Radar: The Cassini Titan RADAR Mapper

被引：160

作者：

Elachi, C

Allison, MD

Borgarelli, L

Encrenaz, P

Im, E

Janssen, MA

Johnson, WTK

Kirk, RL

Lorenz, RD

Lunine, JI

Muhleman, DO

Ostro, SJ

Picardi, G

Posa, F

Rapley, CG

Roth, LE

Seu, R

Soderblom, LA

Vetrella, S

Wall, SD

Wood, CA

Zebker, HA

机构：

[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[2] NASA, Goddard Inst Space Studies, New York, NY 10025 USA

[3] Alenia Aerosp, I-00131 Rome, Italy

[4] Observ Paris, F-92195 Meudon, France

[5] US Geol Survey, Flagstaff, AZ 86001 USA

[6] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA

[7] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA

[8] Univ Roma La Sapienza, I-00184 Rome, Italy

[9] Politecn Bari, Dip Interateneo Fis, I-70126 Bari, Italy

[10] British Antarctic Survey, Cambridge CB3 0ET, England

[11] Fac Ingn, I-80125 Naples, Italy

[12] Univ N Dakota, Grand Forks, ND 58202 USA

[13] Stanford Univ, Stanford, CA 94305 USA

来源：

SPACE SCIENCE REVIEWS | 2004年 / 115卷 / 1-4期

关键词：

D O I：

10.1007/s11214-004-1438-9

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Cassini RADAR instrument is a multimode 13.8 GHz multiple-beam sensor that can operate as a synthetic-aperture radar (SAR) imager, altimeter, scatterometer, and radiometer. The principal objective of the RADAR is to map the surface of Titan. This will be done in the imaging, scatterometer, and radiometer modes. The RADAR altimeter data will provide information on relative elevations in selected areas. Surfaces of the Saturn's icy satellites will be explored utilizing the RADAR radiometer and scatterometer modes. Saturn's atmosphere and rings will be probed in the radiometer mode only. The instrument is a joint development by JPL/NASA and ASI. The RADAR design features significant autonomy and data compression capabilities. It is expected that the instrument will detect surfaces with backscatter coefficient as low as -40 dB.

引用

页码：71 / 110

页数：40

共 54 条

[1] A WAVE DYNAMIC INTERPRETATION OF SATURNS POLAR HEXAGON [J].