TURBULENCE IN PLANETARY OCCULTATIONS - A STRONG SCATTERING FORMULATION INCLUDING AN INHOMOGENEOUS BACKGROUND

被引：6

作者：

HAUGSTAD, BS

机构：

来源：

RADIO SCIENCE | 1982年 / 17卷 / 03期

关键词：

D O I：

10.1029/RS017i003p00565

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：565 / 573

页数：9

共 17 条

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[4] EFFECTS OF INHOMOGENEOUS BACKGROUND ON RADIATION PROPAGATING THROUGH TURBULENT PLANETARY ATMOSPHERES [J].

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[5] TURBULENCE IN PLANETARY OCCULATIONS .4. POWER SPECTRA OF PHASE AND INTENSITY FLUCTUATIONS [J].

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[6] TURBULENCE IN PLANETARY OCCULTATIONS .3. EFFECTS ON ATMOSPHERIC PROFILES DERIVED FROM INTENSITY MEASUREMENTS [J].

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[7] TURBULENCE IN DEEP RADIO OCCULTATIONS [J].

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RADIO SCIENCE, 1981, 16 (06) :1473-1480

[8] STELLAR OCCULTATIONS BY TURBULENT PLANETARY ATMOSPHERES - WAVE-OPTICAL THEORY INCLUDING A FINITE SCALE HEIGHT [J].

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