Not exact matches
Few realize that our entire solar system is swinging
through space passing
through areas of greater or
lesser energy fields from cosmic particles and background
radiation.
For the same reason, infrared astronomy enables researchers to observe cosmic objects
through large clouds of interstellar dust that scatter infrared
radiation substantially
less than visible light.
Few realize that our entire solar system is swinging
through space passing
through areas of greater or
lesser energy fields from cosmic particles and background
radiation.
In fact, because over 90 % of the solar
radiation passes
through the thin transparent surface layer of the oceans, you should use
less than 10 % of that 161W / m ^ 2 in Stefan - Boltzmann calculations.
Urban areas are also
less adept at getting rid of heat
through thermal
radiation because they produce a greater volume of emissions that trap the heat.
No,
less than 2.5 % of the solar
radiation gets
through the Venus atmosphere, and only 1W / m ^ 2 gets
through at the poles.
I would be looking to know what ranges of
radiation the sun has increased by and whether some bands had decreased,
less solar wind perhaps, allowing more cosmic days
through.
I do not believe that the surface at altitude receives
less radiation than at sea level, in fact it should receive more because it passes
through less atmosphere.
Result:
less radiation gets
through, ergo, more CO2 impedes
radiation.
But the dry air column holds a lot
less energy so when the sun goes down and the surface is no longer heating it
through conduction and
radiation the column cools rapidly hence the great diurnal temperature range of the desert and the almost total lack of diurnal temperature change over the ocean.
It stands to reason that if a human optimum emites 100w / m2 of
radiation through a duration, that earth is emitting much
less per square metre.
Changes in visible and infrared solar
radiation alter the surface temperature by simple heating; other parts of the spectrum can also affect climate,
through paths that are
less direct.
He sent infrared
radiation through a tube filled with carbon dioxide, containing somewhat
less gas in total then would be found in a column of air reaching to the top of the atmosphere.
To summarize; «As height is gained each square meter of air will contain
less «energy per molecule» but will proportionately let more
radiation through from below.
That happens partly
through «new» absorption of
radiation that more or
less used to escape directly from the surface, as well as absorption and re-emission of
radiation that used to get absorbed and re-emitted at lower layers, but now (at higher CO2) does so at higher layers.