SOLAR SOFT X-RAYS AND SOLAR ACTIVITY .I. RELATIONSHIPS BETWEEN REPORTED FLARES AND RADIO BURSTS, AND X-RAY BURSTS

被引：19

作者：

TESKE, RG

THOMAS, RJ

机构：

[1] Dept. of Astronomy and the McMath-Hulbert Observatory, The University of Michigan, Ann Arbor, Mich.

来源：

SOLAR PHYSICS | 1969年 / 8卷 / 02期

关键词：

D O I：

10.1007/BF00155382

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Soft solar X-rays (8 ≤ gl ≤ 12 Å) were observed from OSO-III. An analysis of the X-ray enhancements associated with 165 solar flares revealed that there is a tendency for a weak soft X-ray enhancement to precede the cm-λ burst and H α flare. The peak soft X-ray flux follows the cm-λ peak by about 4 min, on the average. Additionally, it was found that flare-rich active centers tend to produce flares which are stronger X-ray and cm-λ emitters than are flares which take place in flare-poor active centers. © 1969 D. Reidel Publishing Company.

引用

页码：348 / &

共 30 条

[1] OBSERVATIONS OF SOLAR X-RAY EMISSION IN 8 TO 20 A BAND [J].