Interferometric imaging with LOFAR remote baselines of the fine structures of a solar type-IIIb radio burst

Context. Solar radio bursts originate mainly from high energy electrons accelerated in solar eruptions like solar flares, jets, and coronal mass ejections. A sub-category of solar radio bursts with short time duration may be used as a proxy to understand wave generation and propagation within the co...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2020-07, Vol.639, p.A115, Article 115
Hauptverfasser:	Zhang, PeiJin, Zucca, Pietro, Sridhar, Sarrvesh Seethapuram, Wang, ChuanBing, Bisi, Mario M., Dabrowski, Bartosz, Krankowski, Andrzej, Mann, Gottfried, Magdalenic, Jasmina, Morosan, Diana E., Vocks, Christian
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy & Astrophysics Coronal mass ejection Emission analysis High energy electrons Imaging Interferometry Kinematics Light speed LOFAR Photovoltaic cells Physical Sciences Radio sources (astronomy) Science & Technology Solar corona Solar flares Solar radio bursts Wave generation Wave propagation
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