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I am trying to model surface temperatures on Mars.
Coming up with insolation received at the various latitudes was fairly simple, the equations are found at the bottom. Assuming a known rate of insolation at each latitude from the equations below, and a known albedo and thermal inertia for each location on the surface. How would one find the surface temperature for a location on the planet? I have thought of using the Stefan-Boltzmann law, but I don't know how to account for the thermal inertia of the surface. I am willing to discount the greenhouse effect for now and assume a transparent atmosphere, but eventually the model will increase in complexity. If anyone has any insight please post here or email me, rpavlick3[NO*SPAM]yahoo.com. Thanks, Ryan Insolation Equations ____________________ The sun has an energy flux, Lo, applying the the inverse square law, the flux density at Mars would be: flux density at Mars = solar flux * (pi/4) * (sun-Mars distance)^2. The sun-Mars distance being: distance = (semi-major axis)(1 - eccentricity^2) / (1 + eccentricity cosine [solar longitude - longitude of perihelion]) Now the irradiance for a time of year and latitude can be found: irradiance = flux density * cosine(zenith angle), cozine(zenith angle) = sin(declination)sin(lat) + cos(lat)cos(dec)cos(hour angle). The solar declination is a function of solar longitude and the axial tilt of the Mars, sin(declination) = sin(obliquity)sin(solar longitude). This can integrated to find: daily insolation = (flux density/pi)(cos(dec)cos(lat)sin(H) = sin(dec)sin(lat)) H = half day length = -tan(dec)* -tan(lat) |
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