.030 align:middle line:84%
We actually did the same by
starting out with a rippled bed

00:17:47.030 --> 00:17:51.490 align:middle line:84%
at low velocities, draping,
going to high angle

00:17:51.490 --> 00:17:54.550 align:middle line:84%
climb, low angle climb,
back into high climb,

00:17:54.550 --> 00:17:55.730 align:middle line:90%
and back into drapes.

00:17:55.730 --> 00:17:58.730 align:middle line:84%
It's an almost
symmetrical climb.

00:17:58.730 --> 00:18:01.670 align:middle line:84%
STUDENT: Climb directly
related to the velocity,

00:18:01.670 --> 00:18:02.685 align:middle line:90%
the change in angle?

00:18:02.685 --> 00:18:04.310 align:middle line:84%
JOHN SOUTHARD: Well,
it's a combination

00:18:04.310 --> 00:18:06.510 align:middle line:84%
of how fast the
ripples are moving

00:18:06.510 --> 00:18:08.710 align:middle line:84%
and how fast the
bed is degrading.

00:18:08.710 --> 00:18:11.270 align:middle line:84%
So look at the
ratio of aggradation

00:18:11.270 --> 00:18:13.510 align:middle line:90%
to bed form movement.

00:18:13.510 --> 00:18:16.430 align:middle line:84%
And the higher, the stronger the
faster the flow and the stronger

00:18:16.430 --> 00:18:18.650 align:middle line:84%
the ripples are moving
for a given aggradation,

00:18:18.650 --> 00:18:23.190 align:middle line:84%
the more likely there is to
be low angle stratification.

00:18:23.190 --> 00:18:26.330 align:middle line:84%
And only when the
ripples move slow

00:18:26.330 --> 00:18:28.150 align:middle line:84%
relative to the
rate of aggradation,

00:18:28.150 --> 00:18:31.130 align:middle line:84%
you get a high angle of climb
until finally, the ripples start

00:18:31.130 --> 00:18:32.470 align:middle line:90%
moving and it's just draped.

00:18:32.470 --> 00:18:33.470 align:middle line:90%
Does that make sense?

00:18:33.470 --> 00:18:38.170 align:middle line:90%


00:18:38.170 --> 00:18:39.910 align:middle line:84%
This is also from
the same place.

00:18:39.910 --> 00:18:42.830 align:middle line:84%
But we made a cut, not just a
vertical cut parallel to flow,

00:18:42.830 --> 00:18:44.350 align:middle line:90%
but we made a horizontal cut.

00:18:44.350 --> 00:18:46.410 align:middle line:84%
And you can see
there are packets

00:18:46.410 --> 00:18:49.690 align:middle line:84%
of laminae, sets of laminae,
separated by the truncation

00:18:49.690 --> 00:18:50.470 align:middle line:90%
surfaces.

00:18:50.470 --> 00:18:54.730 align:middle line:84%
But we're seeing the
truncation surfaces from above.

00:18:54.730 --> 00:18:57.850 align:middle line:84%
And I'm going to
get back to what

00:18:57.850 --> 00:19:01.290 align:middle line:84%
these features on that
horizontal surface

00:19:01.290 --> 00:19:04.028 align:middle line:90%
will show you.

00:19:04.028 --> 00:19:05.570 align:middle line:84%
I've looked at a
lot of the Moenkopi,

00:19:05.570 --> 00:19:08.530 align:middle line:84%
and there's some interesting,
really nice section of stuff

00:19:08.530 --> 00:19:13.090 align:middle line:84%
in the Moenkopi just north of
one of the arms of Lake Mead.

00:19:13.090 --> 00:19:16.210 align:middle line:84%
And so that's classic,
low angle erosional

00:19:16.210 --> 00:19:20.650 align:middle line:90%
stoss cross-stratification.

00:19:20.650 --> 00:19:24.320 align:middle line:84%
At a higher angle, there are
also erosional stoss mainly,

00:19:24.320 --> 00:19:27.140 align:middle line:90%
but there's some arching over.

00:19:27.140 --> 00:19:30.720 align:middle line:84%
And that's the kind
of thing that we say,

00:19:30.720 --> 00:19:33.380 align:middle line:84%
well, might that
be a combined flow

00:19:33.380 --> 00:19:35.940 align:middle line:84%
with both, maybe
unidirectional dominated

00:19:35.940 --> 00:19:38.460 align:middle line:84%
and oscillatory
oscillation influence.

00:19:38.460 --> 00:19:45.940 align:middle line:84%
And the lower the angle of
climb, the more ambiguous it is.

00:19:45.940 --> 00:19:49.380 align:middle line:84%
The one I just showed you looked
clearly like unidirectional flow

00:19:49.380 --> 00:19:50.520 align:middle line:90%
cross-stratification.

00:19:50.520 --> 00:19:52.060 align:middle line:84%
But maybe the
angles climb is such

00:19:52.060 --> 00:19:55.660 align:middle line:84%
that you're only depositing
the very lowest part

00:19:55.660 --> 00:19:58.380 align:middle line:90%
of the foresets.

00:19:58.380 --> 00:20:00.120 align:middle line:84%
And you don't see
the whole profile.

00:20:00.120 --> 00:20:01.980 align:middle line:84%
So you're never can
be sure whether you're

00:20:01.980 --> 00:20:04.340 align:middle line:84%
dealing with purely
unidirectional flow or maybe

00:20:04.340 --> 00:20:05.378 align:middle line:90%
oscillation influence.

00:20:05.378 --> 00:20:07.420 align:middle line:84%
It's one of those problems
you have to live with.

00:20:07.420 --> 00:20:09.545 align:middle line:84%
And I've been struggling
with that for a long time.

00:20:09.545 --> 00:20:11.220 align:middle line:84%
When it gets to
this point, they're

00:20:11.220 --> 00:20:13.470 align:middle line:84%
clearly climbing
depositionally, and you look

00:20:13.470 --> 00:20:14.720 align:middle line:90%
at the profiles of the ripple.

00:20:14.720 --> 00:20:18.240 align:middle line:84%
It sure looks like they're
partly oscillation ripples.

00:20:18.240 --> 00:20:20.230 align:middle line:84%
I think you'd agree
with me that they

00:20:20.230 --> 00:20:24.790 align:middle line:84%
don't look the standard
stoss side, a sharp break

00:20:24.790 --> 00:20:30.430 align:middle line:84%
at the brink, and then a slip
face to form the foresets.

00:20:30.430 --> 00:20:34.750 align:middle line:90%


00:20:34.750 --> 00:20:37.270 align:middle line:84%
Here's a case of climb
ripples, where the truncation

00:20:37.270 --> 00:20:41.490 align:middle line:84%
surfaces are obvious and the
foreset lamination is there,

00:20:41.490 --> 00:20:42.730 align:middle line:90%
but it's much less obvious.

00:20:42.730 --> 00:20:46.278 align:middle line:84%
You have to look
closely to see it.

00:20:46.278 --> 00:20:47.570 align:middle line:90%
All right, now a ribbon furrow.

00:20:47.570 --> 00:20:49.190 align:middle line:84%
Have you ever turned
ribbon furrow?

00:20:49.190 --> 00:20:50.250 align:middle line:90%
It's a terrible term.

00:20:50.250 --> 00:20:52.710 align:middle line:84%
I think it's a terrible-- it
doesn't tell you anything.

00:20:52.710 --> 00:21:01.730 align:middle line:84%
So we look at a flow parallel, a
stratification parallel section.

00:21:01.730 --> 00:21:03.270 align:middle line:90%
And I showed this to you.

00:21:03.270 --> 00:21:06.350 align:middle line:84%
So when you see this
in outcrop, it's

00:21:06.350 --> 00:21:08.310 align:middle line:84%
really nice because
it tells you the flow

00:21:08.310 --> 00:21:10.190 align:middle line:90%
is flowing from left to right.

00:21:10.190 --> 00:21:11.790 align:middle line:84%
And those truncation
surfaces are just

00:21:11.790 --> 00:21:14.610 align:middle line:84%
what you saw when you look
at the vertical section.

00:21:14.610 --> 00:21:17.270 align:middle line:84%
This is a section through
those truncation surfaces.

00:21:17.270 --> 00:21:19.473 align:middle line:84%
Now, why are they
convex downstream?

00:21:19.473 --> 00:21:20.390 align:middle line:90%
Can you think of that?

00:21:20.390 --> 00:21:23.310 align:middle line:84%
Can you give me a simple
answer for why they're concave,

00:21:23.310 --> 00:21:26.970 align:middle line:90%
why they're concave downstream?

00:21:26.970 --> 00:21:29.690 align:middle line:90%
Well, I'll tell you why.

00:21:29.690 --> 00:21:31.650 align:middle line:90%
A trough is being filled.

00:21:31.650 --> 00:21:34.590 align:middle line:84%
And you're filling on the
upstream side of the trough,

00:21:34.590 --> 00:21:36.470 align:middle line:90%
which is concave downstream.

00:21:36.470 --> 00:21:41.410 align:middle line:84%
So the laminae that are
making-- doing the filling--

00:21:41.410 --> 00:21:44.130 align:middle line:90%
are all concave downstream.

00:21:44.130 --> 00:21:45.530 align:middle line:90%
So you make the cut.

00:21:45.530 --> 00:21:47.770 align:middle line:84%
You see these concave
downstream laminae.

00:21:47.770 --> 00:21:49.750 align:middle line:84%
And that gives you the
paleoflow direction.

00:21:49.750 --> 00:21:54.170 align:middle line:84%
It's nice to have, but
it's a terrible term.

00:21:54.170 --> 00:21:56.430 align:middle line:84%
This is that same slide
I just showed you.

00:21:56.430 --> 00:21:59.050 align:middle line:84%
And you can see on
the flow parallel

00:21:59.050 --> 00:22:00.713 align:middle line:84%
section, the
horizontal section, you

00:22:00.713 --> 00:22:02.630 align:middle line:84%
can see the flow is
definitely going that way.

