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On the Solar Dust Ring(s)
Published online by Cambridge University Press: 12 April 2016
Abstract
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
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- Copyright © Reidel 1985
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