Determination of Geometric and Kinematical Parameters of Coronal Mass Ejections Using STEREO Data

Details Determination of Geometric and Kinematical Parameters of Coronal Mass Ejections Using STEREO Data Determination of Geometric and Kinematical Parameters of Coronal Mass Ejections Using STEREO Data

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..416f&link_type=abstract

TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 416-419 (2010).

Astronomy and Astrophysics

Astronomy

Solar Corona, Astronomical Observations, Spacecraft, Curvature Measurement, Corona, Ultraviolet, Spacecraft/Atmosphere Interactions, Spatial Dimensions

Scientific paper

We present a new, relatively simple and fast method to determine true geometric and kinematical CME parameters from simultaneous STEREO A, B observations of CMEs. These parameters are the three-dimensional direction of CME propagation, velocity and acceleration of CME front, CME angular sizes and front position depending on time. The method is based on the assumption that CME shape may be described by a modification of so-called ice-cream cone models. The method has been tested for several CMEs.

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