Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8134095 | Icarus | 2018 | 12 Pages |
Abstract
Trial scattering calculations demonstrate that the observed strong backscattering most likely arises from particles in the size range 1-20â¯Âµm. Our observed backscattering phase curve gives no constraints on the real index of refraction, the particle size distribution or the minimum and maximum particle size cut-offs. However, an upper limit to the imaginary index of refraction of â¼0.01 was required, making these particles quite transparent. Simple spherical scattering calculations including particle size distributions can fit the general characteristics of the phase curve but cannot produce a satisfactory detailed fit.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Uwe Fink, Lyn Doose,