Three-dimensional Reconstruction of Coronal Mass Ejections Using Stereo Polarimetric Observations

Details Three-dimensional Reconstruction of Coronal Mass Ejections Using Stereo Polarimetric Observations Three-dimensional Reconstruction of Coronal Mass Ejections Using Stereo Polarimetric Observations

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.2115m&link_type=abstract

American Astronomical Society, SPD meeting #40, #21.15; Bulletin of the American Astronomical Society, Vol. 41, p.857

Astronomy and Astrophysics

Astronomy

Scientific paper

We present reconstructions of coronal mass ejections (CMEs) on 21August2007 and 31December2007 from STEREO/SECCHI polarimetric observations. Polarimetry of CME scattered white light provides three-dimensional CME structural information. We combine measurements from the STEREO A and B spacecraft spacecraft to determine the three-dimensional orientations of the eruptions using both parallax and polarimetric techniques, and find agreement within uncertainties. In addition, we determine the gross 3D density distribution and direction of
several CMEs.

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