Cme Phenomenology in Different Solar Magnetic Scenarios |
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| Authors: | R Rodríguez Taboada G Gil Moreno A Méndez Berhondo R Pérez-Enriquez |
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| Institution: | (1) Institute of Geophysics and Astronomy, Calle 212 No. 2906, La Coronela, Havana, Cuba;(2) Institute of Geophysics, Universidad Nacional Autónoma de México, Ciudad Universitaria, Mexico D.F |
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| Abstract: | The existence of three magnetic scenarios with magnetic field intensities one order apart was considered. CMEs were associated to different solar activity phenomena and solar features showing different characteristics. Those associated to intense magnetic fields were more complex, having either more components or multiple emissions and a greater magnetic energy to particle acceleration conversion rate. On the other hand, simple CMEs were found to associate to weak magnetic fields. No evidence was found that the process that leads to CME starts before their detection at 1.6 solar radii. This indicates that the whole volume moves upward simultaneously, no matter how deep it reaches into the solar atmosphere. |
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