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.
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© 1985 D. Reidel Publishing Company
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Mukai, T. (1985). On the Solar Dust Ring(s). In: Giese, R.H., Lamy, P. (eds) Properties and Interactions of Interplanetary Dust. Astrophysics and Space Science Library, vol 119. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5464-9_13
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DOI: https://doi.org/10.1007/978-94-009-5464-9_13
Publisher Name: Springer, Dordrecht
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