This might mean that it has a hot
outer atmosphere heated by bubbling convection cells on the young planet — sort of a Jupiter on steroids.
Not exact matches
The sun can unleash solar storms and solar flares — bursts of X-rays and ultraviolet light — that
heat Earth's
outer atmosphere, causing the air to expand and rise.
The release of CO2 into the
atmosphere contributes to the trapping of
heat that would otherwise be emitted into
outer space.
These are spicules, and despite their abundance, scientists didn't understand how these jets of plasma form nor did they influence the
heating of the
outer layers of the sun's
atmosphere or the solar wind.
Because planet b is tidally locked and the
outer atmosphere is so efficient at re-radiating
heat, its «nightside» stays dark and cold (top), unlike bands of even temperature on a Jupiter - like planet (shown below — more).
If the energy delivered to Earth by the Sun or by impacts (or both) were 40 % greater, the Earth would experience a runaway greenhouse.3 That is, more water would evaporate from Earth's surface, so too much
heat trying to escape into
outer space would be blocked by water vapor in the
atmosphere.
The moss observations are thus helping to locate the as yet elusive energy source that is responsible for
heating the Sun's
outer atmosphere.
The main objectives of the mission include obtaining new data on solar activity to help to better forecast space - weather events like solar flares which can directly impact Earth and orbiting satellites, trace the flow of energy from the Sun, better understand how the Sun's
outer atmosphere is
heated, and explore the physical mechanisms which accelerate the solar wind.
These winds and the
heat rising from its interior create bands in Saturn's
outer atmosphere.
The premise of Lindzen's hypothesis was that as the climate warms, the area in the
atmosphere covered by high cirrus clouds will contract to allow more
heat to escape into
outer space, similar to the iris in a human eye contracting to allow less light to pass through the pupil in a brightly lit environment.
But that's actually an understatement by Gallup, since more than 97 % of the world's climatologists say that those carbon gases, which are given off by humans» burning of carbon - based fuels, are causing this planet's temperatures to rise over the long term, as those carbon gases accumulate in the
atmosphere and also block the
heat from being radiated back into
outer space.
Greenhouse gases such as carbon dioxide accumulate in the
atmosphere and trap
heat that normally would exit into
outer space.
The Sun is not
heating the
atmosphere and
outer crust from zero K each day.
(1) The UF6 gas at the
outer rim of a gas centrifuge is at many
atmospheres of pressure and room temperature (or optionally a little warmer, as supplied by a
heating coil), per these pictures of an operating centrifuge cascade.
For the first time, IRIS is making it possible to study these explosive phenomena in enough detail to determine their role in
heating the
outer solar
atmosphere.
I said it was a consequence of the fact that the two boundaries of the
atmosphere —
outer space above us and the ocean below — are an infinite and a near - infinite
heat - sink respectively, which helping to keep the atmospheric temperature within a narrow interval.
Thus
heat from the Sun «creeps» up the temperature gradient in the
atmosphere, and then further up the steeper temperature gradient in the
outer crust, and even further through the mantle until, whether you choose to believe it or not, it actually supports the core temperature, preventing the core from cooling off, even on planets like Uranus where no energy is created in the core.
The evidence here comes from satellite measurements of infrared radiation escaping from the earth into
outer space, from measurements of sunlight reflected from clouds and from measurements of the temperature the earth's surface or of the troposphere, the roughly 10 km thick layer of the
atmosphere above the earth's surface that is filled with churning air and clouds,
heated from below at the earth's surface, and cooled at the top by radiation into space.
**
Heat would still leave the
atmosphere for
outer space, I would have thought even though there is hypothetically no interchange between
atmosphere and earth.
... he realized the extreme complexity of the temperature control at any particular region of the earth's surface, and also that radiative equilibrium was not actually established, but if any substance is added to the
atmosphere which delays the transfer of low temperature radiation, without interfering with the arrival or distribution of the
heat supply, some rise of temperature appears to be inevitable in those parts which are furthest from
outer space.
It means how HIGH up in the
atmosphere heat radiation occurs into
outer space.
The third reason the interior Antarctic data is important is because there is NOTHING on earth that can drive those surface air temperatures down, except a decrease in the energy content of the
atmosphere, OR direct radiational
heat transfer from the surface to
outer space.
That is a very, very tiny fraction of the entire long wavelength band (10 microns and above, to meters of wavelength) of interest for radiational
heat transfer in the
atmosphere to
outer space.