Simultaneous measurements of Martian plasma boundaries by Rosetta and Mars Express

被引:14
作者
Edberg, N. J. T. [1 ,2 ]
Eriksson, A. I. [2 ]
Auster, U. [3 ]
Barabash, S. [6 ]
Boesswetter, A. [4 ]
Carr, C. M. [7 ]
Cowley, S. W. H. [1 ]
Cupido, E. [7 ]
Fraenz, M. [5 ]
Glassmeier, K. -H. [3 ]
Goldstein, R. [8 ]
Lester, M. [1 ]
Lundin, R. [6 ]
Modolo, R. [2 ]
Nilsson, H. [6 ]
Richter, I. [3 ]
Samara, M. [8 ]
Trotignon, J. G. [9 ]
机构
[1] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[2] Swedish Inst Space Phys, S-75121 Uppsala, Sweden
[3] TU Braunschweig, Inst Geophys & Extraterrestrial Phys, Braunschweig, Germany
[4] TU Braunschweig, Inst Theoret Phys, Braunschweig, Germany
[5] Max Planck Inst Solar Syst Res, Katlenburg Lindau, Germany
[6] Swedish Inst Space Phys, S-98128 Kiruna, Sweden
[7] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London, England
[8] SW Res Inst, San Antonio, TX USA
[9] Lab Phys & Chim Environm, Orleans, France
关键词
Mars; Plasma; Rosetta; Mars Express; Bow shock; Magnetic pileup boundary; SOLAR-WIND INTERACTION; BOW SHOCK POSITION; PILE-UP BOUNDARY; GLOBAL-SURVEYOR; MAGNETIC-FIELD; POTENTIAL MEASUREMENTS; TERRESTRIAL PLANETS; RPC; MAGNETOSPHERE; CONSORTIUM;
D O I
10.1016/j.pss.2008.10.016
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the first two-spacecraft near-simultaneous observations of the Martian bow shock (BS), magnetic pileup boundary (MPB) and photo-electron boundary (PEB) obtained by the plasma instruments onboard Rosetta and Mars Express during the Rosetta Mars fly by on February 25, 2007. Our observations are compared with shape models for the BS and MPB derived from previous statistical studies. The MPB is found at its expected position but the BS for this event is found significantly closer to the planet than expected for the rather slow and moderately dense solar wind. Cross-calibration of the density measurements on the two spacecraft gives a density profile through the magnetosheath, indicating an increasing solar wind flux during the Rosetta passage which is consistent with the multiple BS crossings at the Rosetta exit. (C) 2008 Elsevier Ltd. All rights reserved.
引用
收藏
页码:1085 / 1096
页数:12
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