INVERTING THE ZODIACAL LIGHT BRIGHTNESS INTEGRAL

被引：12

作者：

SCHUERMAN, DW

机构：

[1] Space Astronomy Laboratory, State University of New York at Albany, Albany

来源：

PLANETARY AND SPACE SCIENCE | 1979年 / 27卷 / 04期

关键词：

D O I：

10.1016/0032-0633(79)90132-6

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Considerations of the geometry appropriate to observations of the zodiacal light made from out of the ecliptic plane yield the general inversion of the brightness integral. The brightness per unit volume of interplanetary space can thus be determined in the immediate neighborhood of the spacecraft in directions confined to a unique viewing plane which depends upon the spacecraft's trajectory. The implementation of this technique guarantees the maximum information content of optical observations made from future deep-space probes including the Out-of-Ecliptic" mission scheduled for launch in 1983. © 1979."

引用

页码：551 / 556

页数：6