Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1768591 | Advances in Space Research | 2008 | 7 Pages |
Abstract
The scientific objectives of the mission are shortly presented. We describe the three instrumental packages and the profile of the mission which accommodates them. With a launch around 2012-2013, the SMESE microsatellite mission will provide a unique tool for detecting and understanding eruptions (flares and coronal mass ejections). Observations should start around solar maximum, and continue in the declining phase of activity, at a time when the Solar Dynamics Observatory (SDO) should still be operating.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
J.-C. Vial, F. Auchère, J. Chang, C. Fang, W.Q. Gan, K.-L. Klein, J.-Y. Prado, F. Rouesnel, A. Sémery, G. Trottet, C. Wang,