I've wondered if the HAARP system had some way to prime a pump just to get CO2 in
the upper atmosphere more likely to radiate in the infrared; the notion of tickling it so it will actually depart the planet seems like a lovely one, if there's any substance to it.
The third experiment would explore the potential for making cirrus clouds in
the upper atmosphere more porous to radiation bouncing back into space from Earth.
Small, sand - grain sized meteoroids are entering the atmosphere constantly, essentially every few seconds in a given region, and thus ionization trails can be found in
the upper atmosphere more or less continuously.
The night - time emission of green light, with a wavelength of 557.7 nanometres, was detected in the Earth's
upper atmosphere more than a century ago.
We also have around 10 nights per year observation time on bigger telescopes in public and professional observatories, which allows us to employ a narrow band methane filter to detect fireballs in Jupiter's
upper atmosphere more efficiently.
Not exact matches
About 5 to 10 times
more neutral particles could be lost through a process called photochemical escape, which happens when UV radiation breaks apart molecules in the
upper atmosphere.
«Even our
upper estimate, 0.01 bar, is an insignificant amount in comparison to the
atmosphere required to maintain a sufficiently strong greenhouse effect, about 1 bar or
more according to climate models.»
On the other hand, the
upper troposphere is relatively rich in O3 and NOx from natural sources such as downward transport from the stratosphere and lightning; convective overturning conveys the O3 and NOx toward the Earth's surface where these components are
more efficiently removed from the
atmosphere.
In this respect, the phenomenon
more closely resembles Earth's Arctic vortices — seasonal cyclones that appear above the poles and are driven by temperature gradients in the
upper atmosphere.
When the team looked at the overall balance between the radiation upward from the surface of the ice sheet and the radiation both upward and downward from the
upper levels of the
atmosphere across all infrared wavelengths over the course of a year, they found that in central Antarctica the surface and lower
atmosphere, against expectation, actually lose
more energy to space if the air contains greenhouse gases, the researchers report online and in a forthcoming Geophysical Research Letters.
But for planetary scientists, Jupiter's most distinctive mystery may be what's called the «energy crisis» of its
upper atmosphere: how do temperatures average about as warm as Earth's even though the enormous planet is
more than fives times further away from the sun?
Earth's
upper atmosphere and the moon have relatively little oxygen - 16, whereas the solar wind has
more.
While lower - energy ultraviolet radiation breaks up water molecules — a process called photodissociation — ultraviolet rays with
more energy (XUV radiation) and X-rays heat the
upper atmosphere of a planet, which allows the products of photodissociation, hydrogen and oxygen, to escape.
Although CFCs are extremely persistent, remaining in the
upper atmosphere for decades, and although they are 10,000 times
more efficient than carbon dioxide at trapping heat, the process of controlling them has been under way for years, for reasons having nothing to do with the greenhouse effect.
Stronger mean upward airflow transports these chemicals
more quickly into the
upper atmosphere, and the ozone layer will recover
more quickly to its natural state before the introduction of man - made freon compounds.»
Results showed that additional data collected that year through
more frequent observation of meteorological conditions in the Arctic's
upper atmosphere from both land - based research stations and the research vessel Lance plying winter Arctic waters improved the accuracy of cold wave forecasts.
Whereas the lower
atmosphere (at altitudes of less than 200 kilometers) is consistent with ground - based stellar occultations, the
upper atmosphere is much colder and
more compact than indicated by pre-encounter models.
This weakened shielding would have allowed
more energetic particles into the
upper atmosphere, which would have begun to break down the ozone layer that protects Earth from harmful UV radiation, Meert says.
In January 2013, sensors on the ground mapped electrons in the
upper atmosphere and saw a tendril of
more densely packed particles curling away from the north pole, indicating that a plume of plasma was veering off towards the sun.
In the end, the greater the difference between the temperature of the sea and that of the
upper atmosphere, the
more powerful the storm.
NASA is funding 11 science projects across America for scientists to take advantage of the unique astronomical event to learn
more about the Sun and its effects on Earth's
upper atmosphere.
At its height between 1960 and 1980, Polyarka was staffed by
more than fifty working scientists, engineers, and technicians focused on measurements of surface weather, snow depth, sea ice, and conditions in the
upper atmosphere.
They found increases in sea surface temperature and
upper ocean heat content made the ocean
more conducive to tropical cyclone intensification, while enhanced convective instability made the
atmosphere more favorable for the growth of these storms.
«
More heat is trapped in the
upper layers of the ocean, where it can be easily released back into the
atmosphere,» Park said.
There are also numerous «fingerprints» which we would expect to see from an increased greenhouse effect (i.e.
more warming at night, at higher latitudes,
upper atmosphere cooling) that we have indeed observed (Figure 6).
When the spacecraft succumbs to the
atmosphere, breaking up and unable transmit any
more data, it will burn up like a meteor in Saturn's
upper atmosphere, NASA officials said.