00:22:02.630 --> 00:22:06.910 align:middle line:84%
Of course, you already knew
that from the vertical section.

00:22:06.910 --> 00:22:09.250 align:middle line:84%
But sometimes, all you see
is the horizontal section.

00:22:09.250 --> 00:22:10.470 align:middle line:90%
And then you really know.

00:22:10.470 --> 00:22:13.010 align:middle line:90%


00:22:13.010 --> 00:22:17.510 align:middle line:84%
Here's another example I forget
where I took this picture.

00:22:17.510 --> 00:22:21.690 align:middle line:84%
This one I took in Sochi in
Russia at a tea plantation.

00:22:21.690 --> 00:22:22.910 align:middle line:90%
They had paving stones.

00:22:22.910 --> 00:22:25.590 align:middle line:84%
And I forgot about the tea
and just got down and looked

00:22:25.590 --> 00:22:29.292 align:middle line:90%
at them, looked at the rocks.

00:22:29.292 --> 00:22:30.750 align:middle line:84%
But it happens on
large scale, too.

00:22:30.750 --> 00:22:33.170 align:middle line:84%
Now, we're going to talk about
dune cross-stratification.

00:22:33.170 --> 00:22:37.030 align:middle line:84%
Here's a horizontal surface
through large scale dune

00:22:37.030 --> 00:22:38.590 align:middle line:90%
cross-stratification.

00:22:38.590 --> 00:22:41.590 align:middle line:84%
Here's a set of these curving
laminae and another set

00:22:41.590 --> 00:22:43.210 align:middle line:90%
with curving laminae this way.

00:22:43.210 --> 00:22:45.790 align:middle line:84%
And the flow is like
in this way somehow.

00:22:45.790 --> 00:22:48.770 align:middle line:84%
So it's not as common to
see as with small scale,

00:22:48.770 --> 00:22:53.430 align:middle line:84%
because you need a big outcrop,
a nice big outcrop, to see that.

00:22:53.430 --> 00:22:59.630 align:middle line:84%
So dune cross-stratification--
same kind of diagram.

00:22:59.630 --> 00:23:02.250 align:middle line:84%
Remember that at
low flow velocities,

00:23:02.250 --> 00:23:04.400 align:middle line:84%
dunes tend to be
two-dimensional.

00:23:04.400 --> 00:23:06.150 align:middle line:84%
They look the same at
every cross section.

00:23:06.150 --> 00:23:08.192 align:middle line:84%
And at high velocity, it's
the three-dimensional.

00:23:08.192 --> 00:23:11.770 align:middle line:84%
This is-- I drew this, and
it's really too regular.

00:23:11.770 --> 00:23:14.880 align:middle line:84%
But you can see you have
these sets of foresets,

00:23:14.880 --> 00:23:17.460 align:middle line:90%
which are less irregular.

00:23:17.460 --> 00:23:19.840 align:middle line:84%
I think I can say less
irregular than in the three

00:23:19.840 --> 00:23:21.160 align:middle line:90%
dimensional case.

00:23:21.160 --> 00:23:23.000 align:middle line:90%
And again, you see.

00:23:23.000 --> 00:23:28.700 align:middle line:84%
I probably should have
made these more sinuous,

00:23:28.700 --> 00:23:30.220 align:middle line:90%
but it gives you the idea.

00:23:30.220 --> 00:23:33.340 align:middle line:84%
But there's also another one of
the three dimensional ripples.

00:23:33.340 --> 00:23:35.020 align:middle line:90%
It's more likely than dunes.

00:23:35.020 --> 00:23:38.240 align:middle line:84%
It's more likely to see 3D dunes
and their structures than 2D

00:23:38.240 --> 00:23:38.740 align:middle line:90%
dunes.

00:23:38.740 --> 00:23:41.560 align:middle line:84%
And again, this is
pretty much like what

00:23:41.560 --> 00:23:44.460 align:middle line:84%
you see for ripple-- climbing
ripple cross-stratification.

00:23:44.460 --> 00:23:46.240 align:middle line:90%
But it's dunes, much larger.

00:23:46.240 --> 00:23:50.560 align:middle line:84%
And you often see dunes, small
dunes on the large dunes.

00:23:50.560 --> 00:23:53.180 align:middle line:84%
If there's enough surface there
and the velocity is right,

00:23:53.180 --> 00:23:54.840 align:middle line:84%
it'll make dunes
anywhere, including

00:23:54.840 --> 00:23:56.420 align:middle line:90%
on the backs of large dunes.

00:23:56.420 --> 00:23:59.160 align:middle line:90%


00:23:59.160 --> 00:24:02.800 align:middle line:84%
That's Paul Heller, Marianne
Amarto, and my former student,

00:24:02.800 --> 00:24:05.120 align:middle line:84%
Chris Paola, with a
block that just happened

00:24:05.120 --> 00:24:07.240 align:middle line:84%
to be lying there
with two faces almost

00:24:07.240 --> 00:24:08.920 align:middle line:90%
at right angles to each other.

00:24:08.920 --> 00:24:11.600 align:middle line:90%
And I was a photographer.

00:24:11.600 --> 00:24:13.440 align:middle line:90%
And so this is detail.

00:24:13.440 --> 00:24:17.060 align:middle line:84%
So one side shows pretty
good flow parallel

00:24:17.060 --> 00:24:19.520 align:middle line:84%
or nearly full parallel
cross-stratification.

00:24:19.520 --> 00:24:23.000 align:middle line:84%
The other side is sort of
trophy, but somewhat irregular.

00:24:23.000 --> 00:24:24.780 align:middle line:84%
And I'm thinking--
just think about,

00:24:24.780 --> 00:24:26.300 align:middle line:90%
what's the direction of flow?

00:24:26.300 --> 00:24:28.640 align:middle line:84%
And I think, it's not
straight into the board.

00:24:28.640 --> 00:24:32.100 align:middle line:84%
It's probably
something like this,

00:24:32.100 --> 00:24:35.580 align:middle line:84%
to produce that kind of
surface on both sides.

00:24:35.580 --> 00:24:42.980 align:middle line:84%
Here's a close-up of a similar
view of large scale trough

00:24:42.980 --> 00:24:46.580 align:middle line:84%
cross-stratification,
but erosional stoss, flow

00:24:46.580 --> 00:24:48.520 align:middle line:90%
from right to left, obviously.

00:24:48.520 --> 00:24:50.560 align:middle line:90%
And that's just 6 inches there.

00:24:50.560 --> 00:24:55.980 align:middle line:90%


00:24:55.980 --> 00:24:57.560 align:middle line:90%
But how about erosion?

00:24:57.560 --> 00:25:01.020 align:middle line:84%
How about depositional
stoss, climbing dunes?

00:25:01.020 --> 00:25:03.495 align:middle line:84%
I have seen it twice
in my long life.

00:25:03.495 --> 00:25:05.120 align:middle line:84%
I'm going to show
you one picture here.

00:25:05.120 --> 00:25:06.995 align:middle line:84%
It's very uncommon,
because you don't usually

00:25:06.995 --> 00:25:12.070 align:middle line:84%
get a situation, strong flow
and dunes, but a very high rate

00:25:12.070 --> 00:25:13.390 align:middle line:90%
of aggradation.

00:25:13.390 --> 00:25:15.090 align:middle line:90%
And I'll show you a slide.

00:25:15.090 --> 00:25:19.060 align:middle line:84%
This is from the Brushy
Canyon in Delaware Mountains.

00:25:19.060 --> 00:25:20.810 align:middle line:84%
And you can see, it's
not a great picture,

00:25:20.810 --> 00:25:22.310 align:middle line:90%
but it's the best one I have.

00:25:22.310 --> 00:25:26.490 align:middle line:84%
You can see this dune shape
like this, arching over.

00:25:26.490 --> 00:25:28.050 align:middle line:90%
And this is-- that's a lens cap.

00:25:28.050 --> 00:25:29.870 align:middle line:90%
So it's pretty good size.

00:25:29.870 --> 00:25:32.450 align:middle line:84%
I think there's a
turbidite basin.

00:25:32.450 --> 00:25:35.830 align:middle line:84%
I think there was a pre-existing
hollow, good sized hollow,

00:25:35.830 --> 00:25:38.550 align:middle line:90%
which got filled during--

00:25:38.550 --> 00:25:41.350 align:middle line:84%
the ripples were still moving
in there, but the rate of climb,

00:25:41.350 --> 00:25:45.190 align:middle line:84%
because the accumulation of
sediment in the depression,

00:25:45.190 --> 00:25:48.510 align:middle line:84%
was high enough to make a
depositional stoss-- very

00:25:48.510 --> 00:25:49.990 align:middle line:90%
uncommon.

00:25:49.990 --> 00:25:51.010 align:middle line:90%
This is a nice cut.

00:25:51.010 --> 00:25:53.358 align:middle line:84%
We did this in the
Arkansas River, the flow.

00:25:53.358 --> 00:25:54.650 align:middle line:90%
And we knew the flow direction.

00:25:54.650 --> 00:25:55.710 align:middle line:90%
It was a sidebar.

00:25:55.710 --> 00:25:56.590 align:middle line:90%
It's this way.

00:25:56.590 --> 00:25:59.750 align:middle line:84%
And you see the standard
erosional stoss, large scale

00:25:59.750 --> 00:26:07.510 align:middle line:84%
erosional stoss, and the flow
perpendicular troughiness

00:26:07.510 --> 00:26:10.400 align:middle line:90%
of the dunes.

00:26:10.400 --> 00:26:15.040 align:middle line:84%
This is a close-up
of that last slide.

00:26:15.040 --> 00:26:18.800 align:middle line:84%
It's just a classic kind of
trough cross-stratification.

00:26:18.800 --> 00:26:20.560 align:middle line:84%
And there's even a
detail of the detail

00:26:20.560 --> 00:26:22.760 align:middle line:84%
if you want to see what
it really looks like.

00:26:22.760 --> 00:26:26.820 align:middle line:84%
And I won't go into it, but
I always like that photo.

