LOFAR tied-array imaging of Type III solar radio bursts

2014/07/16 by D. E. Morosan, P. T. Gallagher, P. Zucca +82 · 78 citations
Physics and Astronomy · #Corona (planetary geology) #Coronal loop #Coronal mass ejection #Gamma-ray bursts and supernovae #LOFAR #Pulsars and Gravitational Waves Research #Solar and Space Plasma Dynamics #Solar flare #Solar physics #Solar radio #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201423936

published in Astronomy and Astrophysics 568, A67 (EDP Sciences) · 9 pages, 6 figures

arxiv created 2014/07/16 · openalex publication_date 2014/07/18 · arxiv updated 2014/09/05 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06

Abstract

Context. The Sun is an active source of radio emission which is often associated with energetic phenomena such as solar flares and coronal mass ejections (CMEs). At low radio frequencies (<100 MHz), the Sun has not been imaged extensively because of the instrumental limitations of previous radio telescopes.

Citations

• WAVES: The radio and plasma wave investigation on the wind spacecraft
• The STEREO mission: an overview
• The Large Angle Spectroscopic Coronagraph (LASCO)
• The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)

Cited by

• On Solar Recurrent Coronal Jets: Coronal Geysers as Sources of Electron Beams and Interplanetary Type-III Radio Bursts