Solving Atmosphere Layers: Deriving Equations for Venus Surface & Atmos. Temp.

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SUMMARY

The discussion focuses on deriving equations for the temperature of Venus's surface and atmosphere based on its one-layer atmosphere model. Given that 19% of the incoming solar radiation (615 Wm-2) is absorbed, the equations must account for the remaining 81% and the thermal equilibrium of the atmosphere. The key equations derived will relate the absorbed and emitted radiation to the temperatures at the top of the atmosphere and the surface of Venus.

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1. Homework Statement

Consider a one layer atmosphere for the planet Venus. 19% of incoming solar radiation is absorbed by the atmosphere. 99% of the outgoing radiation is absorbed by the atmosphere. The incoming radiation, E, as measured by satellite is 615 Wm-2.

1) Derive two equations, one for the top of the atmosphere and the other for the Venusian surface in terms of x, y and E. Solve for the surface and atmospheric temperatures.



Homework Equations


None we need to create the equations but i do not know where to start.


The Attempt at a Solution


Please help! i have no clue where to start
 
Physics news on Phys.org
If 19% of the incoming radiation from the sun is absorbed, what happens to the other 81%? If the whole atmosphere is in thermal equilibrium, what must the lower atmosphere radiate back out?

AM
 

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