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- International
H2O Project (IHOP)
- Convective
PBL and turbulence dispersion
- Wildfire
research
Stable
PBL (top)
Related websites:
http://www.joss.ucar.edu/cases/
(CASES 97)
http://www.mmm.ucar.edu/science/abl/cases/cases.html
(CASES 99)
CASES-97
During the last few years, Margaret
LeMone, with Kyoko Ikeda, and Robert Grossman (then
at University of Colorado, now at Colorado Research Associates)
analyzed the horizontal variability in the potential temperature
at 2 m T2m. They found that the temperature varied linearly
with station elevation, and the elevation-dependence was dry-adiabatic
for sufficiently high Froude numbers. This year, the study
was extended to include the evolution of the pattern through
the night, and the departures from the linear trend.
Variation through the night: The evolution depended on ambient
conditions. For clear-sky, light wind conditions, the horizontal
variability in T2m increased through the night, as a watershed-scale
circulation developed. As the total horizontal variability
(standard deviation) increased, the standard deviation with
respect to the best fit decreased. Other researchers found
maximum total variability at earlier times. The results of
this study suggest that the time elapsed between sunset and
maximum horizontal variability is related to the scale of
the terrain, the size of the array, and the spacing between
stations. For strong winds and weakly stable thermal stratification,
maximum horizontal variability occurred a few hours after
sunset, and is linked to horizontal advection and vertical
mixing.
Departure from the linear trend: Sites with thick surface
cover (winter wheat) had cooler minimum temperatures than
sites with bare ground, compared to the linear trend. Sites
on ridges tended to be "too warm" and sites near
bluffs tended to be "too cold."
CASES-99
During the past year, Jielun Sun
and Sean Burns focused on
processing the pyrgeometer data collected from CASES-99 and
analyzed nocturnal heat budget and turbulence intermittency.
Burns conducted careful
radiation data processing and discovered mismatches between
data loggers and the pyrgeometers during the field campaign,
and consequently devoted considerable effort to correct the
errors.
Sun focused on origins
of intermittent turbulence by analyzing the night of October
18, 1999 with all the available observations, by closely collaborating
with colleagues involved in CASES-99. She found that the passage
of the atmospheric disturbances of a density current, solitary
waves, and internal gravity waves were responsible for the
intermittent turbulence. Turbulence adjacent to the ground
can be generated by directional wind shear, pressure change,
and drainage flows. Turbulence above the ground can be generated
by thermal instability from overturning of cold air above
warm air by atmospheric waves or large eddies, and can also
be generated by shear instability from wind gusts associated
with the atmospheric disturbances. Quiescence from turbulence
suppression can come from descending motions associated with
passages of atmospheric disturbances due to the mass balance,
energy dissipation in nocturnal cooling air, and directional
shear which strengthens local stability. Occurrence of these
instability and stability factors at various time and heights
lead to apparent intermittent turbulence.
Sun, in collaboration with
Steve Oncley, Tony Delany, and Tom Horst (all NCAR/ATD), designed
instrumentation for the radiative flux divergence measurements
during CASES-99, which resulted in both observed radiative
flux and sensible heat divergence over a relatively deep layer
(between 2 m and 48 m) for the first time in history. Complications
associated with heterogeneous surfaces were considered in
the radiation flux divergence measurement, to avoid the ambiguity
caused by two different fields of views from the radiative
flux measurement at two levels. Through analysis of this data
set, Sun studied the roles
of the sensible heat and radiative flux divergence in the
heat balance and their contribution to the applicability of
Monin-Obukhov similarity theory in stable boundary layers.
It was discovered that, in general, the largest radiative
flux divergence occurs in the early evening under weak wind
conditions following several days of warm trend. Averaging
over the entire field campaign, the radiative flux divergence
tends to be smaller than the local cooling and the sensitive
heat divergence between two levels. However, the day-to-day
variation of the sensible heat flux divergence tends to be
larger than the radiative flux divergence. The radiative cooling
observed between 2 m and 48 m is much smaller than the radiative
cooling observed below 10 m in the literature. This implies
that the radiative flux divergence may decrease with height
as suggested by numerical radiation transfer models. Wind
speed can change not only the sensible heat flux, but also
the surface longwave radiation due to variations of surface
area-exposure of warmer grass stems and soil surfaces compared
to cool grass top, leading to fluctuations of the radiative
flux divergence throughout the night.
