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Solar Radiation Model
Chris Adderley edited this page Sep 1, 2016
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2 revisions
Solar illumination estimate...
Iv = phi*theta(rvp)*I0 * (r0^2)/(rv^2)
- I0 = dose rate at sun surface
- Iv = dose rate at vessel
- r0 = sun radius
- rv = vessel distance from sun
- rvp = vessel distance from planet surface
- theta = magnetosphere attenuation at vessel height
- phi = solar visibility at part