SOURCE FUNCTIONS OF INFRARED FRAUNHOFER LINES FROM EQUIVALENT WIDTHS

被引：6

作者：

ALTROCK, RC

机构：

[1] Sacramento Peak Observatory, Air Force Cambridge Research Laboratories, Sunspot, N.M.

来源：

SOLAR PHYSICS | 1969年 / 7卷 / 01期

关键词：

D O I：

10.1007/BF00148397

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A method for obtaining the source function and value of r0 □ kc/kL,0 from the variation of equivalent width across the solar disk has been applied to several infrared Fraunhofer lines. The results indicate that most of the lines investigated have non-L.T.E. source functions which are less than or equal to the mean continuum intensity. De Jager and Neven (1968) appear to have underestimated the departures from L.T.E. in a number of cases. © 1969 D. Reidel Publishing Company.

引用

页码：3 / &

共 9 条

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[2]

Altrock R. C., 1968, Solar Physics, V5, P260, DOI 10.1007/BF00147140

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SKUMANIC.A .

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[4]

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[5]

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[6]

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[7]

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[8]

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[9]

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