Sun and Burns
also studied dominant eddy scales of the wind, vertical velocity,
water vapor specific humidity and temperature in the nocturnal
boundary layer by using the Haar wavelet transform. They found
that about 50% of the nights, the horizontal wind eddy scale
is about 10 min while the vertical velocity is about 3 min,
which indicates "pancake" type of motions in the
nocturnal boundary layer. Other work included collaboration
with Greg Poulos (Colorado Research Associates) on comparisons
between model flux parameterizations and observed flux data
from CASES-99.
Interaction between heterogeneous
surface and atmosphere (top)
Influence of soil moisture heterogeneity on the PBL
Edward Patton (Pennsylvania
State University), Sullivan,
and Moeng used their clear-PBL
large-eddy simulation code that was recently coupled with
the NOAH (National Center for Environmental Prediction / Oregon
State University/Air Force/Office of Hydrology) land-surface
model to study the planetary boundary layer (PBL) response
to large-scale soil moisture heterogeneity (ranging from 2-30
km). In the presence of heterogeneity, the atmosphere transports
moisture differently depending on the initial moisture state
in the overlying atmosphere, wet versus dry. In both situations,
land-surface heterogeneity induces organized motions that
scale with the heterogeneity (see Movie 8). However, depending
on the moisture state of the overlying atmosphere, the phase-correlated
component can either be the sole contributor to the vertical
water vapor mixing ratio flux, or make zero contribution (Figure
35 b.1). One of the important findings of this study is that
if researchers plan to use the eddy-correlation technique
to measure vertical water vapor mixing ratio fluxes at a point
within a region of large-scale moist or dry soil conditions,
they could dramatically misestimate the vertical fluxes if
they ignore the contributions to the flux from organized motions,
induced via heterogeneous surface forcing.


Links at right show larger versions of these movies.
To
view the movies, place mouse over image. Alternately,
for slower connections, you may use the links below
to download the movies.
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Vertical
(animated GIF)
Vertical
(AVI format)
Vertical
(MPEG format)
Horizontal
(animated GIF)
Horizontal
(AVI format)
Horizontal
(MPEG format)
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| Movie
8. Movies: (click on each to see their associated
movies) show the temporal and spatial evolution of vertical
and horizontal slices of atmospheric mixing ratio perturbations
in the convectively driven planetary boundary layer (PBL)
over a heterogeneous land surface (wavelength ? = 15 km). |
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| Figure 35. Vertical profiles
of the normalized total mixing ratio flux (green) and
the contribution to the total from the large-scale organized
motions (blue) and the background turbulence (red). The
top row presents results from cases where the atmosphere
is initially dry (wetting PBLs), and the bottom row from
cases where the atmosphere is initially wet (drying PBLs).
The left-most panels are the control cases where the land-surface
is horizontally homogeneous. The middle and right panels
present results from cases with horizontally heterogeneous
surface forcing with ? = 5 km and ? = 2 km respectively. |
Atmospheric response to spatial variations
of soil moisture
Related website: http://www.mmm.ucar.edu/science/abl/sgp/sgp.html
Sun investigated responses
of the atmospheric moisture flux to temporal and spatial variations
of soil moisture and spatial variation of vegetation, by analyzing
the aircraft data collected from the Southern Great Plains
(SGP) experiment. She focused on the atmospheric moisture
flux collected by the Canadian Twin Otter aircraft along the
El Reno and Kingfisher tracks, where both atmospheric turbulence
and Electronically Scanned and Thinned Array Radiometer (ESTAR)
soil moisture were well sampled. She found that the latent
heat flux is influenced by the relatively fast temporal variation
of soil moisture and relatively slow spatial variation of
evapotranspiration from the vegetation root zone. The soil
moisture content determines the importance of the spatial
variation of the vegetation in the spatial variation of the
atmospheric moisture flux. Extremely wet and extremely dry
conditions would diminish the contribution of the spatial
variation of the vegetation in the atmospheric moisture flux.
