A TWISTED FLUX MODEL FOR SOLAR PROMINENCES .2. FORMATION OF A DIP IN A MAGNETIC-STRUCTURE BEFORE THE FORMATION OF A SOLAR PROMINENCE

被引：0

作者：

DEMOULIN, P ^{[1
]}

PRIEST, ER ^{[1
]}

机构：

[1] UNIV ST ANDREWS, DEPT APPL MATH, ST ANDREWS KY16 9SS, SCOTLAND

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中图分类号：

P1 [天文学];

学科分类号：

0704 ;

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引用

页码：360 / 368

页数：9

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