Article ID Journal Published Year Pages File Type
8134095 Icarus 2018 12 Pages PDF
Abstract
Trial scattering calculations demonstrate that the observed strong backscattering most likely arises from particles in the size range 1-20 µm. 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 ∼0.01 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
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