OBSERVATION OF SOLAR SOFT X-RAY COMPONENT - STUDY OF ITS RELATION TO TRANSIENT AND SLOWLY-VARYING PHENOMENA OBSERVED AT OTHER WAVELENGTHS

被引：29

作者：

TESKE, RG

机构：

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

来源：

SOLAR PHYSICS | 1969年 / 6卷 / 02期

关键词：

D O I：

10.1007/BF00150944

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Solar X-rays from 8-12 Å have been observed with an ion chamber photometer and fluxes derived from the observations after an assumption concerning the spectral distribution. The time variation of the X-ray flux correlates well with the radio flux, plage index, and sunspot number. Comparisons of X-ray and optical events are given; flares seem to produce soft X-rays, but some soft X-ray bursts are apparently not associated with flares. The total energy involved in the soft X-ray bursts may be a significant amount of the total flare radiation. © 1969 D. Reidel Publishing Company.

引用

页码：193 / &

共 11 条

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