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Magnetic Switchbacks Heat the Solar Corona
Akhavan-Tafti, M.; Kasper, J.; Huang, J.; Thomas, L.;
Published by: \apjl Published on: oct
YEAR: 2022   DOI: 10.3847/2041-8213/ac913d
Parker Data Used; Solar coronal heating; Solar magnetic reconnection; Solar wind; Heliosphere; 1989; 1504; 1534; 711
Discontinuity analysis of the leading switchback transition regions
Context. Magnetic switchbacks are magnetic structures characterized as intervals of sudden reversal in the radial component of the pristine solar wind s magnetic field. Switchbacks comprise of magnetic spikes that are preceded and succeeded by switchback transition regions within which the radial magnetic field reverses. Determining switchback generation and evolution mechanisms will further our understanding of the global circulation and transportation of the Sun s open magnetic flux.
Akhavan-Tafti, M.; Kasper, J.; Huang, J.; Bale, S.;
Published by: Astronomy and Astrophysics Published on: 06/2021
YEAR: 2021   DOI: 10.1051/0004-6361/202039508
magnetic reconnection; magnetic fields; Solar wind; methods: data analysis; magnetohydrodynamics (MHD); instabilities; Parker Data Used