Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8955780 | Journal of Atmospheric and Solar-Terrestrial Physics | 2018 | 9 Pages |
Abstract
The motions of three solar eruptive prominences are studied. The behaviour of the rising prominence body during the eruption is tracked. Height-time profiles of the eruption up to 6 Râ (based on observations by Solar Dynamics Observatory/Atmospheric Imaging Assembly (HeII 304â¯Ã
) and Large Angle and Spectrometric Coronagraph Experiment (LASCO) C2/Solar and Heliospheric Observatory (SOHO)) and possible changes of the velocity of the prominence material are presented. The mechanisms that generate the variations in the material movement are discussed.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Ts Tsvetkov, N. Petrov,