A change
in radiative characteristics alone does not make more energy available because solar insolation at TOA remains the same, mass stays the same and gravity stays the same.
ii) The real question is whether changes
in radiative characteristics alone can result in energy being transferred from the radiative SDL to the mechanical AAL so as to add to the energy in that latterLoop and thereby significantly increase the temperature of atmosphere and surface by in turn increasing the time delay in the transmission of energy through the system.
iv) The answer must depend on whether any slowing down of the throughput of radiation from a mere change
in radiative characteristics within the SDL would overwhelm the flexibility of the adiabatic processes in the AAL.
Not exact matches
It is the
radiative characteristics of the atmosphere that here force ΔOHC not an increase
in atmospheric temperature, prior or otherwise.
This essay is an attempt to link real world observations (the failure of surface temperatures to rise
in tandem with atmospheric CO2) to basic physics and thereby show why the
radiative characteristics of Greenhouse Gases can not increase the surface temperature of a planet when atmospheric mass, the strength of the gravitational field and the power of insolation at the top of the atmosphere remain the same.
Absent
radiative warming it will still warm through conduction and convection and it will cool radiatively because all matter above absolute zero radiates and I'm pretty sure the nitrogen
in our atmosphere is matter and it has a temperature above absolute zero therefore it radiates a continuous black body spectrum
characteristic of that temperature.
The current impasse
in climate science has arisen because AGW proponents say that simply altering the
radiative characteristics of constituent molecules within the atmosphere can result
in a change
in system equilibrium temperature without any need for an increase
in mass, gravity or insolation.
If anything else tries to disturb the temperature (or more accurately energy content) derived from those 3
characteristics alone then all one sees is a change
in circulation adjusting the flow of energy throughput to keep top of atmosphere
radiative balance stable.
Is this point only about the
radiative characteristics of the H2O vapour, and the assumption that relative and / or specific humidity should rise thanks to CO2 - induced increased evaporation, which
in turn would increase downwelling heat radiation — or just the part that slightly hotter surface (due to CO2) also emits more heat to be trapped by the vater vapour?
Based on the understanding of both the physical processes that control key climate feedbacks (see Section 8.6.3), and also the origin of inter-model differences
in the simulation of feedbacks (see Section 8.6.2), the following climate
characteristics appear to be particularly important: (i) for the water vapour and lapse rate feedbacks, the response of upper - tropospheric RH and lapse rate to interannual or decadal changes
in climate; (ii) for cloud feedbacks, the response of boundary - layer clouds and anvil clouds to a change
in surface or atmospheric conditions and the change
in cloud
radiative properties associated with a change
in extratropical synoptic weather systems; (iii) for snow albedo feedbacks, the relationship between surface air temperature and snow melt over northern land areas during spring and (iv) for sea ice feedbacks, the simulation of sea ice thickness.
The strength of
radiative cooling
in turn depends on the
characteristics of the clouds formed by the condensed vapor.
Turner D. D., M. D. Shupe and A. B. Zwink (April 2018):
Characteristic Atmospheric
Radiative Heating Rate Profiles
in Arctic Clouds as Observed at Barrow, Alaska.
The case appears to be similar with some of the basics of the theory of human - caused climate change, too — basics, such as the
radiative characteristics of CO2 and other «greenhouse» gases, or the importance of the greenhouse effect
in the natural regulation of our planetary temperature, are firmly established.
Jensen, M.P., and A.D. Del Genio, 2003:
Radiative and microphysical
characteristics of deep convective systems
in the tropical Western Pacific.
There are still questions about the assumed figures and also the emissivity and
radiative characteristics of gases
in our atmosphere.
The direct CO2
radiative forcing is the change
in infrared
radiative fluxes for a doubling CO2 (typically from 287 to 574 ppm), without any feedback processes (e.g. from changing atmospheric water vapor amount or cloud
characteristics.)