till fifth and higher – six gradations). The contribution is calculated in percents from
the total value. Results are output to the resulting file.
The second stage is studying the dependences of three calculated value on solar
zenith angle. There are consequent questions:
Input optical depths:
Input single scattering albedo values:
Input phase function parameters:
Input surface albedo:
The answers the similar to above considered.
The program calculates desired characteristics ad output them to the resulting
file as functions of the solar zenith angle for all input combinations.
The third stage is studying dependences of desired values on the optical thickness.
There are sequent questions:
Input sun zenith angles (grad):
Input single scattering albedo values:
Input phase function parameters:
Input surface albedo:
Answers are similar to above considered. The program calculates desired
characteristics as functions of all combinations of input parameters and output
result to resulting file.
13.6.3 Requirements to the Report
Compile a concise report reflecting the principal stages and the obtained results of
the performed exercise in form of tables and plots (graphs).
It is needed:
– Plotting obtained dependences (diagrams present the result in case of distribution over interaction ratio).
– Describing (and physically interpreting if possible) obtained dependences.
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13 Monte-Carlo Method for the Solar Irradiance Calculation
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