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Paper: The Distributions of UV Solar Explosive Events
Volume: 463, 2nd ATST-EAST Workshop in Solar Physics: Magnetic Fields from the Photosphere to the Corona
Page: 181
Authors: Mendoza-Torres, J. E.; Niembro-Hernandez, T.
Abstract: We analyze solar Explosive Events observed at the Si IV 139.37 nm emission line in raster mode with SUMER/SoHO. The spatial distributions of EE with different Doppler velocities are analyzed. Spatial offsets of the maximum of the distributions as well as the presence of two sources are commonly observed at the analyzed EE. Also, at some locations near the maximum the 0–18 km s-1 distributions are similar to each other in shape and amplitude. These characteristics indicate that the red and blue Doppler EE sources could be the result of flows inside magnetic arcs.
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