In a stellar atmosphere, the radiation intensity passing through various layers is given as Iout = (Iin)e(−τ) .
a) How large must the optical depth through a material be for the material to absorb 50% of the incident photons, as in the solar photosphere?
b) Regions in the solar chromosphere have an optical depth of τ = 0.1. What fraction of the Sun’s radiation intensity is transmitted through this region?
c) In the optically thin limit, Iout = Iin*e−τ reduces to Iout = Iin*(1 − τ ). Based on this definition, are either the photosphere or chromosphere considered to be optically thin?
In a stellar atmosphere, the radiation intensity passing through various layers is given as Iout =...
10 points! Consider radiation with wavelength λ passing through a planetary atmosphere comprised entirely of co2 with a molecular absorption coefficient of ka of 10-2"m2/molecule. The atmosphere is isothermal with a surface pressure of 600 Pa, a scale height of 10 km, and gravitational acceleration of 3.71ms 2. Calculate the height and pressure of unit optical depth assuming a zenith angle of a) 0° and b) 45 6