STUDY OF THE POST-FLARE LOOPS ON 29 JULY 1973 .1. DYNAMICS OF THE X-RAY LOOPS

被引：38

作者：

NOLTE, JT

GERASSIMENKO, M

KRIEGER, AS

PETRASSO, RD

SVESTKA, Z

机构：

[1] SPACE RES LAB,UTRECHT,NETHERLANDS

[2] UNIV CALIF SAN DIEGO,DEPT PHYS,LA JOLLA,CA 92093

来源：

SOLAR PHYSICS | 1979年 / 62卷 / 01期

关键词：

D O I：

10.1007/BF00150139

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We derive an empirical model of the X-ray emitting post-flare loops observed during the decay phase of the 29 July 1973 flare. We find that the loops are elliptical, with the brightest emitting region at the tops. We determine the height, velocity of growth, and ratio of height to width of the loops at times from 3 to 12 hr after the flare onset. © 1979 D. Reidel Publishing Co.

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页码：123 / 132

页数：10

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