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Theoretical modeling for the stereo mission |
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| Authors: | Markus J Aschwanden L F Burlaga M L Kaiser C K Ng D V Reames M J Reiner T I Gombosi N Lugaz W Manchester IV I I Roussev T H Zurbuchen C J Farrugia A B Galvin M A Lee J A Linker Z Miki? P Riley D Alexander A W Sandman J W Cook R A Howard D Odstr?il V J Pizzo J Kóta P C Liewer J G Luhmann B Inhester R W Schwenn S K Solanki V M Vasyliunas T Wiegelmann L Blush P Bochsler I H Cairns P A Robinson V Bothmer K Kecskemety A Llebaria M Maksimovic M Scholer R F Wimmer-Schweingruber |
| Institution: | 1. Solar & Astrophysics Lab., Lockheed Martin ATC, 3251 Hanover St., Palo Alto, CA, 94304, USA 2. NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, USA 3. University of Michigan, 1141 Space Research Bldg., Ann Arbor, MI, 48109, USA 4. University of New Hampshire, EOS SSC Morse Hall, Durham, NH, 03824, USA 5. SAIC, 10260 Campus Point Dr., San Diego, CA, 92121, USA 6. Dept. Physics & Astronomy, Rice University, PO Box 1892, Houston, TX, 77251, USA 7. Naval Research Laboratory, Code 7660, 4555 Overlook Ave. SW, Washington DC, 20375, USA 8. NOAA/SEC, Code R/E/SE, 325 Broadway, Boulder, CO, 80303, USA 9. University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, 85721-0092, USA 10. Jet Propulsion Laboratory, Mail Stop 169-506, Pasadena, CA, 91109, USA 11. University of Berkeley, Space Sciences Lab., 7 Gauss Way #7450, Berkeley, CA, 94720, USA 12. Max-Planck Institut für Sonnensystemforschung, Max-Planck Str.2, D-37191, Katlenburg-Lindau, Germany 13. Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012, Bern, Switzerland 14. School of Physics, University of Sydney, Sydney, NSW, 2006, Australia 15. Institut für Astrophysik, Universit?t G?ttingen, Friedrich-Hund-Platz 1, 37077, G?ttingen, Germany 16. KFKI RMKI, POB 49, H-1525, Budapest, Hungary 17. Laboratoire d’Astronomie Spatiale, C.N.R.S., BP8, 13376 12, Marseille Cedex, France 18. CNRS & LESIA, Observatore de Paris-Meudon, F-92195, Meudon Cedex, France 19. Center for Interdisciplinary Plasma Science, Max-Planck-Institute for Extraterrestrial Physics, 85740, Garching, Munich, Germany 20. Extraterr, Physics IEAP, University of Kiel, Leibnizstr. 11, Kiel, 24118, Germany |
| Abstract: | 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. |
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