HIGH-RESOLUTION SPECTROSCOPY OF DISK CHROMOSPHERE .4. EVIDENCE FOR PROPAGATION AND DISSIPATION OF MECHANICAL ENERGY IN CHROMOSPHERE

被引：20

作者：

CRAM, LE ^{[1
]}

机构：

[1] UNIV SYDNEY,DEPT APPL MATH,SYDNEY,AUSTRALIA

来源：

SOLAR PHYSICS | 1974年 / 37卷 / 01期

关键词：

D O I：

10.1007/BF00157845

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：75 / 83

页数：9

共 19 条

[1]

ATHAY RG, 1970, SOL PHYS, V12, P175, DOI 10.1007/BF00227116

[2] RADIATIVE ENERGY LOSS FROM SOLAR CHROMOSPHERE AND CORONA [J].

ATHAY, RG .

ASTROPHYSICAL JOURNAL, 1966, 146 (01) :223-&

[3] EMISSION CORES IN H-LINES AND K-LINES .5. ASYMMETRIES IN K2 AND K3 [J].

ATHAY, RG .

SOLAR PHYSICS, 1970, 11 (03) :347-&

[4]

Beckers J.M., 1964, THESIS UTRECHT

[5] HIGH-RESOLUTION SPECTROSCOPY OF DISK CHROMOSPHERE .1. OBSERVING PROCEDURES [J].

BECKERS, JM ;

BROWN, DR ;

MANN, GR ;

MAUTER, HA .

SOLAR PHYSICS, 1972, 25 (01) :81-&

[6]

Cram L. E., 1972, Proceedings of the Astronomical Society of Australia, V2, P146

[7] MULTI-COMPONENT MODELS FOR FORMATION OF CHROMOSPHERIC CA-II K LINE .2. EFFECT OF VELOCITY FIELDS [J].

CRAM, LE .

SOLAR PHYSICS, 1972, 22 (02) :375-&

[8] OBSERVED ODDITIES IN LINES H, K, B AND HBETA [J].

EVANS, JW ;

CATALANO, CP .

SOLAR PHYSICS, 1972, 27 (02) :299-302

[9]

HINES OC, 1960, CAN J PHYS, V38, P1441

[10]

Landau L.D., 2013, COURSE THE ORETICAL

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