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From YouTube: Xiaoning Wu CESM MOM6 Aqua and Ridge Planets
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A
Great,
so
thanks
everyone
for
being
here,
then
we've
got
a
great
introduction
via
Island
Scott
before
and
the
motivation
and
background
of
configuring
fully
coupled
Aqua
planets
and
other
simplified
geometries
without
within
the
CSM
framework
and
I'm
I'm
doing
I'm
enjoying
this
part
of
the
work
as
a
part
of
my
thesis,
research
and
the
work
has
been
done
with
a
lot
of
support
from
my
advisors,
Kevin
and
Chris,
and
as
well
as
a
long
list
of
collaborators.
I
see
many
of
you
in
the
audience.
A
So
a
big
shout
out
and
do
all
the
help
that
we
have
gotten
and
so
just
to
reiterate
what
Isla
has
already
mentioned:
the
motivation
for
kind
of
filling
in
the
Gap
in
the
hierarchy
of
simpler
models,
especially
in
the
couple
of
sense,
so
to
to
look
back
on
the
atmosphere
component
from
a
bit
as
I
introduced,
and
there
is
a
a
need,
higher
hierarchy
of
singular
models.
A
Several
simple
models
for
the
atmosphere
and
the
the
simplified
model,
just
like
sort
of
sitting
on
the
top
of
the
hierarchy
already
just
like
right.
Next
to
the
full
comprehension,
comprehensive
cam
is
a
an
atmospheric.
A
Only
Aqua
planet
that
that
has
the
full
sets
of
atmospheric
Dynamics
and
physics,
but
with
a
simplified
boundary
condition
in
the
term
in
terms
of
a
simplified
SSC
profile,
that's
typically
Zone
only
uniform
and
there
is
a
set
of
protocols
called
the
aquaplan
experiments
that
has
a
set
of
typically
used
curves
that
are
in
in
some
regards
idealizes
from
The
observed
real
world,
and
they
typically
have
the
SST
maximum
right
on
the
equator.
That's
what
we
get
from
The
Real
World,
and
we
will
look
at
that
a
bit
more
later.
A
What
happens
when
it's
coupled?
So
that's
on
the
atmospheric
side,
we
have
the
full
upper
planet
with
either
prescribed
or
a
slab
ocean
configuration
on
the
other
side
for
the
ocean
component.
A
There
is
also
a
long
history
of
idealized
configurations
used
both
for
model
development
and
for
investigating
some
of
the
fundamental
science
questions,
such
as
the
role
of
ocean
geometry
in
the
in
the
impacting
the
ocean
circulation
and
the
overall
climate
and
MIT
gcn
is
one
of
those
models.
That's
widely
used
for
this
kind
of
studies
which
and
gives
us
a
lot
of
insights.
A
You
can
see
it
as
a
slab
atmosphere,
so
both
of
these
components
or
both
sides
of
this
idealized
studies
do
tell
us
a
lot
of
important
science
information
and,
however,
if
we
want
to
look
at
the
other
end
of
the
Spectrum,
which
is
the
fully
coupled
semi-class
models
that
we
use
for
climate
assessments,
then
obviously
we
see
a
gap
between
these
kinds
of
compartments
types
and
idealized
models,
leading
up
to
the
fully
coupled
and
complex,
comprehensive
Earth
system
type
of
models.
A
And
that's
where
our
work
comes
in
in
the
in
the
regard
of
using
fully
carboxylate
plus
models,
but
with
idealized
configurations
in
terms
of
the
boundary
condition.
So
we
have
idealized
geometries,
that's
that's
both,
including
so
for
or
the
Quasi
Aqua
planet
and
idealize.
The
continents.
A
And
to.
A
To
show
one
of
those
aspects
which
could
be
investigated
by
this
kind
of
ideola
setups
include
the
impact
of
ocean
geometry
as
a
Meridian
or
heat
transport.
So
here
is
just
a
quick
snapshot
showing
the
kind
of
Earth's
observation
used
in
simulations
and
our
idealized,
the
rich
and
the
upper
planets,
and
we
already
see
some
Curiosities
in
the
SSC
and
also
how,
in
in
many
regards
the
Meridian
or
heat
transport
and
the
ideal
lifespan
is
don't
look
too
different
from
the
real
Earth.
