RPC-IES: The ion and electron sensor of the Rosetta Plasma Consortium

被引:116
作者
Burch, J. L.
Goldstein, R.
Cravens, T. E.
Gibson, W. C.
Lundin, R. N.
Pollock, C. J.
Winningham, J. D.
Young, D. T.
机构
[1] SW Res Inst, San Antonio, TX 78228 USA
[2] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA
[3] Swedish Inst Space Phys, S-98128 Kiruna, Sweden
基金
美国国家航空航天局;
关键词
comet; 67P/Churyumov-Gerasimenko; solar wind-comet interaction; plasma analyzer; solar wind asteroid interaction;
D O I
10.1007/s11214-006-9002-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The ion and electron sensor (IES) is part of the Rosetta Plasma Consortium (RPC). The IES consists of two electrostatic plasma analyzers, one each for ions and electrons, which share a common entrance aperture. Each analyzer covers an energy/charge range from I eV/e to 22 keV/e with a resolution of 4%. Electrostatic deflection is used at the entrance aperture to achieve a field of view of 90 degrees x 360 degrees (2.8 pi sr). Angular resolution is 5 degrees x 22.5 degrees for electrons and 5 degrees x 45 degrees for ions, vith the sector containing the solar wind being further segmented to 5 degrees x 5 degrees. The three-dimensional plasma distributions obtained by IES will be used to investigate the interaction of the solar wind with asteroids Steins and Lutetia and the coma and nucleus of comet 67P/Churyumov-Gerasimenko (CG). In addition, photoelectron spectra obtained at these bodies will help determine their composition.
引用
收藏
页码:697 / 712
页数:16
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