00:26:26.820 --> 00:26:30.320 align:middle line:84%
And here's some
stuff in the ancient

00:26:30.320 --> 00:26:34.000 align:middle line:84%
that's clearly trough
cross-stratification,

00:26:34.000 --> 00:26:38.000 align:middle line:84%
but not always
easily perceivable.

00:26:38.000 --> 00:26:39.220 align:middle line:90%
Now, the Nubian Sandstone.

00:26:39.220 --> 00:26:40.720 align:middle line:84%
I don't know much
about it, but it's

00:26:40.720 --> 00:26:43.180 align:middle line:84%
known to be a
subaqueous deposit.

00:26:43.180 --> 00:26:44.600 align:middle line:90%
It's marine sandstone.

00:26:44.600 --> 00:26:46.040 align:middle line:90%
And look at these sets.

00:26:46.040 --> 00:26:49.640 align:middle line:84%
They could be called
planar tabular sets,

00:26:49.640 --> 00:26:53.760 align:middle line:84%
but with regular foresets,
erosional foresets.

00:26:53.760 --> 00:26:59.840 align:middle line:84%
And I'm guessing that was made
by relatively low velocity 2D

00:26:59.840 --> 00:27:02.420 align:middle line:84%
dunes, rather than
3D irregular dunes,

00:27:02.420 --> 00:27:08.380 align:middle line:84%
which would produce a lot of
variability in set settings.

00:27:08.380 --> 00:27:11.540 align:middle line:84%
I like this because you
get of the two little sets

00:27:11.540 --> 00:27:13.360 align:middle line:84%
with stratification
this way and this side,

00:27:13.360 --> 00:27:15.360 align:middle line:84%
and although you can't
see it well on this side.

00:27:15.360 --> 00:27:16.320 align:middle line:90%
So it's coming right out.

00:27:16.320 --> 00:27:17.760 align:middle line:84%
The flow is coming
right out at you.

00:27:17.760 --> 00:27:18.927 align:middle line:90%
Does that make sense to you?

00:27:18.927 --> 00:27:22.460 align:middle line:90%


00:27:22.460 --> 00:27:26.380 align:middle line:84%
I took this close-up to show how
the foreset laminae come down

00:27:26.380 --> 00:27:29.880 align:middle line:84%
and flare out into the
trough very nicely.

00:27:29.880 --> 00:27:33.060 align:middle line:84%
And, of course, there's
erosion there at that surface.

00:27:33.060 --> 00:27:35.940 align:middle line:90%
That's pretty large-scale.

00:27:35.940 --> 00:27:39.240 align:middle line:90%
Another example, pretty classic.

00:27:39.240 --> 00:27:42.300 align:middle line:90%


00:27:42.300 --> 00:27:44.100 align:middle line:90%
Now, look at this.

00:27:44.100 --> 00:27:48.860 align:middle line:84%
And you should see by now
that looks fishy, right?

00:27:48.860 --> 00:27:50.220 align:middle line:90%
This was a block.

00:27:50.220 --> 00:27:51.320 align:middle line:90%
And you turn upside down.

00:27:51.320 --> 00:27:52.380 align:middle line:90%
Now it looks right.

00:27:52.380 --> 00:27:57.220 align:middle line:84%
So it's easy to spot when
you attune your eye to it.

00:27:57.220 --> 00:27:58.537 align:middle line:90%
I just-- I'll mention this.

00:27:58.537 --> 00:28:00.620 align:middle line:84%
One thing that's nice to
know would be, how do you

00:28:00.620 --> 00:28:01.880 align:middle line:90%
get the bedform height?

00:28:01.880 --> 00:28:03.620 align:middle line:84%
How do you back out
the bedform height

00:28:03.620 --> 00:28:05.840 align:middle line:84%
from what you see in the
cross-stratification?

00:28:05.840 --> 00:28:07.620 align:middle line:84%
And it seems like a
difficult problem.

00:28:07.620 --> 00:28:10.270 align:middle line:84%
But my former
student, Chris Paola,

00:28:10.270 --> 00:28:12.520 align:middle line:84%
and his colleague in the
math department at University

00:28:12.520 --> 00:28:16.080 align:middle line:84%
of Minnesota wrote a paper
back, quite some time ago,

00:28:16.080 --> 00:28:19.680 align:middle line:84%
developing the idea that the
average set thickness is only

00:28:19.680 --> 00:28:22.460 align:middle line:84%
slightly less than the
average bedform height

00:28:22.460 --> 00:28:24.720 align:middle line:84%
and not very sensitive
to the angle of climb.

00:28:24.720 --> 00:28:25.740 align:middle line:90%
And I read the paper.

00:28:25.740 --> 00:28:26.900 align:middle line:90%
I can be convinced by it.

00:28:26.900 --> 00:28:27.900 align:middle line:90%
But that's nice to know.

00:28:27.900 --> 00:28:29.720 align:middle line:84%
You can back out the
size of the bedform

00:28:29.720 --> 00:28:31.820 align:middle line:84%
just by looking at the
cross-stratification,

00:28:31.820 --> 00:28:33.600 align:middle line:84%
no matter what the
angle of climb is.

00:28:33.600 --> 00:28:36.540 align:middle line:84%
Well, how about backing out
flow depth from cross tread?

00:28:36.540 --> 00:28:37.620 align:middle line:90%
How do you do that?

00:28:37.620 --> 00:28:39.480 align:middle line:84%
Well, for ripples,
you can't do it

00:28:39.480 --> 00:28:42.960 align:middle line:84%
because, as I mentioned to
you in the last presentation,

00:28:42.960 --> 00:28:46.720 align:middle line:84%
the size of ripples is almost
independent of flow depth

00:28:46.720 --> 00:28:48.640 align:middle line:84%
unless the flow
is really shallow

00:28:48.640 --> 00:28:51.480 align:middle line:90%
and make for little ripples.

00:28:51.480 --> 00:28:52.820 align:middle line:90%
They do vary with grain size.

00:28:52.820 --> 00:28:55.760 align:middle line:84%
I think I mentioned they're
somewhat longer spacing

00:28:55.760 --> 00:28:57.340 align:middle line:90%
for coarser grain sizes.

00:28:57.340 --> 00:29:00.280 align:middle line:84%
But with dunes, there's
general agreement

00:29:00.280 --> 00:29:02.740 align:middle line:84%
that if you look at the ratio
of flow depth to dune height,

00:29:02.740 --> 00:29:07.310 align:middle line:84%
it's around 7, which makes
us-- if they're at equilibrium.

00:29:07.310 --> 00:29:09.750 align:middle line:84%
And so that gives you a handle
on how deep the flow was

00:29:09.750 --> 00:29:12.490 align:middle line:84%
when you see the dune
height, which you would see

00:29:12.490 --> 00:29:14.570 align:middle line:90%
from the cross stratification.

00:29:14.570 --> 00:29:16.790 align:middle line:90%
I mean, that's-- backing out.

00:29:16.790 --> 00:29:18.370 align:middle line:84%
Now, I'm not going
to say anything

00:29:18.370 --> 00:29:19.870 align:middle line:84%
about antidune
cross-stratification.

00:29:19.870 --> 00:29:21.770 align:middle line:90%
I don't have any photographs.

00:29:21.770 --> 00:29:26.010 align:middle line:84%
But it's reported in the
literature, and it does happen.

00:29:26.010 --> 00:29:30.470 align:middle line:84%
Here's a case-- here's a
flow, supercritical flow.

00:29:30.470 --> 00:29:33.450 align:middle line:84%
And the waves are
moving, are migrating

00:29:33.450 --> 00:29:35.250 align:middle line:90%
upstream, not downstream.

00:29:35.250 --> 00:29:40.490 align:middle line:84%
And the bed geometry is going
along with the upstream,

00:29:40.490 --> 00:29:41.690 align:middle line:90%
moving antidunes.

00:29:41.690 --> 00:29:47.130 align:middle line:84%
And you're leaving
foresets going upstream.

00:29:47.130 --> 00:29:48.670 align:middle line:84%
Then eventually,
the waves break.

00:29:48.670 --> 00:29:51.250 align:middle line:84%
This gets messed up, and
it doesn't preserve them

00:29:51.250 --> 00:29:51.990 align:middle line:90%
all that well.

00:29:51.990 --> 00:29:55.470 align:middle line:84%
And I've never gotten
a photograph of one,

00:29:55.470 --> 00:29:59.410 align:middle line:90%
so I can't help you with that.

00:29:59.410 --> 00:30:01.220 align:middle line:90%
You often see this at the beach.

00:30:01.220 --> 00:30:04.580 align:middle line:84%
A small stream flows across
the beach to the water.

00:30:04.580 --> 00:30:08.920 align:middle line:84%
And it's high Froude number
flow, fast flow, shallow depth.

00:30:08.920 --> 00:30:10.318 align:middle line:84%
And you get these
standing waves.

00:30:10.318 --> 00:30:11.860 align:middle line:84%
Sometimes they're
standing, sometimes

00:30:11.860 --> 00:30:13.340 align:middle line:90%
they're migrating upstream.

00:30:13.340 --> 00:30:16.140 align:middle line:84%
And they break, and
then they reform.

00:30:16.140 --> 00:30:17.700 align:middle line:90%
Those are antidunes.

00:30:17.700 --> 00:30:20.360 align:middle line:84%
They're not a major part of
the stratigraphic record.

00:30:20.360 --> 00:30:22.900 align:middle line:84%
So now we have to talk about
oscillatory flow features.

00:30:22.900 --> 00:30:25.540 align:middle line:84%
So remember this--
there's UM, that's

00:30:25.540 --> 00:30:28.020 align:middle line:84%
the maximum velocity
during an oscillation,

00:30:28.020 --> 00:30:31.260 align:middle line:84%
period T of the
oscillation, and D0,

00:30:31.260 --> 00:30:33.520 align:middle line:84%
which is the orbital
diameter, how far it moves.

00:30:33.520 --> 00:30:36.980 align:middle line:84%
And only two of those are
independent of each other.