A
But
this
is
just
to
further
show
that
yeah
and
despite
the
extreme
simplification
and
those
setups,
can
help
us
do
important
science
questions
to
get
into
a
bit
of
detail
on
the
set
on
how
we
configure
these
models,
as
I
already
mentioned,
and
the
atmosphere
component
we're
using
scan
for
that's
that's
mostly
motivated
by
a
balance
between
the
complexity
and
the
cost
and
for
the
ocean
model.
A
We
are
using
the
latest
CSM
component,
Bob
six
as
nominal
two
degrees
resolution,
and
about
four
thousand
meter
steps
and
we're
putting
the
bottom
topography
there,
which
is
particularly
important
for
the
aqua
case
and
the
rest
of
the
components,
sea,
ice
and
and
land.
We
were
just
using
a
CSM
default.
We're
reading
we're
really
looking
forward
to
having
the
simplified
land
model,
which
would
make
the
process
much
easier
and
for
our
experiments.
A
We
we
retain
the
seasonal
cycle
by
using
fixed
or
idealized
orbital
parameters,
and
we
initialize
the
ocean
state
from
a
previous
idealized
experiments
provided
by
Pedro.
A
So
our
model
well
with
the
particular
set
of
parameters
we
get
pretty
close
to
cost
equilibrium
in
terms
of
the
top
of
the
atmosphere
balance
by
year,
400
so
and
for
the
rest
of
the
whole,
the
talk
we
will
be
looking
at
the
100
years,
climatology
between
year
400
and
the
year
500.,
and
this
is
the
quick
animation
showing
the
monthly
SST
at
the
year,
400
for
both
this
aqua
and
Rich
planet
on
Aqua.
A
We
observe
something:
that's
that's
very
different
from
the
assumed,
absolutely
only
kind
of
SSD
profiles.
In
the
sense
that
we
have
a
persistent
Global
belt
of
Equatorial
uploading,
so
we
always
get
a
SSC
minimum
right
on
the
equator
throughout
the
seasonal
cycle.
A
And
if
we
look
at
bridge
then
in
some
regards
we
can,
we
can
see
it
as
an
idealize,
the
gigantic
Pacific,
and
we
see
some
analogs
to
the
features
that
are
in
the
Pacific,
including
a
western,
wonderful
on
the
western
side
and
the
Eastern
hotel
with
the
upwelling,
and
we
also
kind
of
see
how
for
the
eastern
coast
Town,
the
adduction
from
the
eastern
boundary
currents
also
contributes
to
that
which
the
effect
is
more
dominant
is
some
Seasons
than
others
all
right.
Getting
a
closer
look
at
the
climatological
sea
surface
temperature.
A
The
first
thing
to
notice
that
is
both
our
planets
are
pretty
warm
and
otherwise
even
warmer
damage
by
two
degrees
and
at
those
temperatures
we
don't
get
CIS
and
then
the
planetary
Albedo
is
mostly
dominated
by
the
effect
of
clouds
and,
as
we've
seen
in
the
animation,
Aqua
has
a
global
called
out
of
Equatorial
operating
and
they
enrich
that
extend
of
our
uploading
has
been
has
been
reduced
to
the
to
the
eastern
part.
A
End
of
the
the
contract
and
the
zonal
gradient
of
SST
in
the
equatorial
region
are
rich
corresponds
to
the
wind
stress
pattern
of
the
surface
and
looking
in
the
vertical
at
the
equatorial
thermocline,
we
see
that
on
Aqua,
the
global
equatorial
operating
corresponds
to
a
really
shallow,
some
replying
on
the
and
right
in
the
equatorial
region,
whereas
Outreach.
A
This
is
a
very
sharp
contrast
that,
due
to
the
presence
of
the
western
boundary,
which
we
see
a
several
client,
that's
more
Earth-like
and
and
again
the
depth
of
the
assemble
kind
of
reflects
the
convergence
of
the
zonal
wind
above
and
we
see
the
location
of
the
Wormhole
being
about
a
third
way
across
the
ocean.
