First Simultaneous Views of the Axial and Lateral Perspectives of a Coronal Mass Ejection

I. CABELLO; H. CREMADES; L. BALMACEDA; I. DOHMEN

SOLAR PHYSICS

SPRINGER

Lugar: Berlin; Año: 2016

0038-0938

The different appearances exhibited by Coronal Mass Ejections (CMEs) are believed to be, in part, the result of different orientations of their main axis of symmetry, consistent with a flux-rope configuration. There are observational reports of CMEs seen along their main axis (axial perspective) and perpendicular to it (lateral perspective), however no simultaneous observations of both perspectives from the same CME have been reported to date. The stereoscopic views of the telescopes aboard the Solar-Terrestrial Relations Observatory (STEREO) twin spacecraft, in combination with the views from the Solar and Heliospheric Observatory (SOHO) and the Solar Dynamics Observatory (SDO), allow us to study the axial and lateral perspectives of a CME simultaneously for the first time. In addition, this study shows that the lateral angular extent (L) increaseslinearly with time, while the angular extent of the axial perspective (D) presents this behavior only from the low corona to ≈ 5 R , where it slows down. The ratio L/D ≈ 1.6 obtained here as the average over several points in time is consistent with measurements of L and D previously performed on events exhibiting only one of the perspectives from the single vantage point provided by SOHO.