DETERMINATION OF VELOCITY AMPLITUDE OF TOTAL PHOTOSPHERIC MOTION FIELD .1. USE OF WEAK AND MODERATELY WEAK LINES

被引：7

作者：

KONDRASHOVA, NN ^{[1
]}

GURTOVENKO, EA ^{[1
]}

机构：

[1] ACAD SCI UKSSR, MAIN ASTRON OBSERV, KIEV, UKSSR

来源：

关键词：

D O I：

10.1007/BF00153666

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：291 / 298

页数：8

共 9 条

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[2]

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[3]

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[4]

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[5]

GURTOVENKO EA, 1969, ASTROMETR ASTROFIZ, V8, P77

[6]

GURTOVENKO EA, 1972, ASTROMETR ASTROFIZ, V16, P77

[7]

HOLWEGER H, 1967, Z ASTROPHYS, V65, P365

[8]

JAGER CD, 1972, SOL PHYS, V25, P71

[9] SOLAR VELOCITY FIELDS - 5-MIN OSCILLATIONS AND SUPERGRANULATION [J].

TANENBAUM, AS ;

WILCOX, JM ;

FRAZIER, EN ;

HOWARD, R .