Basin.
And
that's
a
that's,
a
question
that
we're
still
trying
to
understand
like
what
are
the
controlling
factors
in
the
intensity
of
the
and
the
location
of
the
Western
Wormhole.
A
That's
something
of
to
investigate
and
looking
at
the
ocean
circulation
in
the
vertically
integrated
sense.
And
so
here
we
see
the
barotrope
extreme
function
being
overlaid
on
the
Zone
anomaly
of
SST
and
our
Aqua.
There
is
a
week
we
see
very
little
zono,
normally
as
we
designed
it,
except
for
the
imprints
from
the
bottom
of
Murphy
and
which
is
more
easily
shown
in
the
higher
latitudes
and
Aqua.
A
Just
have
this
massive
Soul
flows,
it's
a
rich
case
that
is
dampened
a
lot
and
the
magnitude
of
the
flow
has
been
reduced
and
we
see
the
more
familiar
double
gyre
kinds
of
kind
of
circulation
with
the
warm
part
and
the
cotton.
In
the
background.
A
To
get
a
better
look
at
the
zonal
flow
at
on
these
two
planets,
and
here
we
are
looking
at
the
zonal
average
of
the
of
the
zonal
flow.
And
again
we
see
how
how
we
just
gets
this
crazy
Zone
objects
and
the
maximum
velocity
definitely
reaches
the
magnitude.
A
That's
not
very
earthquake
in
the
rich
case
that
is
much
reduced
and
we
get
a
lot
of
interesting
features,
especially
in
the
in
the
tropics
that
we
have
analogs
to
the
equatorial
under
and
the
counter
currents
and
which
corresponds
to
the
to
the
depths
of
the
at
about
500
meters.
And
that's.
A
And
so,
and
the
presence
of
the
Arizona
Symmetry
and
the
rich
planets
these
two
asymmetry
in
the
atmosphere
as
well,
and
here
we
are
looking
at
we're
here-
we're
looking
at
the
atmosphere
and
looking
at
the
zonal
circulation
in
the
equatorial
region.
A
In
the
alpha
case,
the
cold
and
dry
equator
corresponds
to
a
belt
of
subsidence,
whereas
range
again
looks
more
familiar
with
a
walker-like
circulation
with
convection
in
all
over
the
Western
Wormhole
and
subsidence
on
the
Eastern
side,
and
that
leads
to
order
contributes
greatly
to
the
overall
difference
in
the
climate
that
we
have
seen.
A
A
Here
we
see
that
the
main
differences,
especially
writing
the
equatorial
region
between
the
net
heating
in
between
upper
and
the
ridge,
is
that
alcohol
receives
a
lot
more
net
heating,
which
is
mostly
due
to
the
greater
amount
of
short
wave
as
well
as
a
lesser
amount
of
latent
heat
loss.
A
So,
in
other
words,
the
the
dry
equatorial
belt
on
Aqua,
despite
it
being
cold,
it
is
actually
a
region
of
heating
for
that
planet
and
compared
to
Ridge,
and
those
energetic
aspects
tell
us
something
about
how
the
over
how
the
overall
meridiano
heat
transfer
should
behave,
and
now
we
are
looking
at
it
from
the
dynamic
side
of
how
the
near
the
overturning
circulation
actually
transports
this.
A
This
heat
for
both
component
here
we
are
seeing
the
Meridian
orbitaly
circulation
in
the
solid
and
dashed
counters,
and
the
color
shading
underlying
both
of
them
are
the
stratification
of
of
the
energy
which,
in
the
atmosphere
scales
with
the
moist
static
energy,
which
again
scales
with
the
equivalent
potential
temperature
and
for
the
ocean,
it's
just
the
potential
temperature
itself
and
for
the
overturning
circulation.
In
the
upper
case,
we
see
that
the
code
equatorial
about
or
the
SSP
minimum
on
the
equator
gives
Rises
to
some
ADM
features
which
are
little
Rivers.
A
Had
these
cells,
and
so
the
other
regions
of
of
of
convection,
all
the
double
itcgs
are
are
actually
we
have
we
get
these
two?
