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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

R.M. MacQueen ,
W.C. Davidson  and
I. Mann
R.M. MacQueen
Affiliation:
Department of Physics, Rhodes College, Memphis, TN 38112
W.C. Davidson
Affiliation:
Department of Physics, Rhodes College, Memphis, TN 38112
I. Mann
Affiliation:
Max Planck Institut, Katlenberg-Lindau, FRG

Abstract

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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
Information
International Astronomical Union Colloquium , Volume 150: Physics, Chemistry and Dynamics of Interplanetary Dust , 1996 , pp. 349 - 352
Copyright
Copyright © Astronomical Society of the Pacific 1996

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