00:30:36.980 --> 00:30:39.060 align:middle line:84%
The third depends
on the other two.

00:30:39.060 --> 00:30:42.580 align:middle line:84%
And so we did this with
bed configurations.

00:30:42.580 --> 00:30:45.940 align:middle line:84%
And sometimes you
see a vertical climb.

00:30:45.940 --> 00:30:48.900 align:middle line:84%
You'd think it'd be very common,
but it isn't common at all.

00:30:48.900 --> 00:30:54.260 align:middle line:84%
I've seen it just a few times
in my field observations.

00:30:54.260 --> 00:30:54.940 align:middle line:90%
Why?

00:30:54.940 --> 00:30:55.580 align:middle line:90%
Why not?

00:30:55.580 --> 00:30:57.120 align:middle line:90%
I can think of two reasons.

00:30:57.120 --> 00:31:00.080 align:middle line:84%
You think about
reasons why, even

00:31:00.080 --> 00:31:01.980 align:middle line:90%
in purely unidirectional flow--

00:31:01.980 --> 00:31:03.920 align:middle line:84%
Do you remember I
told you that, because

00:31:03.920 --> 00:31:07.620 align:middle line:84%
of the asymmetry of the
oscillation, fast and strong,

00:31:07.620 --> 00:31:11.060 align:middle line:84%
one way, slow and weak the other
way to make an oscillation?

00:31:11.060 --> 00:31:13.800 align:middle line:84%
So the sediment transport
rate and shoaling waves

00:31:13.800 --> 00:31:15.240 align:middle line:90%
is toward the beach.

00:31:15.240 --> 00:31:18.400 align:middle line:84%
And so that could cause
the ripples to climb

00:31:18.400 --> 00:31:23.160 align:middle line:90%
at some non-vertical angle.

00:31:23.160 --> 00:31:26.575 align:middle line:90%
And that's very common.

00:31:26.575 --> 00:31:28.200 align:middle line:84%
The other is, of
course, you can always

00:31:28.200 --> 00:31:30.218 align:middle line:84%
have a slight unidirectional
flow component.

00:31:30.218 --> 00:31:31.760 align:middle line:84%
And how would you
tell the difference

00:31:31.760 --> 00:31:34.218 align:middle line:90%
between the one and the other?

00:31:34.218 --> 00:31:34.760 align:middle line:90%
I don't know.

00:31:34.760 --> 00:31:37.440 align:middle line:84%
Maybe other things
about the section

00:31:37.440 --> 00:31:39.620 align:middle line:84%
might be able to
tip you off on that.

00:31:39.620 --> 00:31:41.600 align:middle line:84%
But it's not an easy
thing to deal with.

00:31:41.600 --> 00:31:43.020 align:middle line:90%
I showed you this before.

00:31:43.020 --> 00:31:46.240 align:middle line:84%
This is from the Wappinger
Cambrian in New York,

00:31:46.240 --> 00:31:48.360 align:middle line:90%
in the Hudson Valley.

00:31:48.360 --> 00:31:51.540 align:middle line:84%
And it's pretty clear
they're oscillation ripples.

00:31:51.540 --> 00:31:54.240 align:middle line:84%
But they're moving because you
can see the laminae inside them.

00:31:54.240 --> 00:31:57.940 align:middle line:84%
Almost symmetrical,
but they're shifting.

00:31:57.940 --> 00:32:00.400 align:middle line:84%
Another example, close-up,
the same kind of thing.

00:32:00.400 --> 00:32:03.860 align:middle line:84%
We can be pretty sure
they're oscillation ripples.

00:32:03.860 --> 00:32:05.740 align:middle line:84%
This is one of the
few places I've ever

00:32:05.740 --> 00:32:09.260 align:middle line:84%
seen where the ripples really
are climbing vertically

00:32:09.260 --> 00:32:10.580 align:middle line:90%
for a long distance.

00:32:10.580 --> 00:32:12.420 align:middle line:84%
Now, it's not a
matter of draping,

00:32:12.420 --> 00:32:15.100 align:middle line:84%
because if they were draped,
they'd die out much more rapidly

00:32:15.100 --> 00:32:15.760 align:middle line:90%
upward.

00:32:15.760 --> 00:32:17.820 align:middle line:84%
So these really are,
whatever the environment

00:32:17.820 --> 00:32:21.020 align:middle line:84%
is, whatever the oscillatory
environment is, they're

00:32:21.020 --> 00:32:23.740 align:middle line:90%
climbing almost vertically.

00:32:23.740 --> 00:32:25.820 align:middle line:90%
But I've seldom seen that.

00:32:25.820 --> 00:32:28.820 align:middle line:84%
Here's another example
from the Ferron in Utah.

00:32:28.820 --> 00:32:31.100 align:middle line:84%
And they're climbing at
a pretty steep angle,

00:32:31.100 --> 00:32:34.007 align:middle line:90%
but that's very uncommon.

00:32:34.007 --> 00:32:35.840 align:middle line:84%
It's more common to see
something like this.

00:32:35.840 --> 00:32:37.660 align:middle line:84%
They're clearly
oscillation ripples.

00:32:37.660 --> 00:32:41.020 align:middle line:90%
They're depositional stoss.

00:32:41.020 --> 00:32:46.020 align:middle line:84%
And in this case,
their angle of climb

00:32:46.020 --> 00:32:49.540 align:middle line:84%
suggests that it's because
it's combined flow, rather than

00:32:49.540 --> 00:32:53.700 align:middle line:90%
a purely unidirectional flow.

00:32:53.700 --> 00:32:55.710 align:middle line:84%
This is one of my
favorite photographs.

00:32:55.710 --> 00:32:59.230 align:middle line:90%
It's also from the Moenkopi.

00:32:59.230 --> 00:33:01.050 align:middle line:84%
So there they are,
climbing, climbing,

00:33:01.050 --> 00:33:04.630 align:middle line:84%
climbing, for a long distance
throughout this deposition

00:33:04.630 --> 00:33:05.250 align:middle line:90%
of the bed.

00:33:05.250 --> 00:33:07.750 align:middle line:84%
Flow conditions stayed pretty
much the same for a long time,

00:33:07.750 --> 00:33:08.610 align:middle line:90%
in that case.

00:33:08.610 --> 00:33:11.310 align:middle line:90%


00:33:11.310 --> 00:33:13.830 align:middle line:84%
I showed you this already,
and I mentioned to you

00:33:13.830 --> 00:33:16.930 align:middle line:84%
that it looks fishy
to be current ripples.

00:33:16.930 --> 00:33:24.670 align:middle line:84%
And I'm pretty sure that's it's
either oscillation influenced,

00:33:24.670 --> 00:33:27.750 align:middle line:84%
as well as
unidirectional influence

00:33:27.750 --> 00:33:32.750 align:middle line:90%
at a medium angle of climb.

00:33:32.750 --> 00:33:34.510 align:middle line:90%
That's a close-up.

00:33:34.510 --> 00:33:38.692 align:middle line:84%
So you can see exactly
what I'm talking about.

00:33:38.692 --> 00:33:40.150 align:middle line:84%
I think I showed
you this, too, now

00:33:40.150 --> 00:33:41.750 align:middle line:84%
that we're coming
to unidirectional

00:33:41.750 --> 00:33:43.190 align:middle line:90%
versus oscillatory.

00:33:43.190 --> 00:33:48.270 align:middle line:84%
I'm guessing that's in between
oscillatory unidirectional

00:33:48.270 --> 00:33:49.090 align:middle line:90%
influence.

00:33:49.090 --> 00:33:50.670 align:middle line:90%
That's my guess.

00:33:50.670 --> 00:33:53.880 align:middle line:84%
But I can't pin it down
particularly, either.

00:33:53.880 --> 00:33:59.840 align:middle line:84%
All right, now, I'm
dealing with how

00:33:59.840 --> 00:34:02.280 align:middle line:84%
you can tell between
unidirectional flow,

00:34:02.280 --> 00:34:05.720 align:middle line:84%
depositional source, climbing
ripple, and combined flow

00:34:05.720 --> 00:34:07.840 align:middle line:84%
climbing ripples
without erosion.

00:34:07.840 --> 00:34:10.800 align:middle line:84%
And the only thing I can think
of is try to look at the profile

00:34:10.800 --> 00:34:13.480 align:middle line:84%
and see whether it looks like
unidirectional flow ripples

00:34:13.480 --> 00:34:15.020 align:middle line:90%
or oscillatory flow ripples.

00:34:15.020 --> 00:34:20.179 align:middle line:84%
And when you have deposition
in the stoss, on the stoss,

00:34:20.179 --> 00:34:24.120 align:middle line:84%
as well as in the
lee, you can do that.

00:34:24.120 --> 00:34:27.679 align:middle line:84%
But it's not all that common
to be able to do that.

00:34:27.679 --> 00:34:32.105 align:middle line:84%
So is this combined flow, or
is it unidirectional flow?

00:34:32.105 --> 00:34:33.480 align:middle line:84%
And you look at
it, and from what

00:34:33.480 --> 00:34:35.219 align:middle line:84%
I've said, oh, that's
unidirectional--

00:34:35.219 --> 00:34:37.040 align:middle line:84%
that's unidirectional
flow climbing

00:34:37.040 --> 00:34:38.540 align:middle line:90%
ripple cross-stratification.

00:34:38.540 --> 00:34:40.479 align:middle line:84%
But from what I've
just said, you

00:34:40.479 --> 00:34:43.800 align:middle line:84%
have the suspicion that
maybe it's combined flow.

00:34:43.800 --> 00:34:45.760 align:middle line:84%
And I don't see
any way of telling.

00:34:45.760 --> 00:34:48.420 align:middle line:84%
And yet, combined flow
features must be pretty common,

00:34:48.420 --> 00:34:51.340 align:middle line:84%
which I'm going to talk about
soon if I have the time.

00:34:51.340 --> 00:34:56.460 align:middle line:84%
Here's another example from
the Moenkopi, same problem.