Maybe
the
only
symmetric
regions
of
a
convection
around,
perhaps
10
degrees,
north
and
south
of
subsidence
right
on
the
equator
and
outrage
this.
This
pattern
of
reverse
heavily
is
much
suppressed
due
to
the
presence
of
the
western
wormhole.
A
Now
on
the
ocean
for
the
ocean
side,
the
thermal
stratification
and
they're
done
overturning
young
Aqua
looks
pretty
others
like
in
terms
that
we
get
a
lot
a
really
deep
sonopi
in
the
subtropics
and
associated
with
some
with
how,
because
of
the
lack
of
a
marital
boundary,
how
how
the
how
they
are
on
overturning
circulation
is
basically
goes
through
the
half
of
the
hemisphere
and
and
the
upwelling
water
at
the
equator
returns
from
from
substantial
depths
and
the
Zia
and
Zia
several
client
in
the
subtropics
produce
really
deeply.
A
So
there
is
a
greater
contrast
of
the
of
between
the
upper
branch
of
and
the
lower
branch
of
the
overturning
circulation
and
that's
how
the
ocean
overturning
moves
more
heat
around.
In
the
rich
case.
A
We
see
that
because
of
the
western
boundary,
the
summer
kinds
gets
a
lot
shallower
and
and
that
that,
in
her
influences,
how
the
overturning
transports
and
that
energy
as
well
and
to
tie
it
up
revisiting
the
Meridian
or
heat
transport
calculated
from
those
two
components,
and
we
see
that
consistent
with
both
the
energetic
constraints
and
how
the
Dynamics
was
working
and
the
upper
planet
and
the
the
atmosphere
is
actually
moving
energy
equator
world
and
within
the
10
degrees,
north
and
south,
and
that
is,
and
both
energetically
required
in
terms
that
the
ocean
net
heating
was
greater
than
the
top
of
the
atmosphere
Heating
in
those
regions
and
dynamically.
A
That's
that's
carried
out
by
the
rivers
heavy
circulation
in
the
atmosphere
on
the
rich
planet.
We
still
get
a
little
of
that.
We
both
inside
of
the
deep
Tropics,
but
that
is
much
reduced
from
aqua
and
that
again,
that's
in
terms
of
the
energetics
and
the
Dynamics
that
so
yeah
Rivers
had
these
cells
turn
to
be
a
lot
weaker.
A
So
to
to
put
down
a
couple
points
of
discussion
at
this
point
is
that,
despite
the
simplification
in
the
in
the
overall
geometry,
the
climates
of
the
coupled
aqua
and
the
rich
cases
show
some
features
which
are
relevant
to
understanding
the
comprehensive,
realistic,
realistic
type
of
simulations
in
in
terms
of
how
the
ocean
geometry
impacts.
A
The
overall
climate
State
as
well
as
features
like
the
mirroredomo
key
transport
and
asyla
previously
mentioned
the
this
couple
of
simple
models,
is
planned
to
be
available
within
the
next
release
of
CSN
with
that
and
as
efforts
and
the
software
engineering
side
to
provide
tools
to
streamline
this
kind
of
processes,
so
so
that
the
investigators
can
configure
their
own
setups
to
the
question
of
their
interest
and
some
just
some
ideas
for
the
applications
for
this
type
of
type
of
models.
A
Of
course,
for
the
interests
of
scaffold
atmospheric
ocean
Dynamics,
it's
helpful
to
have
it
for
comprehensive
atmosphere
that
could
be
coupled
to
an
ocean
of
choice
and
the
so
yeah.
That's
the
advantage
of
having
a
comprehensive
atmosphere
is
that
we
will
be
able
to
to
represent
a
a
whole
spectrum
of
atmosphere,
phenomenons
on
different
scales
in
including
synoptic
storms
like
astrological
and
tropical
Cyclones,
and
how
they
might
interact
with
the
ocean
and
on
the
ocean
side.
