Theoretical modeling for the stereo mission

Details Theoretical modeling for the stereo mission Theoretical modeling for the stereo mission

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ssrv..136..565a&link_type=abstract

Space Science Reviews, Volume 136, Issue 1-4, pp. 565-604

Computer Science

26

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

Scientific paper

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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