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The Role of Particle Size in Producing the F- Coronal Scattered Brightness
Published online by Cambridge University Press: 27 February 2018
Abstract
Motivated by new infrared observations, we examine the contribution of various size intervals of interplanetary dust particles to visible and infrared scattered radiances of the solar F-corona, employing Mie theory and particle size distributions based upon differing interpretations of lunar microcrater evidence and interplanetary flux measurements.
- Type
- IX. Zodiacal Light and Thermal Emission
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- Copyright © Astronomical Society of the Pacific 1996