A
The
and
the
other
track
of
studies
inspired
by
the
amateages
and
series
of
studies
is
to
explore
increasing
complex,
complex
geometries
and
how
those
affect
the
the
ocean,
circulation
and
other
aspects
of
the
climate,
and
on
that
we
will
hear
more
from
Sarah
who's
talking
next
and
other
exciting
things
like
the
aimog,
and
so
that's
on
the
general
state
of
the
main
climate
of
these
ideolized
models
and
before
taking
questions.
A
I
just
wanted
to
show
a
couple
of
more
things
which
are
under
investigation,
but
I
think
I
really
curious
to
look
at
so
we've
had
looked
at
the
the
mean
state.
However,
there's
also
a
lot
of
interesting
variability
on
these
planets
one
one
of
them
is,
and
inner
annual
variability
in
sat
that
really
I
think
it
looks
a
lot
alike
and
so
on
the
rich
planet.
A
And
here
the
top
flood
is
showing
the
first
principle
component
of
the
equatorial
SSC,
where
we
see
the
region
of
a
dominant
variance
B
in
the
in
the
Eastern
Hotel.
So
that's
a
pretty
and
so
like
pattern.
Although
the
the
frequency
doesn't
quite
line
up
with
the
realistic,
and
so
but
it's
it's
a
reasonable
time
scale
and
that's
something
we
are.
A
We
are
trying
to
explore
a
bit
further
another
aspect
of
variability
on
the
atmospheric
side,
that
is,
the
season
of
seasonal
variability,
one
of
the
dominant
notes
being
the
Madden
during
oscillation
and
I
guess.
This
is
probably
less
familiar
with
the
most
oceanographers.
But
this
is
just
the
show
in
the
a
a
spectrum
of
Equatorial
modes
which
is
taken
between
the
15
degrees,
north
and
south,
and
looking
at
a
high
frequency,
meaning
three
hourly
precipitation
and
mjo.
A
Is
this
guy
right
here
and
that
which
distinguishes
itself
from
from
the
Kelvin
waves
and
that's
something
unique
to
Rich
that
we
don't
see
so
much.
That's
another
curious
aspect,
and
one
last
thing
I
wanted
to
show,
because
just
because
we
mentioned
skill
interactions
is
that
one
of
the
major
motivations
you
use.
A
A
comprehensive
atmosphere
like
canv4
is
that
we
get
something
extra
seconds
and-
and
this
is
using
the
sea
surface
temperature
from
the
rich
experiment
and
using
those
to
force
a
high
resolution,
meaning
quarter
degree
kind
of
four
on
the
atmosphere
where
we
see
that
the
E
from
the
Western
worm
pool
in
the
summer
season.
A
We
see
the
emergence
of
of
tropical
Cyclones
in
this
case
three
of
them,
which
again
is
quite
it's
not
too
far
from
what
we
expect
from
what
we
observing
the
in
the
pacifics
and
in
the
tracks
from
one
year
we
see
the
kind
of
a
symmetry
between
the
western
side
and
the
Eastern
side
in
triple
Second
Genesis.
So
that's
a
that's
the
further
direction
that
we're
looking
at
and
yeah.
A
A
B
That's
great
questions
for
zoning.
B
C
Hi
I
have
a
question:
go
ahead.
Well,
I
have
a
bunch
of
questions.
It's
it's
so
good
to
see
the
simulations
and
see
a
lot
of
the
features
that
I
found
in
mine,
which
are
quite
different
from
Marshall's.
First
aquaplan
simulations
I
saw
that
when
you
show
the
design
currents
in
the
aqua
simulation,
the
the
color
scale
was
saturated,
so
yeah.
What?
What
is
the
maximum
speed
that
you
found
on
the
crater
on
the
surface,
where
mine
were
ridiculously
large,
like
four
meters
per
second
yeah.
A
Mine
is
with
the
mom.
Six
is
not
it's
still
really
large,
especially
on
this
slide.
Yep.
The
maximum
is
like
more
than
two
meters
per
second,
more.
C
C
And
I
haven't
been
able
to
slow
them
down
so
I
play
with
the
bottom,
drag
and
and
increasing
in
them
by
orders
of
magnitude,
and
and
they
stay
the
same.
So
it's
something
I
still
understand.
I
thought
it
would
be
controlled
by
the
magnitude
of
friction
on
the
bottom.
