Rosetta Orbiter Spectrometer for ion and neutral analysis-ROSINA

被引：24

作者：

Balsiger, H ^{[1
]}

Altwegg, K

Arijs, E

Bertaux, JL

Berthelier, JJ

Bochsler, P

Carignan, GR

Eberhardt, P

Fisk, LA

Fuselier, SA

Ghielmetti, AG

Gliem, F

Gombosi, TI

Kopp, E

Korth, A

Livi, S

Mazelle, C

Reme, H

Sauvaud, JA

Shelley, EG

Waite, JH

Wilken, B

Woch, J

Wollnik, H

Wurz, P

Young, DT

机构：

[1] Univ Bern, Inst Phys, CH-3012 Bern, Switzerland

[2] Ctr Etud Spatiale Rayonnements, F-31029 Toulouse, France

[3] IPSL, F-94100 St Maur, France

[4] MPI Aeron, D-37191 Katlenburg Lindau, Germany

[5] Univ Giessen, Inst Phys, D-35392 Giessen, Germany

[6] Tech Univ Braunschweig, D-38106 Braunschweig, Germany

[7] Lockheed Palo Alto Res Labs, Palo Alto, CA 94394 USA

[8] SW Res Inst, San Antonio, TX 78228 USA

[9] Univ Michigan, Space Phys Res Lab, Ann Arbor, MI 48109 USA

[10] BIRA, B-1180 Brussels, Belgium

来源：

SPACE EXPLORATION OF THE OUTER SPACE SOLAR SYSTEM AND COMETARY NUCLEI | 1998年 / 21卷 / 11期

关键词：

D O I：

10.1016/S0273-1177(97)00945-9

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) will answer outstanding questions concerning the main objectives of the mission. To accomplish the very demanding objectives, ROSINA will have unprecedented capabilities, including: very wide mass range from 1 amu to >300 amu; very high mass resolution (ability to resolve CO from N-2 and C-13 from (CH)-C-12); very wide dynamic range and high sensitivity; the ability to determine cometary gas and ion flow velocities and temperatures. (C) 1998 COSPAR. Published by Elsevier Science Ltd.

引用

页码：1527 / 1535

页数：9