http://arxiv.org/abs/1903.04960
Bodies in the outer Solar System may consist of, or be covered by, solid ammonia. Their temperature depends on its emissivity. We calculate that emissivity as a function of frequency, angle and polarization and convolve it with a Planck function to obtain its integrated emissivity.
S. Wang and J. Katz
Wed, 13 Mar 19
41/125
Comments: 7 pp., 3 figs