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On the Solar Dust Ring(s)

Published online by Cambridge University Press:  12 April 2016

T. Mukai
T. Mukai*
Affiliation:
Kanazawa Institute of Technology Nonoichi, Ishikawa 921 Japan

Abstract

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Based on a mechanism to form the solar dust ring, it is proved that the observed peak in infrared F-corona cannot be explained by silicate type grain alone. Preliminary analysis on the recent infrared data of F-corona by Maihara et al.(1984) has suggested that the ring particle has different physical properties compared with the dust grains, which produce the background F-corona.

Type
I. Zodiacal Light and F-Corona: Observations
Information
International Astronomical Union Colloquium , Volume 85: Properties and Interactions of Interplanetary Dust , 1985 , pp. 59 - 62
Copyright
Copyright © Reidel 1985

References

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