THEORETICAL CHROMOSPHERIC FLARE SPECTRA .2. HYDROGEN EQUILIBRIUM FOR BROWNS (1973) MODELS FOR HEATING BY NONTHERMAL ELECTRONS

被引：35

作者：

CANFIELD, RC ^{[1
]}

机构：

[1] SACRAMENTO PEAK OBSERV,SUNSPOT,NM 88349

来源：

SOLAR PHYSICS | 1974年 / 34卷 / 02期

关键词：

D O I：

10.1007/BF00153672

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：339 / 348

页数：10

共 10 条

[1]

BROWN JC, 1973, SOL PHYS, V31, P143, DOI 10.1007/BF00156080

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SOLAR PHYSICS, 1974, 34 (01) :193-206

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SOLAR PHYSICS, 1971, 18 (03) :347-+

[5]

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[6] KINEMATIC MODEL OF A SOLAR-FLARE [J].

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WU, ST ;

HAN, SM .

SOLAR PHYSICS, 1973, 30 (01) :111-120

[7]

POTTASCH SR, 1965, B ASTRON I NETH, V18, P7

[8] DEPARTURES FROM THE SAHA EQUATION UNDER VARYING CONDITIONS OF LYMAN CONTINUOUS OPACITY [J].

POTTASCH, SR ;

THOMAS, RN .

ASTROPHYSICAL JOURNAL, 1959, 130 (03) :941-953

[9] SPECTRA OF SOLAR-FLARES [J].

SVESTKA, Z .

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1972, 10 :1-+

[10]

WHITE OR, 1962, ASTROPHYS J SUPPL, V70, P333

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