Analysis of the possibilities to determine lunar soil characteristics with the help of bistatic radar


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

An opportunity of determining the lunar soil characteristics via bistatic radar involving high-power ground-based transmitters operating in meter and decameter wave ranges and receivers located aboard Moon satellite is analyzed. Direct and inverse problems concerning stratified soil sounding to a large depth, as well as algorithms for determining the regolith layer thickness, permittivity, radio wave absorption, and regolith and bedrock densities, are examined.

作者简介

O. Yushkova

Kotel’nikov Institute of Radio Engineering and Electronics (Fryazino Branch)

编辑信件的主要联系方式.
Email: o.v.y@mail.ru
俄罗斯联邦, Fryazino, Moscow oblast, 141190

O. Yakovlev

Kotel’nikov Institute of Radio Engineering and Electronics (Fryazino Branch)

Email: o.v.y@mail.ru
俄罗斯联邦, Fryazino, Moscow oblast, 141190

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Inc., 2017