SPECTRUM LINE INTENSITY AS A SURROGATE FOR SOLAR IRRADIANCE VARIATIONS

被引：38

作者：

LIVINGSTON, WC

WALLACE, L

WHITE, OR

机构：

[1] NATL OPT ASTRON OBSERV,KITT PEAK NATL OBSERV,TUCSON,AZ 85726

[2] LAZY FW RANCH,MANCOS,CO 81328

来源：

SCIENCE | 1988年 / 240卷 / 4860期

关键词：

D O I：

10.1126/science.240.4860.1765

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

引用

页码：1765 / 1767

页数：3

共 13 条

[1] SOLAR LUMINOSITY FLUCTUATIONS AND ACTIVE REGION PHOTOMETRY [J].

CHAPMAN, GA ;

HERZOG, AD ;

LAWRENCE, JK ;

SHELTON, JC .

ASTROPHYSICAL JOURNAL, 1984, 282 (02) :L99-L101

[2]

FOUKAL P, IN PRESS ASTROPHYS J

[3] COMPARISON OF HEII 304-A AND HEI 10830-A SPECTROHELIOGRAMS [J].

HARVEY, JW ;

SHEELEY, NR .

SOLAR PHYSICS, 1977, 54 (02) :343-351

[4]

HOYT D, 1988, TN194STR NATL CTR AT

[5] SOLAR LUMINOSITY VARIATION .4. THE PHOTOSPHERIC LINES, 1976-1980 [J].

LIVINGSTON, W ;

HOLWEGER, H .

ASTROPHYSICAL JOURNAL, 1982, 252 (01) :375-385

[6]

LIVINGSTON W, 1987, ASTROPHYS J, V413, P808

[7] ONE-COMPONENT AND MULTICOMPONENT MODELS OF UPPER PHOTOSPHERE BASED ON MOLECULAR SPECTRA .1. VIOLET SYSTEM OF CN(0,0) [J].

MOUNT, GH ;

LINSKY, JL ;

SHINE, RA .

SOLAR PHYSICS, 1973, 32 (01) :13-30

[8] USING CN LAMBDA 3883 SPECTROHELIOGRAMS TO MAP WEAK PHOTOSPHERIC MAGNETIC FIELDS [J].

SHEELEY, NR .

SOLAR PHYSICS, 1971, 20 (01) :19-&

[9] SOLAR LUMINOSITY VARIATION .3. CALCIUM K VARIATION FROM SOLAR MINIMUM TO MAXIMUM IN CYCLE 21 [J].

WHITE, OR ;

LIVINGSTON, WC .

ASTROPHYSICAL JOURNAL, 1981, 249 (02) :798-816

[10] VARIABILITY OF CHROMOSPHERIC AND PHOTOSPHERIC LINES IN SOLAR CYCLE-21 [J].

WHITE, OR ;

LIVINGSTON, WC ;

WALLACE, L .

JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 1987, 92 (D1) :823-827

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