Sentences with phrase «upper atmosphere more»

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.
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