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Improves h/e radiation
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@@ -6,10 +6,13 @@
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#define R_IDEAL_GAS_EQUATION 8.31 //kPa*L/(K*mol)
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#define ONE_ATMOSPHERE 101.325 //kPa
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#define STEFAN_BOLTZMANN_CONSTANT 0.0000000567 //W/(m^2*K^4)
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#define IDEAL_GAS_ENTROPY_CONSTANT 1164 //(mol^3 * s^3) / (kg^3 * L). Equal to (4*pi/(avrogadro's number * planck's constant)^2)^(3/2) / (avrogadro's number * 1000 Liters per m^3).
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//radiation constants
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#define STEFAN_BOLTZMANN_CONSTANT 0.0000000567 //W/(m^2*K^4)
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#define COSMIC_RADIATION_TEMPERATURE 3.15 //K
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#define AVERAGE_SOLAR_RADIATION 200 //W/m^2. Kind of arbitrary. Really this should depend on the sun position much like solars.
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#define CELL_VOLUME 2500 //liters in a cell
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#define MOLES_CELLSTANDARD (ONE_ATMOSPHERE*CELL_VOLUME/(T20C*R_IDEAL_GAS_EQUATION)) //moles in a 2.5 m^3 cell at 101.325 Pa and 20 degC
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