Theoretical modeling for the STEREO mission

被引：33

作者：

Aschwanden, Markus J. ^{[1
]}

Burlaga, L. F. ^{[2
]}

Kaiser, M. L. ^{[2
]}

Ng, C. K. ^{[2
]}

Reames, D. V. ^{[2
]}

Reiner, M. J. ^{[2
]}

Gombosi, T. I. ^{[3
]}

Lugaz, N. ^{[3
]}

Manchester, W., IV ^{[3
]}

Roussev, I. I. ^{[3
]}

Zurbuchen, T. H. ^{[3
]}

Farrugia, C. J. ^{[4
]}

Galvin, A. B. ^{[4
]}

Lee, M. A. ^{[4
]}

Linker, J. A. ^{[5
]}

Mikic, Z. ^{[5
]}

Riley, P. ^{[5
]}

Alexander, D. ^{[6
]}

Sandman, A. W. ^{[6
]}

Cook, J. W. ^{[7
]}

Howard, R. A. ^{[7
]}

Odstrcil, D. ^{[8
]}

Pizzo, V. J. ^{[8
]}

Kota, J. ^{[9
]}

Liewer, P. C. ^{[10
]}

Luhmann, J. G. ^{[11
]}

Inhester, B. ^{[12
]}

Schwenn, R. W. ^{[12
]}

Solanki, S. K. ^{[12
]}

Vasyliunas, V. M. ^{[12
]}

Wiegelmann, T. ^{[12
]}

Blush, L. ^{[13
]}

Bochsler, P. ^{[13
]}

Cairns, I. H. ^{[14
]}

Robinson, P. A. ^{[14
]}

Bothmer, V. ^{[15
]}

Kecskemety, K. ^{[16
]}

Llebaria, A. ^{[17
]}

Maksimovic, M. ^{[18
,19
]}

Scholer, M. ^{[20
]}

Wimmer-Schweingruber, R. F. ^{[21
]}

机构：

[1] Lockheed Martin ATC, Solar & Astrophys Lab, Palo Alto, CA 94304 USA

[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[3] Univ Michigan, Ann Arbor, MI 48109 USA

[4] Univ New Hampshire, Durham, NH 03824 USA

[5] SAIC, San Diego, CA 92121 USA

[6] Rice Univ, Dept Phys & Astron, Houston, TX 77251 USA

[7] USN, Res Lab, Washington, DC 20375 USA

[8] NOAA, SEC, Boulder, CO 80303 USA

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

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

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

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

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

[14] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia

[15] Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany

[16] HKFI RMKI, H-1525 Budapest, Hungary

[17] CNRS, Astron Spatiale Lab, F-13376 Marseille, France

[18] Observ Paris, CNRS, F-92195 Meudon, France

[19] Observ Paris, LESIA, F-92195 Meudon, France

[20] Max Planck Inst Extraterr Phys, Ctr Interdisciplinary Plasma Sci, D-85740 Munich, Germany

[21] Univ Kiel, Phys IEAP, D-24118 Kiel, Germany

来源：

SPACE SCIENCE REVIEWS | 2008年 / 136卷 / 1-4期

基金：

英国科学技术设施理事会;

关键词：

STEREO mission; solar corona; solar wind; coronal mass ejection (CME); solar filaments; heliosphere; interplanetary shocks; interplanetary particle beams; solar energetic particle events (SEP); solar flares; space weather; stereoscopy; 3D reconstruction techniques; white-light emission; EUV emission; interplanetary radio emission;

D O I：

10.1007/s11214-006-9027-8

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We summarize the theory and modeling efforts for the STEREO mission, which will be used to interpret the data of both the remote-sensing (SECCHI, SWAVES) and in-situ instruments (IMPACT, PLASTIC). The modeling includes the coronal plasma, in both open and closed magnetic structures, and the solar wind and its expansion outwards from the Sun, which defines the heliosphere. Particular emphasis is given to modeling of dynamic phenomena associated with the initiation and propagation of coronal mass ejections (CMEs). The modeling of the CME initiation includes magnetic shearing, kink instability, filament eruption, and magnetic reconnection in the flaring lower corona. The modeling of CME propagation entails interplanetary shocks, interplanetary particle beams, solar energetic particles (SEPs), geoeffective connections, and space weather. This review describes mostly existing models of groups that have committed their work to the STEREO mission, but is by no means exhaustive or comprehensive regarding alternative theoretical approaches.

引用

页码：565 / 604

页数：40

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