00:34:56.460 --> 00:34:59.000 align:middle line:84%
It's nice to think that it's
always unidirectional flow,

00:34:59.000 --> 00:35:00.480 align:middle line:84%
but it doesn't have
to be that way.

00:35:00.480 --> 00:35:03.540 align:middle line:90%


00:35:03.540 --> 00:35:06.860 align:middle line:84%
And the other thing is, we
see climbing oscillatory flow

00:35:06.860 --> 00:35:07.420 align:middle line:90%
bedforms.

00:35:07.420 --> 00:35:11.500 align:middle line:84%
And they're usually on a small
scale, not on a large scale.

00:35:11.500 --> 00:35:13.820 align:middle line:84%
And I'm going to get to
that presently when we talk

00:35:13.820 --> 00:35:18.740 align:middle line:90%
about combined flow features.

00:35:18.740 --> 00:35:22.460 align:middle line:84%
So I'm going to
repeat a slide that I

00:35:22.460 --> 00:35:28.020 align:middle line:84%
showed last time, a graph, a
diagram, that you may remember.

00:35:28.020 --> 00:35:32.600 align:middle line:84%
And it's orbital velocity
versus oscillation period.

00:35:32.600 --> 00:35:34.480 align:middle line:84%
And you can see that
in the lower left,

00:35:34.480 --> 00:35:42.100 align:middle line:90%
this is for weak flows.

00:35:42.100 --> 00:35:44.247 align:middle line:84%
The ripples are
small, and they're

00:35:44.247 --> 00:35:46.080 align:middle line:84%
three-dimensional--
they're two-dimensional.

00:35:46.080 --> 00:35:48.420 align:middle line:84%
But above this line,
they become larger,

00:35:48.420 --> 00:35:50.230 align:middle line:84%
and they become
three-dimensional.

00:35:50.230 --> 00:35:54.830 align:middle line:84%
Now, so it's down in here that
we usually see these small scale

00:35:54.830 --> 00:35:55.770 align:middle line:90%
oscillation ripples.

00:35:55.770 --> 00:35:57.030 align:middle line:90%
And they're understandable.

00:35:57.030 --> 00:36:02.030 align:middle line:84%
But this is-- it's not
exactly terra incognita,

00:36:02.030 --> 00:36:03.550 align:middle line:90%
but it's close to it.

00:36:03.550 --> 00:36:06.005 align:middle line:84%
And we know the bedforms
exist because they've

00:36:06.005 --> 00:36:07.630 align:middle line:84%
been observed in many
flume experiments

00:36:07.630 --> 00:36:09.330 align:middle line:84%
and in some natural
environments.

00:36:09.330 --> 00:36:11.070 align:middle line:84%
And we know they're
three-dimensional.

00:36:11.070 --> 00:36:13.930 align:middle line:84%
So what kind of stratification
do they present?

00:36:13.930 --> 00:36:16.550 align:middle line:90%


00:36:16.550 --> 00:36:18.910 align:middle line:84%
That's where we get the
hummocky cross-stratification.

00:36:18.910 --> 00:36:24.350 align:middle line:84%
This is a term that's been
around since the 1970s.

00:36:24.350 --> 00:36:26.110 align:middle line:84%
It's a kind of medium
scale to large scale

00:36:26.110 --> 00:36:28.430 align:middle line:84%
cross-stratification,
which I think,

00:36:28.430 --> 00:36:29.990 align:middle line:84%
and I think most
people think, it's

00:36:29.990 --> 00:36:32.850 align:middle line:84%
produced by oscillatory
bedforms during aggregation.

00:36:32.850 --> 00:36:35.150 align:middle line:84%
But they're large in
a three-dimensional.

00:36:35.150 --> 00:36:39.270 align:middle line:90%


00:36:39.270 --> 00:36:43.470 align:middle line:84%
Aggradation in the presence of
3D large oscillation ripples

00:36:43.470 --> 00:36:47.050 align:middle line:84%
and what we're
dealing with here.

00:36:47.050 --> 00:36:49.410 align:middle line:84%
It's been controversial,
but the general belief

00:36:49.410 --> 00:36:52.670 align:middle line:84%
is it's purely
oscillation-dominant flow.

00:36:52.670 --> 00:36:55.750 align:middle line:84%
I showed you my favorite
outcrop last time.

00:36:55.750 --> 00:36:59.690 align:middle line:84%
Remember that 45 degree
dipping bedding surface,

00:36:59.690 --> 00:37:02.330 align:middle line:84%
where the hummocky-- where the
hummocks and swales arranged

00:37:02.330 --> 00:37:02.950 align:middle line:90%
around it.

00:37:02.950 --> 00:37:04.350 align:middle line:90%
And they're all very isotropic.

00:37:04.350 --> 00:37:06.370 align:middle line:84%
They're not moving in
one direction or another.

00:37:06.370 --> 00:37:08.890 align:middle line:90%
And so we know that happens.

00:37:08.890 --> 00:37:11.050 align:middle line:84%
It was a purely
oscillatory flow produced

00:37:11.050 --> 00:37:14.210 align:middle line:84%
these large, three-dimensional
hummocky valley bed

00:37:14.210 --> 00:37:15.570 align:middle line:90%
configurations.

00:37:15.570 --> 00:37:19.130 align:middle line:84%
And I wish that I had
gone around the corner

00:37:19.130 --> 00:37:22.610 align:middle line:84%
and taken a picture of the
section through that bed.

00:37:22.610 --> 00:37:24.470 align:middle line:84%
We saw only the
top surface of it.

00:37:24.470 --> 00:37:28.030 align:middle line:84%
And it was classic, medium-scale
hummocky cross-stratification.

00:37:28.030 --> 00:37:30.410 align:middle line:84%
So that tips me off
that maybe everything

00:37:30.410 --> 00:37:34.130 align:middle line:90%
we're talking about across--

00:37:34.130 --> 00:37:36.890 align:middle line:84%
everything we're talking
about, oscillatory flow

00:37:36.890 --> 00:37:40.970 align:middle line:84%
cross-stratification, involves
large 3D bedforms aggrading

00:37:40.970 --> 00:37:42.150 align:middle line:90%
in various ways.

00:37:42.150 --> 00:37:43.910 align:middle line:84%
And I'm going to go
through some slides.

00:37:43.910 --> 00:37:47.340 align:middle line:84%
I might not get to combine
flow features right now.

00:37:47.340 --> 00:37:51.340 align:middle line:90%


00:37:51.340 --> 00:37:55.540 align:middle line:84%
Irregular shifting,
but isotropic shifting.

00:37:55.540 --> 00:37:58.220 align:middle line:84%
Now, there's a term swaly
cross-stratification.

00:37:58.220 --> 00:38:00.120 align:middle line:84%
They usually spell it
with an E in there,

00:38:00.120 --> 00:38:02.140 align:middle line:84%
and I don't like that,
because it's like shaly.

00:38:02.140 --> 00:38:05.340 align:middle line:84%
We spell chailey without
the E. But anyway--

00:38:05.340 --> 00:38:07.060 align:middle line:84%
and they think of it
as something else,

00:38:07.060 --> 00:38:08.520 align:middle line:90%
SCS instead of HDS.

00:38:08.520 --> 00:38:12.140 align:middle line:84%
To me, there's a gradation
between SCS and HCS

00:38:12.140 --> 00:38:14.300 align:middle line:84%
depending on the
rate of aggradation

00:38:14.300 --> 00:38:16.440 align:middle line:84%
relative to the shifting
of the bedforms.

00:38:16.440 --> 00:38:18.140 align:middle line:84%
If the rate of
aggradation is slow

00:38:18.140 --> 00:38:19.940 align:middle line:84%
and they're acting
that way, you're

00:38:19.940 --> 00:38:22.020 align:middle line:84%
going to see lots
of trough fillings

00:38:22.020 --> 00:38:23.980 align:middle line:84%
and very little
by way of swales.

00:38:23.980 --> 00:38:25.960 align:middle line:84%
But for a higher
rate of aggradation,

00:38:25.960 --> 00:38:28.440 align:middle line:84%
you're going to see not
just erosion in the troughs,

00:38:28.440 --> 00:38:32.840 align:middle line:84%
but you also see deposition
over the crest of the swales.

00:38:32.840 --> 00:38:34.800 align:middle line:84%
This is the classic
block diagram.

00:38:34.800 --> 00:38:39.140 align:middle line:84%
We gave a short course way back
in 1975, John Harms was the one.

00:38:39.140 --> 00:38:40.760 align:middle line:90%
He originated this term.

00:38:40.760 --> 00:38:44.720 align:middle line:84%
He was the first to perceive
that it's a distinctive style

00:38:44.720 --> 00:38:46.300 align:middle line:90%
of cross-stratification.

00:38:46.300 --> 00:38:48.240 align:middle line:84%
And he thought about
how it would happen.

00:38:48.240 --> 00:38:52.040 align:middle line:84%
And in later years,
he would say,

00:38:52.040 --> 00:38:55.400 align:middle line:84%
there are people nowadays who
make their careers out of HCS.

00:38:55.400 --> 00:38:57.280 align:middle line:84%
But he was the one
who started it.

00:38:57.280 --> 00:39:01.280 align:middle line:84%
It's an illustration of
that there's a saying,

00:39:01.280 --> 00:39:03.280 align:middle line:84%
I wouldn't have believed
it if I hadn't seen it.

00:39:03.280 --> 00:39:05.405 align:middle line:84%
You can reverse it and say,
I wouldn't have seen it

00:39:05.405 --> 00:39:06.680 align:middle line:90%
if I hadn't believed it.

00:39:06.680 --> 00:39:08.560 align:middle line:84%
Everybody was seeing
HCS, but they never

00:39:08.560 --> 00:39:11.920 align:middle line:84%
gave any particular credence
or significance to it

00:39:11.920 --> 00:39:14.240 align:middle line:84%
until somebody, Harms,
came along and realized

00:39:14.240 --> 00:39:16.980 align:middle line:84%
this is a very specific
kind of depositional model.

