Fig 3.1 (presumably from Pierrehumbert's book) shows that
the radiation balance at TOA depends on surface temperature.
(in the sentence you responded to, i should have said
radiation balance at the tropopuase, not tropospheric radiation balance).
Moreover, the loss of sea ice would have altered the planetary albedo, causing the planet to warm until clouds cover had increased enough for
the radiation balance at the TOA to be restored.
In addition, observational records are available for surface temperature (space - based monitoring, in situ monitoring, and proxy data) and
the radiation balance at the top of the atmosphere.
It's defined there as, «the effect of clouds on
the radiation balance at the top of the atmosphere.»
In the futuristic climate scenarios, differences in the time of day of precipitation had very important impacts on
the radiation balance at the surface.
Callendar's calculations focused on
the radiation balance at the surface, whereas Arrhenius had (correctly) focussed on the balance at the top of the atmosphere.
How does CO2 increase affect the water vapor exchange, the cloud amount and its incredibly complex feedbacks involving aerosols, precipitation efficiency, and the resultant
radiation balance at the 1 - 2 meter height thermometer shelters where humanity defines his / her climate?
In that survey, it was almost universal that groups tuned for
radiation balance at the top of the atmosphere (usually by adjusting uncertain cloud parameters), but there is a split on pratices like using flux corrections (2 / 3rds of groups disagreed with that).
Not exact matches
Examining the
radiation balance as a function of latitude, we see that tropical regions have a
radiation surplus; the deficit over the higher latitudes peaks
at the poles.
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.
There is a
balance in the task force recommendation, said Dr. Anthony D'Amico, chief of genitourinary
radiation oncology
at Brigham and Women's Hospital and the Dana Farber Cancer Institute, in Boston.
An energy surplus there gives rise to warming which causes a rise in infra - red
radiation leading to more energy loss
at the top of the atmosphere and hence a trend back into energy
balance (negative feedback).
What happens
at the «top of atmosphere» — the level where outgoing
radiation leaves for space, not itself a very easy concept — is the restoration of equilibrium, the increase in temperature that, through Helmholtz - Boltzmann
at the Earth's brightness temperature 255K, restores the
balance between incoming and outgoing energies.
Earth's energy
balance In response to a positive radiative forcing F (see Appendix A), such as characterizes the present - day anthropogenic perturbation (Forsteret al., 2007), the planet must increase its net energy loss to space in order to re-establish energy
balance (with net energy loss being the difference between the outgoing long - wave (LW)
radiation and net incoming shortwave (SW)
radiation at the top - of - atmosphere (TOA)-RRB-.
The change in
radiation balance is more heating of the oceans
at one side (specifically high in the subtropics, as expected), but more heat released
at higher altitudes, thus somewhere acting as a net negative feedback to higher sea surface temperatures.
But the remaining heating in the pipeline is proportional to the system's climate sensitivity, since the planet is less efficient
at adjusting to
radiation balance in a highly sensitivity system.
Gavin told me years ago
at RC that whenever Triana was in place, we'd still need a corresponding instrument on the night side to get a simple answer to the
radiation balance question.
Using satellite
radiation balance measurements and ocean heaing measurements the earth appears to be gaining heat
at a rate of 0.6 Watts / M2 on average.
Miskolczi is saying that this is nonsense, that
radiation must
balance at the top of the atmosphere.
Lacis points out that only outgoing
radiation can
balance the global energy budget of the Earth; as clearly the convection and conduction ends
at the boundary of the atmosphere.
radiative forcing a change in average net
radiation at the top of the troposphere resulting from a change in either solar or infrared
radiation due to a change in atmospheric greenhouse gases concentrations; perturbance in the
balance between incoming solar
radiation and outgoing infrared
radiation
Note that the inversion
at the tropopause is entirely a result of ozone reacting with incoming solar
radiation and particles so any change in the ozone creation / destruction
balance is going to affect the air circulation below the tropopause.
Effectively, infrared
radiation emitted to space originates from an altitude with a temperature of, on average, — 19 °C, in
balance with the net incoming solar
radiation, whereas the Earth's surface is kept
at a much higher temperature of, on average, +14 °C.
The main place this attempt
at modelling breaks down, IMHO, is assessing the effect of a change in
radiation balance on a change in global temperature, without feedbacks.
Until the surface warms to a level that emits
radiation at a rate that is
balanced with the higher level of energy capture there will continue to be «net energy capture».
He was right that surface temperature is determined by the
balance between incoming solar energy and outgoing infrared
radiation, and that the
balance that matters is the
radiation budget
at the top of the atmosphere.
