USING ECLIPSE OBSERVATIONS TO TEST SCINTILLATION MODELS

被引：5

作者：

GEORGOBIANI, D ^{[1
]}

KUHN, JR ^{[1
]}

BECKERS, JM ^{[1
]}

机构：

[1] ASSOC UNIV RES ASTRON INC,NATL SOLAR OBSERV,SUNSPOT,NM 88349

来源：

SOLAR PHYSICS | 1995年 / 156卷 / 01期

关键词：

D O I：

10.1007/BF00669570

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Near second and third contact during a solar eclipse the spatial spectrum of the solar illumination changes as the relative power at high spatial frequencies increases strongly. Since groundlevel atmospheric scintillation depends on a weighted integral of the image power spectrum, we can expect to see a measurable time dependence to solar scintillation during an eclipse. This effect was observed during an annular solar eclipse and quantitatively compared with a scintillation model.

引用

页码：1 / 5

页数：5

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