00:39:16.980 --> 00:39:18.580 align:middle line:90%
So that's what HDS is now.

00:39:18.580 --> 00:39:21.720 align:middle line:84%
And everybody is seeing it,
whereas nobody saw it before.

00:39:21.720 --> 00:39:24.160 align:middle line:84%
And one of the prime
characteristics

00:39:24.160 --> 00:39:27.840 align:middle line:84%
is you have places where
conformable laminae end up

00:39:27.840 --> 00:39:30.640 align:middle line:84%
going into a truncation
surface and then maybe back

00:39:30.640 --> 00:39:31.860 align:middle line:90%
out into conformity.

00:39:31.860 --> 00:39:32.760 align:middle line:90%
That's if you see--

00:39:32.760 --> 00:39:37.090 align:middle line:84%
that's a tip off that
we're dealing with HCS.

00:39:37.090 --> 00:39:38.340 align:middle line:90%
That's what I just showed you.

00:39:38.340 --> 00:39:41.000 align:middle line:84%
But also, we see
places where hummocks

00:39:41.000 --> 00:39:43.140 align:middle line:84%
turn into swales
during deposition

00:39:43.140 --> 00:39:45.340 align:middle line:84%
and where swales
turn into hummocks.

00:39:45.340 --> 00:39:46.720 align:middle line:90%
I got that right-- yeah, right.

00:39:46.720 --> 00:39:48.040 align:middle line:90%
That's very characteristic.

00:39:48.040 --> 00:39:50.040 align:middle line:84%
And I can show you some
photos pretty soon.

00:39:50.040 --> 00:39:50.920 align:middle line:90%
Let's ignore this.

00:39:50.920 --> 00:39:53.980 align:middle line:84%
This was an attempt on
my part, some years ago,

00:39:53.980 --> 00:39:58.980 align:middle line:84%
to organize everything about
HCS and other oscillatory

00:39:58.980 --> 00:40:00.660 align:middle line:90%
flow, large scale bedforms.

00:40:00.660 --> 00:40:03.420 align:middle line:84%
It doesn't quite work, because
I can't draw the sketch as well.

00:40:03.420 --> 00:40:05.867 align:middle line:84%
And I invite you to look at
it if you want to look at it.

00:40:05.867 --> 00:40:07.200 align:middle line:90%
So let's get on to other things.

00:40:07.200 --> 00:40:10.860 align:middle line:84%
OK, here's the swale
going to a hummock.

00:40:10.860 --> 00:40:12.820 align:middle line:90%
It happens.

00:40:12.820 --> 00:40:17.980 align:middle line:84%
Here's a hummock growing from
a flat surface, planar surface.

00:40:17.980 --> 00:40:23.580 align:middle line:84%
Here's a nice, big, broad
hummock all by itself.

00:40:23.580 --> 00:40:25.440 align:middle line:84%
Here's a swale
going into planar.

00:40:25.440 --> 00:40:29.260 align:middle line:90%


00:40:29.260 --> 00:40:34.340 align:middle line:84%
Here's a hummock going into
a swale with the same kind

00:40:34.340 --> 00:40:37.500 align:middle line:84%
of thing-- from
conformable to truncation

00:40:37.500 --> 00:40:39.270 align:middle line:90%
to conformable over there.

00:40:39.270 --> 00:40:40.690 align:middle line:90%
That's another tip off.

00:40:40.690 --> 00:40:43.847 align:middle line:84%
When you see that kind of thing,
you must be dealing with HCS.

00:40:43.847 --> 00:40:45.430 align:middle line:84%
There's a hummock
going into-- there's

00:40:45.430 --> 00:40:49.190 align:middle line:90%
a swale going into a hummock.

00:40:49.190 --> 00:40:53.950 align:middle line:84%
And a hummock going into
a swale with erosion,

00:40:53.950 --> 00:40:56.250 align:middle line:84%
trailing off into
conformity over that way.

00:40:56.250 --> 00:40:57.370 align:middle line:90%
That's very common.

00:40:57.370 --> 00:41:00.510 align:middle line:90%


00:41:00.510 --> 00:41:02.470 align:middle line:84%
I carried this out
of the Wood Canyon

00:41:02.470 --> 00:41:06.130 align:middle line:84%
Formation in the Southern
end of the Nopah range once.

00:41:06.130 --> 00:41:07.990 align:middle line:90%
And it's not that big.

00:41:07.990 --> 00:41:09.790 align:middle line:84%
It was heavy, but I
could carry it out.

00:41:09.790 --> 00:41:12.350 align:middle line:84%
It shows medium
scale, hummocky swale

00:41:12.350 --> 00:41:14.052 align:middle line:90%
topography on the bed surface.

00:41:14.052 --> 00:41:15.510 align:middle line:84%
This is from the
Wood Canyon, right

00:41:15.510 --> 00:41:17.870 align:middle line:84%
at the precambrian-cambrian
boundary.

00:41:17.870 --> 00:41:20.330 align:middle line:84%
And although you can't see
it very well in this picture,

00:41:20.330 --> 00:41:23.830 align:middle line:84%
it shows medium scale
hummocky cross-stratification.

00:41:23.830 --> 00:41:26.312 align:middle line:84%
I was going to bring
it, but I can't find it.

00:41:26.312 --> 00:41:28.270 align:middle line:84%
It's somewhere around
the house or in the barn,

00:41:28.270 --> 00:41:29.490 align:middle line:90%
and I couldn't find it.

00:41:29.490 --> 00:41:32.750 align:middle line:84%
But it's one of my
prized possessions.

00:41:32.750 --> 00:41:36.290 align:middle line:84%
Here's a better view of
the cross-stratification,

00:41:36.290 --> 00:41:40.960 align:middle line:84%
which looked like medium-scale
cross-stratification.

00:41:40.960 --> 00:41:43.520 align:middle line:84%
This is the classic
John Harms photo

00:41:43.520 --> 00:41:44.860 align:middle line:90%
when he developed the concept.

00:41:44.860 --> 00:41:47.580 align:middle line:84%
He showed this photo in
the short course we gave.

00:41:47.580 --> 00:41:50.280 align:middle line:90%


00:41:50.280 --> 00:41:51.860 align:middle line:90%
This is very characteristic.

00:41:51.860 --> 00:41:55.040 align:middle line:84%
You can see truncation
surfaces going into conformity

00:41:55.040 --> 00:41:58.815 align:middle line:84%
and being overtopped
by another hummock.

00:41:58.815 --> 00:41:59.940 align:middle line:90%
This is pretty large-scale.

00:41:59.940 --> 00:42:00.982 align:middle line:90%
I mean, this is 6-inches.

00:42:00.982 --> 00:42:03.800 align:middle line:84%
So this is, like,
this is meter plus

00:42:03.800 --> 00:42:07.400 align:middle line:90%
scale we're dealing with here.

00:42:07.400 --> 00:42:09.960 align:middle line:84%
Same kind of thing-- look
at this, conformability

00:42:09.960 --> 00:42:13.760 align:middle line:84%
into truncation and then back
into conformity over here

00:42:13.760 --> 00:42:15.760 align:middle line:84%
because of the way those
hummocks and swales are

00:42:15.760 --> 00:42:17.180 align:middle line:90%
interacting with one another.

00:42:17.180 --> 00:42:20.920 align:middle line:90%


00:42:20.920 --> 00:42:23.800 align:middle line:84%
A swale overtopped by a
hummock and another hummock

00:42:23.800 --> 00:42:29.740 align:middle line:84%
on top with that same erosion
surface, truncation going on.

00:42:29.740 --> 00:42:33.160 align:middle line:90%


00:42:33.160 --> 00:42:36.260 align:middle line:90%
Even more classic HCS--

00:42:36.260 --> 00:42:39.460 align:middle line:84%
conformability into
truncation, and probably back

00:42:39.460 --> 00:42:41.700 align:middle line:90%
to conformability over there.

00:42:41.700 --> 00:42:43.780 align:middle line:84%
When you see that,
that's a tip-off.

00:42:43.780 --> 00:42:47.180 align:middle line:84%
This is from the Johnnie
formation in the Nopah range

00:42:47.180 --> 00:42:48.300 align:middle line:90%
in California.

00:42:48.300 --> 00:42:51.120 align:middle line:84%
And a lot of indistinct
planar lamination,

00:42:51.120 --> 00:42:52.800 align:middle line:84%
but then it got
hummocky and swaley.

00:42:52.800 --> 00:42:55.100 align:middle line:84%
But then it stopped
over top, I guess

00:42:55.100 --> 00:42:57.480 align:middle line:84%
I should say, by planar
lamination again.

00:42:57.480 --> 00:43:00.180 align:middle line:84%
As the current velocity
changes, as the water

00:43:00.180 --> 00:43:04.740 align:middle line:84%
flow velocity changes, you
can go from one to the other.

00:43:04.740 --> 00:43:08.200 align:middle line:84%
This is more like what they call
swaley cross-stratification.

00:43:08.200 --> 00:43:11.960 align:middle line:84%
You see a fair number of
hummocky-looking features,

00:43:11.960 --> 00:43:13.220 align:middle line:90%
shallow features.

00:43:13.220 --> 00:43:15.840 align:middle line:84%
And it doesn't look much
like what I just showed you,

00:43:15.840 --> 00:43:17.860 align:middle line:84%
because I think the
aggradation rate is low

00:43:17.860 --> 00:43:21.100 align:middle line:84%
relative to how fast these
things are shifting around.

00:43:21.100 --> 00:43:24.100 align:middle line:84%
That's my that's my colleague,
Roger Walker, explaining

00:43:24.100 --> 00:43:30.660 align:middle line:84%
swaley cross-stratification to
a bunch of students long ago.

00:43:30.660 --> 00:43:33.670 align:middle line:84%
And I guess this is HCS,
too, on a small scale-- very

00:43:33.670 --> 00:43:35.530 align:middle line:90%
small scale, medium scale.

