Multiple regions of shock-accelerated particles during a solar coronal mass ejection

Multiple regions of shock-accelerated particles during a solar coronal mass ejection

The Sun is an active star that can launch large eruptions of magnetized plasma into the heliosphere, known as coronal mass ejections (CMEs). These can drive shocks that accelerate particles to high energies, often resulting in radio emission at low frequencies (

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Veröffentlicht in:Nature astronomy 2019-05, Vol.3 (5), p.452-461
Hauptverfasser: Morosan, Diana E., Carley, Eoin P., Hayes, Laura A., Murray, Sophie A., Zucca, Pietro, Fallows, Richard A., McCauley, Joe, Kilpua, Emilia K. J., Mann, Gottfried, Vocks, Christian, Gallagher, Peter T.
Format: Artikel
Sprache:eng
Schlagworte:
639/33/525/870
704/525/870
Astronomy
Astrophysics and Cosmology
Physics
Physics and Astronomy
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Zusammenfassung:The Sun is an active star that can launch large eruptions of magnetized plasma into the heliosphere, known as coronal mass ejections (CMEs). These can drive shocks that accelerate particles to high energies, often resulting in radio emission at low frequencies (
ISSN:2397-3366
2397-3366
DOI:10.1038/s41550-019-0689-z