Loudzoo
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Thats my simple question!
The discussion centers on the ability of longwave infrared (IR) radiation to heat ocean waters. Participants clarify that while IR does heat water, it does so at a minimal rate compared to shortwave radiation, primarily contributing to evaporation rather than increasing the bulk temperature of the ocean. The IPCC estimates that a doubling of CO2 in the atmosphere increases radiative forcing by 3.7 W/m², affecting only the top few molecules of water. Ultimately, the consensus indicates that increased atmospheric back radiation may not significantly raise ocean temperatures but could slow cooling processes.
PREREQUISITESClimate scientists, oceanographers, environmental researchers, and anyone interested in the interactions between atmospheric conditions and ocean temperatures.
Loudzoo said:IR does not penetrate below 1cm
... not "wrong," into a "semantic ditch," perhaps. If you're going to give me all the solar radiation that penetrates further than 1 mm by the Kebes plot (shorter than 2 μm), you've given me 80 - 90% of the IR. If you define IR as only that radiation that is absorbed in 1 mm or less, and ignore the 0.8 - 2 μm gap between visible and IR acknowledged by a specific argument, you're losing a lot of energy.Loudzoo said:Where am I going
What is "back radiation?"Loudzoo said:Can an increase in Atmospheric back radiation
Not being "flip" with you --- just wanted to be sure we're both working from the same initial set of ideas/postulates/principles.Loudzoo said:Heat moves from hot to cold obviously.
Welcome to the wonderful world of energy "balances" in non-equilibrium systems. The system we're "analyzing" (hah!) has as heat sources the sun, ~ 10-4steradians at ~ 5800 K or 1-1.3 kW/m2 at Earth surface, and crustal heat leak of 10-30 mW/m2, negligible. The heat sink is 4π steradians at ~ 4 K, the CMB. What else do we know? Some fraction of incident solar radiation is reflected, what fraction is subject to some uncertainty; some fraction is transmitted, very small through the atmospheric "halo", but enough to illuminate an otherwise totally eclipsed moon; and, some fraction is absorbed by atmo-, hydro-, and lithospheres, exchanged by conduction, convection, and radiation, and radiated to the CMB.Loudzoo said:And quite frankly I'm confused!
Loudzoo said:I understand the popular theory well enough but I don't understand the physical process of how additional CO2 in the atmosphere can lead to higher ocean temperatures. Can you help me?