C
C
Configuration
in
some
of
these
configurations,
you
can
switch
sides
and
you
end
up
having
the
model
in
the
East
really
yeah,
yeah
and
I
have
a
third
question.
You
run
them
for
500
years
or
for
400
years.
What's
the
drift
that
you
have?
Oh
surprised,
you're,
not
having
a
lot
of
drift,
starting
from
my
initial
conditions,
given
that
your
climate
is
so
much
warmer
mine
I
took
some
of
the
parameters
in
the
atmosphere,
so
that
would
get
a
global
mean
temperature
of
14
degrees.
I
thought
it
would.
C
A
That's
a
good
question:
I
didn't
put
the
plot
here,
but
yeah
by
the
end
of
year,
400
the
drift
in
terms
of
post,
TOA
balance
and
the
ocean
potential
temperature
was
pretty
small,
like
oh
pretty
degradation
for
purpose
all
of
these
planets.
So
our
our
deep
ocean
is
still
dripping.
That's
why
it's
active,
but
the
overall
event
is
not
that
bad
and
another
part
of
your
question,
the
a
heavy
Waters
like
temperatures
and
in
some
in
some
regards
that
translates
to
like
Motors
like
Albedo.
A
That's
that's,
certainly
one
of
the
aspects
that
we
can
like,
so
to
speak,
to
it
too,
and
for
the
idealized
words
and,
however,
we
just
we
just
felt
that,
because
of
because
of
their
their
well,
even
though
they're
idealized,
there
are
still
a
lot
of
degrees
of
freedom,
and
we
can
always
try
to
line
some
aspects
more.
It's
like
approach
to
others
and
and
the
in
our
case.
We
we
think
it's
the
absence
of
Cs.
Is
it's
not
the
worst
thing
we
can
like?
A
We
get
all
the
action
from
the
atmosphere
and
in
terms
of
the
American
heat
transport,
which
is
what
we
are
looking
at,
it's
already
pretty
Earth-like,
so
we
think
it's
it's
a
reasonable
configuration
for
our
question,
even
though
for
other
questions
when
where
a
Meridian
or
a
Earth-like,
Meridian
or
temperature
gradient
is
more
desirable
or
if
CIS
is
more
desirable,
then
there
are
reasons
to
go
to
to
to
go
to
to
tend
to
those
dimensions
a
bit
more.
That's
that's
like
our
rationale.
C
A
Not
at
this
point,
because
we
are,
we
are
happy
with
the
Quasi
equilibrium,
climate
and
and
a
a
large
part
of
that
is
a
data
management
issue.
B
A
Of
the
Computing
hours
so
yeah,
if,
if
there's
infinite
like
space,
then
maybe
it
will
be
curious
to
see
what
happens.
Oh
and
and
along
those
lines
there
are
disadvantages
and
studies
are
like
multi-incremental
space.
You
can
like
prefer
them,
and
things
like
that.
So
on
the
on
the
millennial
scale
that
there
there
would
be
some
interesting
things
to
see,
but
for
now
we're
settling
with
this
quantity
equilibrium
that
we
have
got.
C
B
A
lot
of
kind
of
oceanographic
studies
along
these
lines
would
take
as
their
next
step
of
reducing
their
idealization,
adding
a
Drake
Passage,
although
usually
with
some
kind
of
a
deep
Ridge
or
adding
a
wider
Pacific
and
a
narrower
Atlantic
Basin.
Have
you
thought
about
what
your
next
steps
are
going
past
this
first
very
idealized
case
and
how
that
might
fit
into
this
previous
literature
right.
A
Great
question
and
the
great
Segway
into
Sarah's
talk
next
on
a
more
increasing,
complex
form
of
ideal
as
geometries
and
for
for
questions
like
amok
and
a
lot
of
others.
We
wouldn't
need
a
smaller
Basin
to
represent
those
are
for
for
my
question,
which
is
actually
on
the
interaction
between
triple
Cyclones
and
the
ocean.
We
are.
We
are
happy
with
the
big
Pacific
and
we're
just
going
to
look
at
a
specific,
like
kind
of
actions,
but
I.