«Because the solar - thermal energy
balance of Earth [
at the top of the atmosphere (TOA)-RSB- is maintained by radiative processes only, and because all the global net advective energy transports must equal zero, it follows that the global average surface temperature must be determined in full by the radiative fluxes arising from the patterns of temperature and absorption of
radiation.»
The job of the
radiation module is to calculate the solar heating rate profiles and the thermal cooling rate profiles, including the energy deposition
at the ground surface, as well as the energy
balance at the top of the atmosphere for the specified climate variable distribution
at each grid box.
Then that lowest atmosphere layer emit and a 50 - 50 split sends it half up and half down; and the up ward is again absorbed by a higher and now cooler layer; which in turn emits but now
at a lower temperature; until finally some much higher and much cooler layer gets to emit
radiation that actually escapes to space and that radiating temperature is the one that must
balance with the incoming TSI insolation rate.
Over millions of years the earth has arrived
at a temperature
balanced between incoming solar energy and outgoing
radiation of energy to space.
Drivers of the land climate system have larger effects
at regional and local scales than on global climate, which is controlled primarily by processes of global
radiation balance.
It also
balances at the surface including
radiation, latent heat, heat flux, and it
balances within the atmosphere.
Yes, inert gases do absorb incident Solar
radiation in the UV and visible spectra, so the atmosphere warms to radiative
balance, and the temperature
at the base of the atmosphere determines (or «supports») the surface temperature.
1) The influence of methane on the Earth energy
balance is not due to the absorption peak
at 3.3 µm because that wavelength has very little role in solar
radiation and even less in IR radiated from the Earth.
Surface temperature must therefore increase, just enough for the LW
radiation that is rejected to space
at TOA to
balance the SW
radiation that is absorbed.
(1) Using physics: Palmer et
at (2001) Importance of the deep ocean for estimating decadal changes in Earth's
radiation balance, in GRL Vol 38, L13707, doi: 10.1029 / 2011GL047835 (2) Using observations: von Schuckmann et al (2001) How well can we derive Global Ocean Indicators from Argo data?
It will not rise
at all if the absorption is
balanced by an equal amount of emission (as would occur if its emissivity would be increased from a change in its molecular composition — e.g. the formation of ozone from UV
radiation or mixing a little CO2 within it).
There is no relation between the
radiation flows exchanged by surface and air (whose net
balance is about zero) and the
radiation from the top of the air lost to the cosmos some kilometres above the surface; the cooling of the «top of the air»
at mid and high latitudes is compensated by advection of humid air from mid latitudes.
For instance, if the outgoing and incoming
radiation are
balanced at 270 ppm, then let's guess WHAT YEAR they said the incoming
radiation was 343 / w / m ^ 2 and outgoing was 103?
In particular, in layers of air
at different altitudes they found a different
balance between the way clouds trapped
radiation and warmed the planet, or reflected sunlight back into space and cooled it.
The
balance between incoming and outgoing
radiation at TOA is what determines the Earths atmospheric average temperature.
In the absence of absorption of terrestrial
radiation by the atmosphere (and with the other caveats about still having the same albedo and such), that average temperature would have to be 255 K
at the surface because of radiative
balance and then the temperature would decrease with height
at the lapse rate from there.
There certainly are, the energy
balance is done
at the surface of «h», and the area is the same for both outgoing and incoming
radiation, «Ac», since «h» is immersed in «c».
Notice that the Earth System mean temperature I had to use to provide 240 Watts / m ^ 2 of
radiation to Space to
balance the input absorbed from by the Earth System from the Sun was 255 K. However, the actual mean temperature
at the Surface is closer to 288 K.
That is determined by consideration of the absorption of the atmosphere of terrestrial
radiation (and
radiation emitted by the atmosphere), which essentially ends up determining
at what altitude the temperature has to be determined via radiative
balance between the Earth system (earth + atmosphere) and the sun and space [which for the earth system with its current albedo is ~ 255 K].
Ira said: «Notice that the Earth System mean temperature I had to use to provide 240 Watts / m ^ 2 of
radiation to Space to
balance the input absorbed from by the Earth System from the Sun was 255 K. However, the actual mean temperature
at the Surface is closer to 288 K.
The greenhouse effect, by affecting the rate
at which the earth emits
radiation back out into space for a given surface temperature, causes the earth's temperature to warm in order to maintain radiative
balance.
Notice that the upward longwave flux
at TOA is 240 W / m ² — this
balances the absorbed solar
radiation.
As of November 2014, there were 14 Earth System Models from 12 centers in eight countries that modeled temperature, soil moisture, and solar
radiation at a daily resolution for
at least one of the three RCPs (S1 Table)(Note: all Earth System Models that we used include feedbacks of plant production on water
balance).