First, the satellite can see actual low clouds only when
higher cloud layers are not present.
The lack of absorption features means that GJ 1214 b can not have a diffuse hydrogen atmosphere unless it also has
a high cloud layer that blocks the starlight from streaming through.
Not exact matches
The false colors represent the altitudes of the various
cloud layers — blue being the
highest and red being the lowest.
Observations by Akatsuki found a
high speed equatorial current in the lower to middle
cloud layer, though what drives it remains unexplained.
It's even more dramatic when a thin
layer of
high clouds is present.
These include a widening of one of the brown belts just north of the equator, which has spawned wave patterns throughout the northern hemisphere, both in the
cloud layers and
high above in the planet's stratosphere,» said Dr Fletcher from the University of Leicester's Department of Physics and Astronomy.
During the dry season, with no fog
layer to reflect sunlight, the smaller
cloud cover allows plants to receive much
higher radiation, increasing evaporation and photosynthesis rates, another process missed by the GCMs.
While the large atmospheric pressure at the surface and the
high altitude of the Venusian
cloud layer appears to exclude the possibility of
cloud - to - ground lightning (Gurnett et al. 2001; Aplin 2006), several authors have suggested that lightning discharges above, between or within
clouds may occur (Borucki 1982; Russell & Scarf 1990; Gurnett et al. 2001).
In the second half of the talk I will present our recent studies of the young stellar population in W3 - AFGL333, located in a
high density
layer between the expanding W4 HII region and the W3 giant molecular
cloud.
Based on the available data, the astronomers concluded that the planet's atmosphere is either a thin but dense
layer rich in water steam or a thick
layer of
high clouds or hazes, similar to those seen in the atmospheres of Venus and Titan in the Solar System.
But they do at least have certain basic physical principles in their
cloud representations —
clouds over ice have less albedo effect than
clouds over water, you don't get
high clouds in regions of subsidence, stable boundary
layers lead to marine stratus, etc..
A simple counterexample illustrates this: consider two massive
cloud layers with equal shortwave albedo, one at
high altitude, one at low altitude.
(Note that radiative forcing is not necessarily proportional to reduction in atmospheric transparency, because relatively opaque
layers in the lower warmer troposphere (water vapor, and for the fractional area they occupy, low level
clouds) can reduce atmospheric transparency a lot on their own while only reducing the net upward LW flux above them by a small amount; colder,
higher - level
clouds will have a bigger effect on the net upward LW flux above them (per fraction of areal coverage), though they will have a smaller effect on the net upward LW flux below them.
The meeting will mainly cover the following themes, but can include other topics related to understanding and modelling the atmosphere: ● Surface drag and momentum transport: orographic drag, convective momentum transport ● Processes relevant for polar prediction: stable boundary
layers, mixed - phase
clouds ● Shallow and deep convection: stochasticity, scale - awareness, organization, grey zone issues ●
Clouds and circulation feedbacks: boundary -
layer clouds, CFMIP, cirrus ● Microphysics and aerosol -
cloud interactions: microphysical observations, parameterization, process studies on aerosol -
cloud interactions ● Radiation: circulation coupling; interaction between radiation and
clouds ● Land - atmosphere interactions: Role of land processes (snow, soil moisture, soil temperature, and vegetation) in sub-seasonal to seasonal (S2S) prediction ● Physics - dynamics coupling: numerical methods, scale - separation and grey - zone, thermodynamic consistency ● Next generation model development: the challenge of exascale, dynamical core developments, regional refinement, super-parametrization ●
High Impact and Extreme Weather: role of convective scale models; ensembles; relevant challenges for model development
The towering
clouds were so
high that they punched through the troposphere (the lowest
layer of the atmosphere where most weather occurs) and sent air loaded with ice crystals rushing into the stratosphere, a
higher layer that normally contains very little moisture.
The rising zones, meanwhile, soar
high into the atmosphere, and contain
clouds of ammonia ice crystals that reflect sunlight, and block the view of the darker
layers below, just like
clouds here on Earth.
Composite imaging is an extremely useful tool for helping people understand the Earth — they allow researchers to capture certain features at
higher resolution; reduce the obscuring effect of
cloud coverage in certain areas; and overlay various data
layers to help identify patterns and trends.
When solar activity is
high and (under the GCR -
cloud theory)
cloud cover is low, a
high amount of solar radiation reaches the oceans unblocked by
clouds, where it penetrates and warms the upper ocean
layer.
The energy released now heats the gas till it becomes an ionised plasma due to the
high Temperature, the escape of this centraally generated energy to the suface of the «
cloud», now a proto star will eventually stop the collapse as the outer
layers also heat, and the outer plasma will become opaque to the EM radiation generted at the million degree buring interface.
Pooh, Dixie Erlykin and Wolfendale do specify that, relatively speaking, the greatest effect was seen in low
cloud cover and mid
cloud cover, and they use the f value for those levels in their calculations, but if CR affect
higher layers dissimilarly so as to reduce the net effect that should be noted.
Rather than having a thin atmosphere and solid - and - liquid surface like Earth, Saturn is a gas giant whose deep atmosphere is
layered with multiple
cloud decks at
high altitudes.
It is similar to
cloud seeding, except at
high altitudes, and is designed to produce thin
layers of
cloud.
Given that the NARR
high - level
cloud layer is situated above 350 mb, this latitudinal asymmetry is likely due to the positioning of the subtropical and polar jet streams.
Well, you can guess it based on the type of
clouds — in zones of
high pressure the dominant
cloud type are the stratus family — thin,
layered clouds, that absorb far less energy than cumulus
clouds, and can dramatically increase albedo, therefore act as climate coolers.
The climate models with the mixed
layer oceans underestimate both the subtropical low
cloud cover and the
high - latitude sea ice / surface albedo, and consequently have a smaller warming response to OHT.