First 4D Reconstruction of an Eruptive Prominence Using Three Simultaneous View Directions

作者：Chifu I^*; Inhester B; Mierla M; Chifu V; Wiegelmann T

来源：Solar Physics, 2012, 281(1): 121-135.

DOI：10.1007/s11207-012-0107-5

• Prominences
• 3D reconstruction
• Stereoscopy
• Corona

Data from the STEREO (Solar Terrestrial Relations Observatory) mission are intensively used for 3D reconstruction of solar coronal structures. After the launch of the SDO (Solar Dynamic Observatory) satellite, its additional observations give the possibility to have a third eye for more accurate 3D reconstruction in the very low corona (< 1.5 R (aS (TM))). With our reconstruction code MBSR (Multi-view B-spline Stereoscopic Reconstruction), we use three view directions (STEREO A, B, and SDO) to perform the 3D reconstruction and evolution of a prominence which triggered a CME on 1 August 2010. In the paper we present the reconstruction of this prominence from the moment it starts to erupt until it leaves the field of view of the coronagraph. We also determine the evolution of the leading edge of the CME. Based on the temporal evolution, we analyze some of its properties, such as velocity, acceleration, opening and rotation angles and evolution of the cavity.

• 出版日期2012-11