Coronal mass ejections: acceleration and surface associations

Coronal mass ejections: acceleration and surface associations

The fact that eruptive-prominence-associated coronal mass ejection events may be accelerated over significant heights and times in the corona complicates the determination of possible surface or low-coronal associations. A specific example of one such eruptive-prominence-associated event, observed i...

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Veröffentlicht in:Solar physics 1985-02, Vol.95 (2), p.359-361
1. Verfasser: MACQUEEN, R. M
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Sprache:eng
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Astronomy
Corona. Coronal loops, streamers, and holes
Earth, ocean, space
Exact sciences and technology
Solar physics
Solar system
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container_title Solar physics
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creator MACQUEEN, R. M
description The fact that eruptive-prominence-associated coronal mass ejection events may be accelerated over significant heights and times in the corona complicates the determination of possible surface or low-coronal associations. A specific example of one such eruptive-prominence-associated event, observed in both the inner and outer solar corona on Aug. 5, 1980, is used to illustrate the magnitude of the uncertainty of determining an onset time of the ejection. It is noted that such uncertainties may influence statistically determined associations.
doi_str_mv 10.1007/BF00152412
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source SpringerNature Journals; EZB-FREE-00999 freely available EZB journals
subjects Astronomy
Corona. Coronal loops, streamers, and holes
Earth, ocean, space
Exact sciences and technology
Solar physics
Solar system
title Coronal mass ejections: acceleration and surface associations
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