CORRELATION OF SIMULTANEOUS ULTRAVIOLET (0.36 MU-M) AND INFRARED (8-MU-M TO 14-MU-M) IMAGES OF VENUS

被引：4

作者：

DINER, DJ ^{[1
]}

WESTPHAL, JA ^{[1
]}

机构：

[1] CALTECH,DIV GEOL & PLANETARY SCI,PASADENA,CA 91125

来源：

ICARUS | 1979年 / 38卷 / 01期

基金：

美国国家航空航天局;

关键词：

D O I：

10.1016/0019-1035(79)90087-3

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present evidence for a correlation between features observed in simultaneous infrared (8 to 14 μm) and ultraviolet (0.36 μm) images obtained during Venus' 1975 and 1977 apparitions. The sense of the observed correlation is such that bright uv markings correspond to bright (warm) ir features, and similarly, dark uv markings correspond to dark (cool) ir features. © 1979.

引用

页码：81 / 89

页数：9

共 13 条

[1]

COFFEEN DL, 1974, PLANETS STARS NEBULA

[2]

FOUNTAIN JW, 1974, PLANETS STARS NEBULA

[3]

HAPKE B, 1974, ATMOSPHERE VENUS, P69

[4]

Ksanfomaliti L. V., 1976, Cosmic Research, V14, P670

[5]

Ksanfomaliti L. V., 1976, Soviet Astronomy, V20, P476

[6]

KSANFOMALITY LV, 1976, 226 SPAC RES I AC SC

[7]

MURRAY B, 1963, J GEOPHYS RES, V58, P4813

[8] Photographs of Venus [J].

Ross, FE .

ASTROPHYSICAL JOURNAL, 1928, 68 (01) :57-92

[9]

TRAVIS LD, 1975, J ATMOS SCI, V32, P1190, DOI 10.1175/1520-0469(1975)032<1190:OTOOUC>2.0.CO

[10]

← 1 2 →