RADIAL BRIGHTNESS DISTRIBUTION OF SUN AT 3.2 MM AS DETERMINED FROM JUNE 30, 1973 TOTAL SOLAR ECLIPSE AND A REANALYSIS OF MARCH 7, 1970 TOTAL SOLAR ECLIPSE

被引：5

作者：

SWANSON, PN ^{[1
]}

HAGEN, JP ^{[1
]}

机构：

[1] PENN STATE UNIV,RADIO ASTRON OBSERV,UNIVERSITY PK,PA 16802

来源：

SOLAR PHYSICS | 1975年 / 43卷 / 01期

关键词：

D O I：

10.1007/BF00155142

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：57 / 62

页数：6

共 8 条

[1] OBSERVATIONS OF 7 MARCH, 1970 TOTAL SOLAR ECLIPSE AT WAVELENGTHS OF 3.2 AND 8.3 MM [J].

HAGEN, JP ;

HAAS, RW ;

WEFER, FL ;

VOGT, RW ;

SWANSON, PN .

SOLAR PHYSICS, 1971, 21 (02) :286-+

[2] METHOD FOR DERIVING RADIAL BRIGHTNESS DISTRIBUTIONS FROM ECLIPSE OBSERVATIONS [J].

HAGEN, JP ;

SWANSON, PN .

ASTROPHYSICAL JOURNAL, 1975, 198 (01) :219-222

[3]

SHIMABUKURO FI, 1974, COMMUNICATION

[4] HIGH-RESOLUTION OBSERVATIONS OF CHROMOSPHERE AT MM AND CM WAVELENGTHS [J].

SIMON, M .

SOLAR PHYSICS, 1971, 21 (02) :297-&

[5]

SIMON M, 1971, COMMUNICATION

[6]

SWANSON PN, 1971, 022 PENNS STAT U DEP

[7] NO EVIDENCE OF ANY SOLAR LIMB BRIGHTENING IN RANGE OF 3.5-MM-2-CM [J].

TLAMICHA, A .

SOLAR PHYSICS, 1969, 10 (01) :150-&

[8] SOLAR RADIATION AT 3.2 MM DURING JULY 20 1963 ECLIPSE [J].

TOLBERT, CW ;

KRAUSE, LC ;

STRAITON, AW .

ASTROPHYSICAL JOURNAL, 1964, 140 (01) :306-&

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