Magnetic reconnection flares in the protoplanetary nebula and the possible origin of meteorite chondrules

A possible episodic heating mechanism that could account for chondrule formation is discussed. The mechanism involves the transient release of energy as a result of magnetic flares in the corona of the protosolar nebula. The possible magnetic behavior of the protosolar nebula is outlined, based on m...

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Veröffentlicht in:Icarus (New York, N.Y. 1962) N.Y. 1962), 1989-09, Vol.81 (1), p.74-91
Hauptverfasser: Lavy, Eugene H., Araki, Suguru
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Sprache:eng
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