MARS RADAR MAPPING - STRONG BACKSCATTER FROM THE ELYSIUM BASIN AND OUTFLOW CHANNEL

被引：25

作者：

HARMON, JK ^{[1
]}

SULZER, MP ^{[1
]}

PERILLAT, PJ ^{[1
]}

CHANDLER, JF ^{[1
]}

机构：

[1] HARVARD SMITHSONIAN CTR ASTROPHYS,CAMBRIDGE,MA 02138

来源：

ICARUS | 1992年 / 95卷 / 01期

关键词：

D O I：

10.1016/0019-1035(92)90197-F

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Radar reflectivity maps of Mars, obtained at Arecibo in 1990 using a modified delay-Doppler technique, have revealed strong depolarized echoes coming from the Elysium flood basin and outflow channel as well as from Elysium Mons. This result is consistent with recent studies which show that much of the basin/channel floor is covered with lava flows. © 1992.

引用

页码：153 / 156

页数：4

共 16 条

[1]

Carr M., 1981, SURFACE MARS

[2] MARTIAN CHANNELS AND VALLEYS - THEIR CHARACTERISTICS, DISTRIBUTION, AND AGE [J].