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Detailed Reference Information |
Misconi, N.Y. (1993). The spin of cosmic dust: rotational bursting of circumsolar dust in the F corona. Journal of Geophysical Research 98: doi: 10.1029/93JA01521. issn: 0148-0227. |
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This paper will list, investigate, and evaluate the various spin mechanisms for cosmic dust particles that have been suggested in the literature. This evaluation will concentrate on the possibility of particle fragmentation (rotational bursting) of cosmic dust. The importance of particle fragmentation is manifested by the fact that dust particle size distribution will be changed. More importantly, repeated fragmentation of interplanetary dust particles will give rise to some of the observed ''&bgr; meteoroids.'' Some of these particles are driven out of the solar system and into interstellar space by solar radiation pressure. If this mass loss mechanism is taking place in stellar systems, then it becomes a source for interstellar dust. This paper also addresses the possibility that massive rotational bursting by circumsolar dust particles is taking place in the F corona region. This rotational bursting of F coronal dust could be taking place because of the classical ''Paddack effect,'' along with a similar spin mechanism suggested by the author, and caused by coronal mass ejections. ¿ American Geophysical Union 1993 |
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Abstract |
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Keywords
Interplanetary Physics, Interplanetary shocks, Interplanetary Physics, Solar wind plasma, Interplanetary Physics, Flare and stream dynamics |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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