WAVELENGTH DEPENDENCE OF SEEING

被引：41

作者：

BOYD, RW ^{[1
]}

机构：

[1] UNIV CALIF BERKELEY, DEPT PHYS, BERKELEY, CA 94720 USA

来源：

JOURNAL OF THE OPTICAL SOCIETY OF AMERICA | 1978年 / 68卷 / 07期

关键词：

ATMOSPHERIC TURBULENCE;

D O I：

10.1364/JOSA.68.000877

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The deleterious effects of atmospheric inhomogeneities on telescope angular resolution (seeing effects) were studied at a wavelength of 10 mu m with an imaging upconverter. Seeing was found to be systematically better by a factor of 1. 9 at 10 mu m than in the visible, in good agreement with theoretical predictions. A discussion of the theory of astronomical seeing is included.

引用

页码：877 / 883

页数：7

共 28 条

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BOYD, RW
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COULMAN, CE
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FITZMAURICE, MW
BUFTON, JL
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[J]. JOURNAL OF THE OPTICAL SOCIETY OF AMERICA, 1969, 59 (01) : 7 - +
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FRIED, DL
[J]. JOURNAL OF THE OPTICAL SOCIETY OF AMERICA, 1967, 57 (02) : 268 - &
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FRIED, DL
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