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Solar energetic particles and radio burst emission View all abstracts by submitter

Rositsa Miteva   Submitted: 2017-12-30 08:58

We present a statistical study on the observed solar radio burst emission associated with the origin of in situ detected solar energetic particles. Several proton event catalogs in the period 1996-2016 are used. At the time of appearance of the particle origin (flare and coronal mass ejection) we identified radio burst signatures of types II, III and IV by inspecting dynamic radio spectral plots. The information from observatory reports is also accounted for during the analysis. The occurrence of solar radio burst signatures is evaluated within selected wavelength ranges during the solar cycle 23 and the ongoing 24. Finally, we present the burst occurrence trends with respect to the intensity of the proton events and the location of their solar origin.

Authors: R. Miteva, S. W. Samwel and V. Krupar
Projects: None

Publication Status: Published by EDP Sciences 2017
Last Modified: 2018-01-03 11:40
Go to main E-Print page  Understanding Breaks in Flare X-Ray Spectra: Evaluation of a Cospatial Collisional Return-current Model  A quasi-periodic fast-propagating magnetosonic wave associated with the eruption of a magnetic flux rope  Edit Entry  Download Preprint  Delete Entry 

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