C. Carreau, ASPERA - 4 & MAG teams, Venus Express, ESA Annotated image illustrating loss of hydrogen through plasma wake Venus may have lost oceans of water due to a runaway greenhouse effect which evaporated water into the
upper atmosphere, where ultraviolet light dissociated water into ionized atomic hydrogen and oxygen (some later incorporated into carbon dioxide) that were blown away by the Solar wind due to the lack of a strong magnetic field like the Earth's (
more).
Our next step will be to look for other features in the
upper atmosphere, as well as investigating the Great Cold Spot itself in
more detail.»
The best possible observations of the detached layer are made in ultraviolet light because the small haze particles which populate this part of Titan's
upper atmosphere scatter short wavelengths
more efficiently than longer visible or infrared wavelengths.
1) the
atmosphere (which can also be subdivided into northern and southern hemispheres, and even into Hadley Cells) all with fairly short time constants 2) the
upper ocean — time constant on the order of years to decades 2a) the biosphere — time scale from 1 year to decades and even centuries and millennia for some processes 3) abyssal ocean (timescale of many decades to ~ a century or
more) 5) the geosphere — timescale of millennia to eons.
On its current trajectory, Cassini has also taken the first - ever in - situ samples of Saturn's
atmosphere, and Linda Spilker, the Cassini project scientist, said those early results suggest that the chemical and dynamic interactions between particles from the planet's rings and the planet's
upper atmosphere are «
more complex... than we had both anticipated.»
Amid the gold - rush
atmosphere of recent months, however, something very strange has emerged, something
more pertinent to art than to money — a new attitude, now pervasive in the
upper echelons of the art world, about the meaning and experience and value of art itself.
-- warm the
upper atmosphere so it radiates
more heat away?
* If warming warms the lower
atmosphere more than the
upper atmosphere, then the vertical gradients will likely increase.
Wuld this result in a GH effect due to
more IR bouncing off the cooler «
upper atmosphere»?
of anthropogenic CO2 releases that have been taken out of the
atmosphere (over and above the amount taken out of the
atmosphere that balances the natural additions to the
atmosphere), perhaps mainly as a direct biogeochemical feedback (increased CO2 favoring
more rapid biological fixation of C, net flux of CO2 into water until equilibrium for the given storage of other involved chemical species in the
upper ocean) fairly promptly.
Less TOA cooling will occur if bands are placed where, in the
upper atmosphere or near TOA, they absorb
more of the increases in radiation from below from surface + tropospheric (+ lower stratospheric) warming.
Adding
more optical thickness to the same band reduces OLR in that band, cooling at least some portion of the
upper atmosphere up to the TOA level, and increases in OLR outside that band results in some portion of that cooling remaining at full equilibrium (as expained by Andy Lacis).
Add in that if it's the sun, the entire
atmosphere will warm, since there's just simply
more energy put in to the system, whereas if it is CO2 or other blanketing method, there's no extra energy put in, therefore the ground will warm and the
upper air cool (since the
upper air isn't getting the warming from the lower layers it used to get and the lower layers aren't losing the heat they used to).
Yes, but the
upper part of the
atmosphere will remain thin by virtue of the fact that if you add
more gas, the TOA goes to a higher altitude.
Demand is not as sexy as giant wind turbine platforms being towed out to sea or strung up on steel kites into the
upper atmosphere, but demand side effciences are faster, less costly, and
more effective.
For the
upper -
atmosphere cooling, I simply remark that infrared coming up from below is blocked
more, as
more greenhouse gases are added, so of course it's cooler above the blocking.
As
more optical thickness is added to a «new» band, it will gain greater control over the temperature profile, but eventually, the equilibrium for that band will shift towards a cold enough
upper atmosphere and warm enough lower
atmosphere and surface, such that farther increases will cool the
upper atmosphere or just that portion near TOA while warming the lower
atmosphere and surface — until the optical thickness is so large (relative to other bands) that the band loses influence (except at TOA) and has little farther effect (except at TOA).
The
upper layers of the earth's oceans are a lead suspect for absorbing
more heat that otherwise would remain in the
atmosphere.
For instance, back in the 1960s, simple climate models predicted that global warming caused by
more carbon dioxide would lead to cooling in the
upper atmosphere (because the heat is getting trapped at the surface).
The NCAR scientists now state these satellites still see there is
more energy radiation entering the
upper atmosphere than leaving it, in whatever part of the spectrum.
The ITCZ lies at the foot of the ascending branch of the Hadley circulation, and the circulation transports energy in the direction of its
upper branch, because energy (or,
more precisely, moist static energy) usually increases with height in the
atmosphere.
Note that this argument applies to all levels of the
atmosphere, including the
upper levels where carbon dioxide is relatively less abundant, and that the line of reasoning also becomes
more potent (in the sense that less additional warming is forced) the
more carbon dioxide that either humans or nature emit.
All that the gravito - thermal GHE does is redistribute the heat from the only energy SOURCE the Sun,
more to the surface (the 33K G - T) and less to the
upper troposphere (the even larger NEGATIVE -LRB--35 C) ANTI-GREENHOUSE EFFECT) from the center of mass of the
atmosphere at 5.1 km to the top of the troposphere.
During a cooling phase, surface
atmosphere could cool as heat is transported to
upper atmosphere by
more intense weather and then radiates away.