00:43:35.530 --> 00:43:38.430 align:middle line:90%


00:43:38.430 --> 00:43:41.310 align:middle line:84%
Look at that big
hummock, same kind

00:43:41.310 --> 00:43:46.412 align:middle line:84%
of features going on there that
we've seen before close up.

00:43:46.412 --> 00:43:48.870 align:middle line:84%
This is interesting, because
there's pretty deep scour over

00:43:48.870 --> 00:43:50.690 align:middle line:90%
here that truncated this stuff.

00:43:50.690 --> 00:43:56.270 align:middle line:84%
And it got overtopped by this
and goes to conformity again.

00:43:56.270 --> 00:43:57.630 align:middle line:90%
And I tell you--

00:43:57.630 --> 00:44:01.450 align:middle line:84%
I've told you some things about
combined-flow stratification,

00:44:01.450 --> 00:44:03.420 align:middle line:84%
but I want to just show
you a couple of slides.

00:44:03.420 --> 00:44:04.670 align:middle line:90%
You can look at them yourself.

00:44:04.670 --> 00:44:05.770 align:middle line:90%
You've seen this before.

00:44:05.770 --> 00:44:09.030 align:middle line:84%
This is from Simon
Dumas' experiments

00:44:09.030 --> 00:44:11.270 align:middle line:84%
over in the laboratory
in building N9.

00:44:11.270 --> 00:44:13.630 align:middle line:90%
And these lines are fakey.

00:44:13.630 --> 00:44:16.190 align:middle line:84%
These are all gradational--
symmetric small,

00:44:16.190 --> 00:44:19.470 align:middle line:84%
symmetric large, asymmetric
small, asymmetric large.

00:44:19.470 --> 00:44:21.870 align:middle line:84%
And so this is
purely oscillatory.

00:44:21.870 --> 00:44:23.250 align:middle line:90%
That's purely unidirectional.

00:44:23.250 --> 00:44:26.530 align:middle line:84%
And look at this broad range
of possibilities in between.

00:44:26.530 --> 00:44:27.870 align:middle line:90%
It's a jungle.

00:44:27.870 --> 00:44:29.590 align:middle line:84%
I mean, in Grotzinger's
terminology,

00:44:29.590 --> 00:44:32.550 align:middle line:90%
the dog's breakfast.

00:44:32.550 --> 00:44:37.210 align:middle line:84%
And we don't know as much about
combined poststratification

00:44:37.210 --> 00:44:40.930 align:middle line:84%
as with the more classical
unidirectional flow

00:44:40.930 --> 00:44:43.250 align:middle line:84%
and oscillatory
flow classification.

00:44:43.250 --> 00:44:45.490 align:middle line:90%
Progress has been slow.

00:44:45.490 --> 00:44:48.170 align:middle line:84%
Unless I missed some
very recent papers,

00:44:48.170 --> 00:44:52.530 align:middle line:84%
Nobody has really come to grips
with the whole systematics

00:44:52.530 --> 00:44:55.290 align:middle line:90%
of these intermediate features.

00:44:55.290 --> 00:44:57.170 align:middle line:84%
But they must be
important out there,

00:44:57.170 --> 00:45:00.370 align:middle line:84%
because it can't always be
purely unidirectional, purely

00:45:00.370 --> 00:45:00.870 align:middle line:90%
oscillatory.

00:45:00.870 --> 00:45:02.290 align:middle line:90%
There must be combinations.

00:45:02.290 --> 00:45:05.150 align:middle line:84%
And as I told you when we
dealt with bed configuration,

00:45:05.150 --> 00:45:07.050 align:middle line:84%
combined flow bed
configurations,

00:45:07.050 --> 00:45:08.672 align:middle line:84%
there's a wide range
of possibilities.

00:45:08.672 --> 00:45:10.130 align:middle line:84%
And when they're
grades, it's going

00:45:10.130 --> 00:45:12.630 align:middle line:84%
to produce a wide range
of cross stratification.

00:45:12.630 --> 00:45:14.050 align:middle line:84%
And we've only
begun to understand

00:45:14.050 --> 00:45:15.970 align:middle line:84%
how we recognize
where we would be

00:45:15.970 --> 00:45:19.050 align:middle line:84%
in this vast sea
of possibilities.

00:45:19.050 --> 00:45:21.410 align:middle line:84%
And I think that's
probably about all I have.

00:45:21.410 --> 00:45:26.470 align:middle line:90%
This is from Simon Dumas' paper.

00:45:26.470 --> 00:45:32.710 align:middle line:84%
And you can see this--
concentrate on small scale bed

00:45:32.710 --> 00:45:37.770 align:middle line:84%
forms with mainly oscillatory,
but partly unidirectional.

00:45:37.770 --> 00:45:39.412 align:middle line:84%
And it's a very
three-dimensional.

00:45:39.412 --> 00:45:40.870 align:middle line:84%
And when they
agrade, they're going

00:45:40.870 --> 00:45:42.995 align:middle line:84%
to leave a particular kind
of cross-stratification.

00:45:42.995 --> 00:45:46.210 align:middle line:84%
And I'm not sure what it's
going to look like, frankly.

00:45:46.210 --> 00:45:51.550 align:middle line:90%


00:45:51.550 --> 00:45:53.550 align:middle line:84%
All right, this is going
to be the last slide

00:45:53.550 --> 00:45:56.950 align:middle line:84%
here, a bunch of
things to say about how

00:45:56.950 --> 00:45:59.110 align:middle line:90%
you make interpretations.

00:45:59.110 --> 00:46:01.230 align:middle line:84%
Now, if you have vertical
climb, asymmetric, you

00:46:01.230 --> 00:46:03.750 align:middle line:84%
know it's oscillatory
flow right.

00:46:03.750 --> 00:46:07.010 align:middle line:84%
If you have depositional stoss
climb of asymmetrical ripples,

00:46:07.010 --> 00:46:08.510 align:middle line:84%
you have to look
at the ripple shape

00:46:08.510 --> 00:46:11.070 align:middle line:84%
and try to back out,
whether it's combined

00:46:11.070 --> 00:46:14.943 align:middle line:90%
flow or unidirectional flow.

00:46:14.943 --> 00:46:17.110 align:middle line:84%
STUDENT: Does that have to
do with [INAUDIBLE], when

00:46:17.110 --> 00:46:19.490 align:middle line:84%
you say look at shape,
do you mean concavity?

00:46:19.490 --> 00:46:23.270 align:middle line:84%
JOHN SOUTHARD: Well,
the shape of the ripple

00:46:23.270 --> 00:46:25.570 align:middle line:84%
that you can see
in the structure,

00:46:25.570 --> 00:46:27.310 align:middle line:84%
to some-- you can
always see that.

00:46:27.310 --> 00:46:29.260 align:middle line:84%
At low angles of climb,
you don't know that.

00:46:29.260 --> 00:46:31.400 align:middle line:84%
And I think that's
mentioned here.

00:46:31.400 --> 00:46:35.240 align:middle line:84%
When it's erosional stoss,
very asymmetrical ripples.

00:46:35.240 --> 00:46:38.340 align:middle line:84%
It's probably
unidirectional flow,

00:46:38.340 --> 00:46:40.140 align:middle line:84%
but it may be not
purely oscillatory,

00:46:40.140 --> 00:46:41.680 align:middle line:90%
a unidirectional flow.

00:46:41.680 --> 00:46:45.320 align:middle line:84%
Isotropic HCS, on
a good sized scale,

00:46:45.320 --> 00:46:47.640 align:middle line:84%
it's almost certainly
oscillatory flow.

00:46:47.640 --> 00:46:49.300 align:middle line:90%
I've convinced myself of that.

00:46:49.300 --> 00:46:51.940 align:middle line:84%
I think the general
feeling is the truth.

00:46:51.940 --> 00:46:56.100 align:middle line:84%
If it's anisotropic HCS--
well, you see that sometimes.

00:46:56.100 --> 00:46:58.480 align:middle line:84%
But I haven't seen
it very often.

00:46:58.480 --> 00:47:03.240 align:middle line:84%
And that must be influenced
by unidirectional flow.

00:47:03.240 --> 00:47:05.320 align:middle line:84%
If you see large scale
trough stratification--

00:47:05.320 --> 00:47:06.960 align:middle line:90%
and I showed a lot of it--

00:47:06.960 --> 00:47:10.120 align:middle line:84%
we assume, when we look at
it, it's unidirectional flow.

00:47:10.120 --> 00:47:12.240 align:middle line:84%
But it may be
unidirectional flow

00:47:12.240 --> 00:47:13.980 align:middle line:90%
with an oscillation influence.

00:47:13.980 --> 00:47:16.500 align:middle line:84%
And we can't back out the
oscillation influence.

00:47:16.500 --> 00:47:20.760 align:middle line:84%
It's one of those things that
become difficult to manage.

00:47:20.760 --> 00:47:24.280 align:middle line:84%
And now there's a spectral gap
that I mentioned last time.

00:47:24.280 --> 00:47:27.400 align:middle line:84%
Ripples are always about
10, 15 centimeters,

00:47:27.400 --> 00:47:28.680 align:middle line:90%
thereabouts-- maybe 20.

00:47:28.680 --> 00:47:31.500 align:middle line:84%
And dunes seldom get
below a meter or half

00:47:31.500 --> 00:47:34.780 align:middle line:84%
meter at the least, unless
the flows are really shallow.

00:47:34.780 --> 00:47:42.220 align:middle line:84%
And so if we see
cross-stratification

00:47:42.220 --> 00:47:45.660 align:middle line:84%
that looks like it's scales
in that spectral gap,

00:47:45.660 --> 00:47:50.380 align:middle line:84%
we almost can conclude that it's
oscillatory flow because you

00:47:50.380 --> 00:47:52.460 align:middle line:84%
don't make oscillatory
flow ripples

00:47:52.460 --> 00:47:56.700 align:middle line:84%
in that spectrum, unidirectional
flow ripples in that gap.

00:47:56.700 --> 00:47:58.500 align:middle line:90%
So I'm going to quit there.

