The Venusian induced magnetosphere:: A case study of plasma and magnetic field measurements on the Venus Express mission

被引：26

作者：

Kallio, E. ^{[1
]}

Zhang, T. L. ^{[2
]}

Barabash, S. ^{[3
]}

Jarvinen, R. ^{[1
]}

Sillanpaa, I. ^{[1
]}

Janhunen, P. ^{[1
]}

Fedorov, A. ^{[4
]}

Sauvaud, J. -A. ^{[4
]}

Mazelle, C. ^{[4
]}

Thocaven, J. -J. ^{[4
]}

Gunell, H. ^{[20
]}

Andersson, H. ^{[3
]}

Grigoriev, A. ^{[3
]}

Brinkfeldt, K. ^{[3
]}

Futaana, Y. ^{[3
]}

Holmstrom, M. ^{[3
]}

Lundin, R. ^{[3
]}

Yamauchi, M. ^{[3
]}

Asamura, K. ^{[5
]}

Baumjohann, W. ^{[2
]}

Lammer, H. ^{[2
]}

Coates, A. J. ^{[6
]}

Linder, D. R. ^{[6
]}

Kataria, D. O. ^{[6
]}

Curtis, C. C. ^{[7
]}

Hsieh, K. C. ^{[7
]}

Sandel, B. R. ^{[7
]}

Grande, M. ^{[8
]}

Koskinen, H. E. J. ^{[1
,9
]}

Sales, T. ^{[1
]}

Schmidt, W. ^{[1
]}

Riihela, P. ^{[1
]}

Kozyra, J. ^{[10
]}

Krupp, N. ^{[11
]}

Woch, J. ^{[11
]}

Luhmann, J. G. ^{[12
]}

McKenna-Lawlor, S. ^{[13
]}

Orsini, S. ^{[14
]}

Cerulli-Irelli, R. ^{[14
]}

Mura, A. ^{[14
]}

Milillo, A. ^{[14
]}

Maggi, M. ^{[14
]}

Roelof, E. ^{[15
]}

Brandt, P. ^{[15
]}

Russell, C. T. ^{[16
]}

Szego, K. ^{[17
]}

Winningham, J. D. ^{[18
]}

Frahm, R. A. ^{[18
]}

Scherrer, J. R. ^{[18
]}

Sharber, J. R. ^{[18
]}

机构：

[1] Finnish Meteorol Inst, FIN-00101 Helsinki, Finland

[2] Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria

[3] Swedish Inst Space Phys, SE-98128 Kiruna, Sweden

[4] Ctr Etud Spatiale Rayonnements, F-31028 Toulouse, France

[5] Inst Space & Astronaut Sci, Sagamihara, Kanagawa, Japan

[6] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England

[7] Univ Arizona, Tucson, AZ 85721 USA

[8] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England

[9] Univ Helsinki, Dept Phys Sci, FIN-00014 Helsinki, Finland

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

[11] Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany

[12] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA

[13] Natl Univ Ireland, Space Technol Ireland, Maynooth, Kildare, Ireland

[14] Inst Fis Spazio Interplanetari, I-00133 Rome, Italy

[15] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA

[16] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA

[17] KFKI Res Inst Particle & Nucl Phys, H-1525 Budapest, Hungary

[18] SW Res Inst, San Antonio, TX USA

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

[20] W Virginia Univ, Dept Phys, Morgantown, WV 26506 USA

来源：

PLANETARY AND SPACE SCIENCE | 2008年 / 56卷 / 06期

基金：

英国科学技术设施理事会;

关键词：

Venus; Venus-solar wind interaction; planetary magnetospheres; solar wind; numerical modelling;

D O I：

10.1016/j.pss.2007.09.011

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Plasma and magnetic field measurements made onboard the Venus Express on June 1, 2006, are analyzed and compared with predictions of a global model. It is shown that in the orbit studied, the plasma and magnetic field observations obtained near the North Pole under solar minimum conditions were qualitatively and, in many cases also, quantitatively in agreement with the general picture obtained using a global numerical quasi-neutral hybrid model of the solar wind interaction (HYB-Venus). In instances where the orbit of Venus Express crossed a boundary referred to as the magnetic pileup boundary (MPB), field line tracing supports the suggestion that the MPB separates the region that is magnetically connected to the fluctuating magnetosheath field from a region that is magnetically connected to the induced magnetotail lobes. (c) 2007 Elsevier Ltd. All rights reserved.

引用

页码：796 / 801

页数：6

共 6 条

[1] The analyser of space plasmas and energetic atoms (ASPERA-4) for the Venus express mission [J].

Barabash, S. ;

Sauvaud, J.-A. ;

Gunell, H. ;

Andersson, H. ;

Grigoriev, A. ;

Brinkfeldt, K. ;

Holinstroem, M. ;

Lundin, R. ;

Yamauchi, M. ;

Asamura, K. ;

Baumjohann, W. ;

Zhang, T. L. ;

Coates, A. J. ;

Linder, D. R. ;

Kataria, D. O. ;

Curtis, C. C. ;

Hsieh, K. C. ;

Sandel, B. R. ;

Fedorov, A. ;

Mazelle, C. ;

Thocaven, J. J. ;

Grande, M. ;

Koskinen, Hannu E. J. ;

Kallio, E. ;

Saeles, T. ;

Riihela, P. ;

Kozyra, J. ;

Krupp, N. ;

Woch, J. ;

Luhmann, J. ;

McKenna-Lawlor, S. ;

Orsini, S. ;

Cerulli-Irelli, R. ;

Mura, M. ;

Milillo, M. ;

Maggi, M. ;

Roelof, E. ;

Brandt, P. ;

Russell, C. T. ;

Szego, K. ;

Winningham, J. D. ;

Frahm, R. A. ;

Scherrer, J. ;

Sharber, J. R. ;

Wurz, P. ;

Bochsler, P. .

PLANETARY AND SPACE SCIENCE, 2007, 55 (12) :1772-1792

[2]

BERTUCCI C, 2005, J GEOPHYS RES, P110

[3] Venus-solar wind interaction:: Asymmetries and the escape of O+ ions [J].

Kallio, E. ;

Jarvinen, R. ;

Janhunen, P. .

PLANETARY AND SPACE SCIENCE, 2006, 54 (13-14) :1472-1481

[4] MAGNETIC-FIELD FLUCTUATIONS IN THE VENUS MAGNETOSHEATH [J].

LUHMANN, JG ;

TATRALLYAY, M ;

RUSSELL, CT ;

WINTERHALTER, D .

GEOPHYSICAL RESEARCH LETTERS, 1983, 10 (08) :655-658

[5] AVERAGE DIMENSION AND MAGNETIC-STRUCTURE OF THE DISTANT VENUS MAGNETOTAIL [J].

SAUNDERS, MA ;

RUSSELL, CT .

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1986, 91 (A5) :5589-5604

[6] Distribution of magnetic flux density in soft-contact EMCC rectangular mold [J].

Zhang Lin-tao ;

Wang En-gang ;

Deng An-yuan ;

He Ji-cheng .

JOURNAL OF IRON AND STEEL RESEARCH INTERNATIONAL, 2006, 13 (05) :14-+

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