Open Access. Powered by Scholars. Published by Universities.®
Articles 1 - 1 of 1
Full-Text Articles in Entire DC Network
Theoretical Modeling For The Stereo Mission, Marcus J. Aschwanden, L. F. Burlaga, M. L. Kaiser, C. K. Ng, D. V. Reames, M. J. Reiner, Tamas I. Gombosi, Noe Lugaz, Ward B. Manchester Iv, Ilia I. Roussev, Thomas H. Zurbuchen, Charlie J. Farrugia, Antoinette B. Galvin, M. A. Lee, J. A. Linker, Z. Mikic, Pete Riley, D. Alexander, A. W. Sandman, J. W. Cook, R. A. Howard, D. Odstrcil, V. J. Pizzo, J. Kota, Et Al.
Theoretical Modeling For The Stereo Mission, Marcus J. Aschwanden, L. F. Burlaga, M. L. Kaiser, C. K. Ng, D. V. Reames, M. J. Reiner, Tamas I. Gombosi, Noe Lugaz, Ward B. Manchester Iv, Ilia I. Roussev, Thomas H. Zurbuchen, Charlie J. Farrugia, Antoinette B. Galvin, M. A. Lee, J. A. Linker, Z. Mikic, Pete Riley, D. Alexander, A. W. Sandman, J. W. Cook, R. A. Howard, D. Odstrcil, V. J. Pizzo, J. Kota, Et Al.
Coronal Mass Ejection Research Group
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 …