00:47:58.500 --> 00:48:02.340 align:middle line:84%
I had a few comments
about the fact

00:48:02.340 --> 00:48:06.780 align:middle line:84%
that many beds, a single event,
don't have uniform conditions

00:48:06.780 --> 00:48:07.400 align:middle line:90%
throughout.

00:48:07.400 --> 00:48:08.780 align:middle line:90%
I showed you some.

00:48:08.780 --> 00:48:11.180 align:middle line:84%
It can start slow and
go fast and start slow,

00:48:11.180 --> 00:48:12.200 align:middle line:90%
or the other way around.

00:48:12.200 --> 00:48:16.980 align:middle line:84%
And I had just a few slides
that aren't particularly needed

00:48:16.980 --> 00:48:18.060 align:middle line:90%
at this point.

00:48:18.060 --> 00:48:20.320 align:middle line:84%
So that's my pitch on
cross-stratification.

00:48:20.320 --> 00:48:22.460 align:middle line:84%
I've been a fan of
cross-stratification since I was

00:48:22.460 --> 00:48:27.230 align:middle line:84%
a grad student in
1960, early 1960s.

00:48:27.230 --> 00:48:31.910 align:middle line:84%
And it wasn't all that
well-understood at that time.

00:48:31.910 --> 00:48:34.750 align:middle line:84%
It wasn't totally
mysterious, but people

00:48:34.750 --> 00:48:36.668 align:middle line:84%
have made a lot of
progress up to now

00:48:36.668 --> 00:48:38.210 align:middle line:84%
in interpreting
cross-stratification.

00:48:38.210 --> 00:48:40.790 align:middle line:84%
And I've tried to
cover the ground rules,

00:48:40.790 --> 00:48:43.110 align:middle line:90%
cover the ground on that.

00:48:43.110 --> 00:48:46.830 align:middle line:90%
So that's my pitch.

00:48:46.830 --> 00:48:48.750 align:middle line:90%
[? Lyle. ?]

00:48:48.750 --> 00:48:51.230 align:middle line:84%
STUDENT: You showed a bunch
of different sizes of Hummocky

00:48:51.230 --> 00:48:52.510 align:middle line:90%
Cross-stratification, HCS.

00:48:52.510 --> 00:48:58.070 align:middle line:84%
What's the significance
of the size of HCS?

00:48:58.070 --> 00:48:59.450 align:middle line:84%
JOHN SOUTHARD: In
presentation 3,

00:48:59.450 --> 00:49:04.030 align:middle line:84%
I showed you my favorite
outcrop with a meter scale HCS.

00:49:04.030 --> 00:49:06.810 align:middle line:84%
And I showed you another
slide-- it wasn't a good one,

00:49:06.810 --> 00:49:10.350 align:middle line:84%
but it's the only
one I had-- of three,

00:49:10.350 --> 00:49:15.270 align:middle line:84%
four decimeter scale,
which must be common.

00:49:15.270 --> 00:49:19.730 align:middle line:84%
If the larger scale is common
and the smaller scale is common,

00:49:19.730 --> 00:49:21.760 align:middle line:84%
the intermediate scale
must be common, too,

00:49:21.760 --> 00:49:23.840 align:middle line:84%
judging from the
various experiments

00:49:23.840 --> 00:49:26.020 align:middle line:84%
of the kind that Simon
Dumas did and others.

00:49:26.020 --> 00:49:28.103 align:middle line:84%
There are a couple of
others' really good studies.

00:49:28.103 --> 00:49:31.520 align:middle line:84%
And I don't know how
to deal with that.

00:49:31.520 --> 00:49:34.000 align:middle line:84%
STUDENT: Does it have
to do with wave period?

00:49:34.000 --> 00:49:37.222 align:middle line:90%
Or what's controlling the--

00:49:37.222 --> 00:49:39.180 align:middle line:84%
JOHN SOUTHARD: Well, you
remember I mentioned--

00:49:39.180 --> 00:49:43.480 align:middle line:84%
I mentioned along the way, and I
showed you this dimensionless 3D

00:49:43.480 --> 00:49:48.920 align:middle line:84%
diagram of oscillatory flow
features and the fact that when

00:49:48.920 --> 00:49:52.360 align:middle line:84%
you make lab experiments, you
could fill any of that whole 3D

00:49:52.360 --> 00:49:54.000 align:middle line:90%
diagram with points.

00:49:54.000 --> 00:49:56.020 align:middle line:84%
But when you're dealing
with real waves,

00:49:56.020 --> 00:49:59.120 align:middle line:84%
there are certain constraints
on how the waves themselves work

00:49:59.120 --> 00:50:03.720 align:middle line:84%
that only some subset of space
in that 3D diagram can be

00:50:03.720 --> 00:50:07.920 align:middle line:84%
occupied by natural flow
oscillatory features.

00:50:07.920 --> 00:50:10.840 align:middle line:84%
I tried to make that
point, and it's generally

00:50:10.840 --> 00:50:12.600 align:middle line:90%
agreed that would be the case.

00:50:12.600 --> 00:50:14.507 align:middle line:84%
So is that relevant
to your question?

00:50:14.507 --> 00:50:15.340 align:middle line:90%
STUDENT: I think so.

00:50:15.340 --> 00:50:17.140 align:middle line:90%
Yeah, I don't know.

00:50:17.140 --> 00:50:22.580 align:middle line:84%
I think people, HCS is commonly
used as a storm [INAUDIBLE]

00:50:22.580 --> 00:50:25.000 align:middle line:84%
JOHN SOUTHARD: Yes, What
else-- what else could it be?

00:50:25.000 --> 00:50:26.000 align:middle line:90%
That's how I look at it.

00:50:26.000 --> 00:50:28.083 align:middle line:84%
STUDENT: And I'm just
wondering if there's further

00:50:28.083 --> 00:50:30.440 align:middle line:84%
you can go based on
the measuring the size,

00:50:30.440 --> 00:50:31.682 align:middle line:90%
like anything you can learn.

00:50:31.682 --> 00:50:33.140 align:middle line:84%
JOHN SOUTHARD:
Well, I did show you

00:50:33.140 --> 00:50:36.100 align:middle line:84%
a medium scale one, my
favorite little piece there.

00:50:36.100 --> 00:50:38.120 align:middle line:84%
And so I haven't
seen many like that.

00:50:38.120 --> 00:50:41.000 align:middle line:84%
And I don't know why it's scarce
compared to the larger scale.

00:50:41.000 --> 00:50:41.820 align:middle line:90%
I don't know that.

00:50:41.820 --> 00:50:43.740 align:middle line:84%
There's some reason
for that, and I haven't

00:50:43.740 --> 00:50:45.380 align:middle line:90%
come to grips with that.

00:50:45.380 --> 00:50:48.540 align:middle line:84%
But that's all I
can say about it.

00:50:48.540 --> 00:50:50.900 align:middle line:90%
Other questions, comments?

00:50:50.900 --> 00:50:53.420 align:middle line:84%
Thanks for staying
to the bitter end.

00:50:53.420 --> 00:50:55.420 align:middle line:84%
STUDENT: Could you mention
what that reference--

00:50:55.420 --> 00:50:57.080 align:middle line:90%
you had that reference for the--

00:50:57.080 --> 00:51:00.760 align:middle line:84%
I didn't quite write it down--
for the average set thickness.

00:51:00.760 --> 00:51:03.980 align:middle line:84%
JOHN SOUTHARD: Yes,
OK, Paola and Borgman--

00:51:03.980 --> 00:51:08.780 align:middle line:84%
well, you have the
PowerPoint, don't you?

00:51:08.780 --> 00:51:09.940 align:middle line:90%
And you can--

00:51:09.940 --> 00:51:11.300 align:middle line:90%
I don't know the reference.

00:51:11.300 --> 00:51:11.940 align:middle line:90%
We can go back.

00:51:11.940 --> 00:51:13.480 align:middle line:90%
It was 1990 something.

00:51:13.480 --> 00:51:14.260 align:middle line:90%
I don't remember.

00:51:14.260 --> 00:51:17.220 align:middle line:84%
STUDENT: Because Bill
Arnot told me that--

00:51:17.220 --> 00:51:18.810 align:middle line:90%
I was on a field trip with him.

00:51:18.810 --> 00:51:23.692 align:middle line:84%
He said he always assumes one
third of the bed thickness is--

00:51:23.692 --> 00:51:26.150 align:middle line:84%
JOHN SOUTHARD: Well, they seem
to think that it pretty much

00:51:26.150 --> 00:51:28.410 align:middle line:90%
scaled with the set thickness.

00:51:28.410 --> 00:51:30.290 align:middle line:90%
But read the paper.

00:51:30.290 --> 00:51:31.430 align:middle line:90%
I read it once.

00:51:31.430 --> 00:51:34.430 align:middle line:84%
I have to confess
it was only once.

00:51:34.430 --> 00:51:36.630 align:middle line:90%
And it seemed reasonable to me.

00:51:36.630 --> 00:51:39.490 align:middle line:84%
Bill Arnot is another close
younger colleague of mine.

00:51:39.490 --> 00:51:40.570 align:middle line:90%
I was on his thesis--

00:51:40.570 --> 00:51:42.570 align:middle line:84%
I was examiner on
his thesis committee.

00:51:42.570 --> 00:51:44.450 align:middle line:84%
Went to Edmonton
for his defense.

00:51:44.450 --> 00:51:46.170 align:middle line:90%
And then after, we drove down.

00:51:46.170 --> 00:51:49.173 align:middle line:84%
We were 400 some miles to
his field area in Montana,

00:51:49.173 --> 00:51:50.590 align:middle line:84%
had a great time
for a whole week.

00:51:50.590 --> 00:51:52.570 align:middle line:84%
So we've been a close
colleague ever since.

00:51:52.570 --> 00:51:55.550 align:middle line:84%
He and Paul Meyer are my
closest younger colleagues.

00:51:55.550 --> 00:51:58.740 align:middle line:90%
OK, so that's it.

00:51:58.740 --> 00:52:17.000 align:middle line:90%