SOLAR CHROMOSPHERIC MODELING BASED ON SUBMILLIMETER LIMB BRIGHTNESS PROFILE

被引：9

作者：

HERMANS, LM

LINDSEY, C

机构：

来源：

ASTROPHYSICAL JOURNAL | 1986年 / 310卷 / 02期

关键词：

D O I：

10.1086/164742

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：907 / 911

页数：5

共 7 条

[1]

AUER LH, 1972, 555 KITT PEAK NAT OB

[2]

AVRETT EH, 1985, COMMUNICATION

[3]

Carbon D. F., 1969, Theory and observation of normal stellar atmospheres, proceedings of 3rd Harvard-Smithsonian conference on stellar atmospheres, P377

[4]

HERMANS LM, 1984, THESIS U HAWAII

[5] EXTREME LIMB PROFILES OF THE SUN AT FAR-INFRARED AND SUBMILLIMETER WAVELENGTHS [J].

LINDSEY, C ;

BECKLIN, EE ;

ORRALL, FQ ;

WERNER, MW ;

JEFFERIES, JT ;

GATLEY, I .

ASTROPHYSICAL JOURNAL, 1986, 308 (01) :448-458

[6] STRUCTURE OF THE SOLAR CHROMOSPHERE .3. MODELS OF THE EUV BRIGHTNESS COMPONENTS OF THE QUIET SUN [J].

VERNAZZA, JE ;

AVRETT, EH ;

LOESER, R .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1981, 45 (04) :635-+

[7]

VERNAZZA JE, 1973, AP J, V184, P604

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