RADIATIVE SIGNATURES FROM IMPACT OF COMET SHOEMAKER-LEVY-9 ON JUPITER

被引：14

作者：

AHRENS, TJ ^{[1
]}

TAKATA, T ^{[1
]}

OKEEFE, JD ^{[1
]}

ORTON, GS ^{[1
]}

机构：

[1] JET PROP LAB,PASADENA,CA 91109

来源：

GEOPHYSICAL RESEARCH LETTERS | 1994年 / 21卷 / 14期

关键词：

D O I：

10.1029/94GL01578

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

The visible optical power emitted from the expansion plumes from 0.4 and 2 km diameter fragments of Shoemaker-Levy are expected to be, approximately 25% and comparable to, the visible solar flux reflected from Jupiter, respectively, for several minutes, and could be easily observed by sensors on the Galileo spacecraft. Earth-based observers can detect these plumes as these expand over the SW limb of Jupiter and come into earth view some n-minutes after impact!

引用

页码：1551 / 1553

页数：3

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