The spatial variations of the vegetation play a dominant role
in the spatial variation of the latent heat flux when the
soil moisture is below about 20%, but not dry enough to cause
severe vegetation damage.
Horizontal transport of CO2 over complex terrain
Sun led an investigation
of horizontal transport of CO2 at Niwot Ridge, in collaboration
with Steve Oncley, Tony Delany, Britt Stephens and Teresa
Campos (all NCAR/ATD), and Alex Guenther and Andrew Turnipseed
(both NCAR/ACD), Russ Monson (University of Colorado), Dean
Anderson (U.S. Geological Survey), and Brian Lamb (Washington
State University). A pilot experiment investigating the horizontal
transport of CO2 within a forest canopy layer was conducted
in August/September of 2002. The CO2 concentrations were measured
at three to four levels within the canopy layer, at eight
locations, within a 300 m2 area. To ensure the relative accuracy
between locations, the CO2 concentration was measured by two
central CO2 analyzers and 18 inlets, from various levels,
at various locations. In addition, a central CO2 inter-comparison
system was designed to provide quality-control for the CO2
measurement from different CO2 sensors. Further information
related to this work, which was supported by NCAR Opportunity
Funds and the NCAR Biogeosciences Initiative, is available
at http://www.mmm.ucar.edu/science/abl/forest/.
Investigation of impacts of cold land transition in the
global climate change
Related website: http://www.mmm.ucar.edu/science/abl/floss/
Burns assisted Larry Mahrt
(Oregon State University) in setting up MMM thermocouples
on a 20-m tower near Walden, Colorado, in early December 2001,
during Fluxes over Snow Surfaces (FLOSS). He also was involved
in monitoring the thermocouple temperatures during the experiment
to ensure the quality of the data. The FLOSS field experiment
was conducted in collaboration with Steve Oncley, Tony Delany,
and Steve Semmer (all NCAR/ATD), and Larry Mahrt, Dean Vickers,
and Richard Cuenca (all Oregon State University).
Interaction between ocean
and atmosphere (top)
Effect of wave breaking on the ocean boundary layer
Sullivan, James McWilliams
(University of California, Los Angeles) and Moeng,
in collaboration with Ken Melville (Scripps Institute of Oceanography),
are developing a stochastic wave breaking model for use in
simulations of the ocean boundary layer (OBL). Turbulence-resolving
simulations of the OBL typically impose a mean (constant)
surface wind stress at the water surface, despite the known
spatial and temporal variations in stress. This assumption
neglects intermittent processes and, in particular, wave breaking,
which is believed to be an important mechanism for transferring
momentum and energy from waves to the ocean currents. The
wave breaking model for the OBL neglects the complexity of
a full air-water microphysical interface and, instead, focuses
on important bulk processes, intermittent momentum and energy
transmission from breaking waves. Direct numerical simulations
are initially being used to test various aspects of this model.
Preliminary results are shown in Figure 36 c.1.
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| Figure 36. Visualization
of the horizontal current field u, panels left and right
of a), and vertical momentum flux uw, panels left and
right of b), at z/h = -0.014 below the water surface.
Snapshots in the upper panels are for an OBL driven by
a constant surface stress while the flow fields in the
lower panels contain strong breaker forcing. Wave breaking
is observed to greatly disrupt the elongated near-wall
streaky structures associated with wall-bounded shear
flows. Intense impulses from the breaking waves impart
strong vertical momentum flux, both positively and negatively
signed, to the water column. Even though the observed
white cap covereage of the breakers at the surface is
very intermittent (less than 2\%) the presence of breaking
eventually stirs the entire surface layer of the OBL. |
Effect of ocean waves on the atmospheric surface
layer
Anna Rutgersson (Uppsala University and the Swedish Meteorological
and Hydrological Institute) and Sullivan
are investigating the effect of waves on the turbulent structure
in the atmosphere using Direct Numerical Simulations (DNS)
databases. There have been experimental indications that the
effect of very fast waves (swell) over the ocean is different
than previously believed. This could have large impact on
global climate models, since the world oceans cover such a
large part of the globe. The DNS data show significant wave-induced
peaks in power spectra that extend up to higher levels for
very fast moving waves. When separating the vertical momentum
flux into quadrants, the cases with waves, and especially
very fast waves, have larger amplitude transport events, with
both positive and negative transport related to the waves.
