Solar energetic particles and radio burst emission

0489395 - ÚFA 2019 RIV FR eng J - Článek v odborném periodiku
Miteva, R. - Samwel, S. W. - Krupař, Vratislav
Solar energetic particles and radio burst emission.
Journal of Space Weather and Space Climate. Roč. 7, DEC (2017), č. článku A37. ISSN 2115-7251. E-ISSN 2115-7251
Grant CEP: GA ČR(CZ) GJ17-06818Y
Institucionální podpora: RVO:68378289
Klíčová slova: solar energetic particles * solar radio burst emission * solar cycle
Obor OECD: Fluids and plasma physics (including surface physics)
Impakt faktor: 2.333, rok: 2017
https://www.swsc-journal.org/articles/swsc/abs/2017/01/swsc170028/swsc170028.html

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.
Trvalý link: http://hdl.handle.net/11104/0283814