TEMPORAL CHARACTERISTICS OF THE SOLAR UV FLUX AND HE-I LINE AT 1083 NM

被引：42

作者：

DONNELLY, RF

HARVEY, JW

HEATH, DF

REPOFF, TP

机构：

[1] NATL SOLAR OBSERV,NATL OPT ASTRON OBSERV,TUCSON,AZ 85726

[2] NASA,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1985年 / 90卷 / NA7期

关键词：

D O I：

10.1029/JA090iA07p06267

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：6267 / 6273

页数：7

共 12 条

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[3] DIFFERENCES IN THE TEMPORAL VARIATIONS OF SOLAR UV FLUX, 10.7-CM SOLAR RADIO FLUX, SUNSPOT NUMBER, AND CA-K PLAGE DATA CAUSED BY SOLAR ROTATION AND ACTIVE REGION EVOLUTION
DONNELLY, RF
HEATH, DF
LEAN, JL
ROTTMAN, GJ
[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1983, 88 (NA12): : 9883 - 9888
[4] COMPARISON BETWEEN MGII AND CAII SPECTROHELIOGRAMS
FREDGA, K
[J]. SOLAR PHYSICS, 1971, 21 (01) : 60 - &
[5] HARVEY JW, 1984, NASA C PUBL, V2310, P197
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[7] HEATH DF, 1983, ERL424ARL7 NATL OC A
[8] HEATH DF, 1984, ERL ARL129 NATL OC A
[9] A 3-COMPONENT MODEL OF THE VARIABILITY OF THE SOLAR ULTRAVIOLET FLUX - 145-200 NM
LEAN, JL
WHITE, OR
LIVINGSTON, WC
HEATH, DF
DONNELLY, RF
SKUMANICH, A
[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1982, 87 (NA12): : 307 - 317
[10] LEAN JL, 1985, P INT RAD S HAMPTON