This can be seen, both in the DNS-data, and from measurements
over the sea. Figure 37 c.2 shows the relative contribution
from the four quadrants from DNS (blue) and measurements taken
over the Baltic Sea (red). In spite of the differences between
DNS-simulations and measured situations, the structure of
the quadrants is similar. All quadrants have larger contributions
during swell in both the measurements and the DNS.
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| Figure 37.
Quadrant analysis from DNS (blue) and measurements from
the Baltic Sea (red) during growing sea (upper) and swell
(lower). Note that there are different scales on the axis
for growing sea and swell. |
Relationship between the atmospheric momentum transport
and oceanic waves
Related websites:
http://www.mmm.ucar.edu/science/abl/showex/showex.html
http://www.mmm.ucar.edu/science/abl/cblast/
Sun and Burns,
in collaboration with Douglas Vandemark (NASA Goddard Space
Flight Center), Mark Donelan (University of Miami), Tim Crawford,
Jerry Crescenti, and Jeff French (all NOAA Air Resources Laboratory),
and Larry Mahrt (Oregon State University), continued investigation
of retrieving two-dimensional wave spectra, using three laser
altimeters, on board the LongEZ aircraft. Sun
and Burns found that the
wavelet analysis method is able to retrieve wavenumbers, based
on wave slopes, simultaneously measured by the three laser
altimeters. Therefore, the wavenumber is independent of where
the wave slope is collected (i.e., whether the wave slope
is collected along a straight line under the aircraft track,
whether the aircraft flies at an angle from the wave propagation
direction, or the aircraft flies at variable speed). However,
when the wave slope is too small to be measured by the three
laser altimeters, or the random noise of the measured wave
slope is large, the wave analysis method may fail to retrieve
the wave propagation direction. This result implies that the
size of the triangle where the three laser altimeters were
located can affect retrievable wavelengths.
Subfilter-scale turbulence
in LES (top)
Related websites:
http://www.atd.ucar.edu/sssf/projects/hats
http://www.whoi.edu/science/AOPE/dept/CBLASTmain.html
Sullivan, Lenschow, and
Moeng, in collaboration
with Thomas Horst (NCAR/ATD), Jeff
Weil (Cooperative Institute for Research in the Environmental
Sciences/Colorado University), and Jan Kleissl, Charles Meneveau,
and Marc Parlange (all Johns Hopkins), continued their analysis
of the sonic array data taken during the Horizontal Array
Turbulence Study (HATS) field campaign. The objective of this
effort is to improve subfilter scale (SFS) parameterizations
in LES models. From the HATS dataset, they found that subfilter-scale
(SFS) turbulent motions in the atmospheric surface layer are
sensitive to the relative positions of the spectral peak of
the vertical velocity ?w, and the filter cutoff scale ?f.
A priori testing of SFS models with the HATS dataset shows
that the turbulent kinetic energy and Smagorinsky model coefficients
Ck and Cs, derived from the measurements, are smaller than
the theoretical estimates based on the assumption of a sharp
spectral cutoff. The correlations between measured and observed
SFS fluxes and energy transfer are relatively low for an eddy
viscosity model, and mixed SFS models that explicitly include
a Leonard term exhibit higher correlations (see Figure 38
d).
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| Figure 38. Correlations
between the HATS observations and an eddy viscosity model,
and a mixed model (eddy viscosity plus a Leonard term)
for the different components of the SFS flux tensor tau.
The colored symbols denote different sonic array configurations.
The correlation for the vertical momentum flux tau is
shown as a solid line. Note the improved correlation obtained
by explicitly including the Leonard term. |
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