3D Study of Solar Eruptions Using SDO and STEREO Observations

Details 3D Study of Solar Eruptions Using SDO and STEREO Observations 3D Study of Solar Eruptions Using SDO and STEREO Observations

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh23a1834d&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH23A-1834

Astronomy and Astrophysics

Astrophysics

[7509] Solar Physics, Astrophysics, And Astronomy / Corona

Scientific paper

Combination of data from the recently launched SDO and the two STEREO spacecraft -that are now at about 80deg from the Sun-Earth direction- offers the unprecedented opportunity to observe simultaneously the region where a CME originates and the CME moving outward in the plane-of-the-sky. This allows us to compute trajectories for the CME and the associated eruptive prominence and, at the same time, to study the on-disk CME manifestations such as flares, dimming regions, and coronal waves with very high spatial and temporal resolution. We present examples of Earth-directed CMEs, when the CME can be traced from the Sun to the Earth, that take advantage of this unique satellite configuration.

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