Skip navigation
Skip navigation

Shock location and CME 3D reconstruction of a solar type II radio burst with LOFAR

Butcher, Harvey; Zucca, P; Morosan, D E; Rouillard, A P; Fallows, R; Gallagher, P T; Magdalenic, J; Klein, K-L; Mann, Gottfried; Vocks, Christian; Carley, E P; Bisi, M M


Context. Type II radio bursts are evidence of shocks in the solar atmosphere and inner heliosphere that emit radio waves ranging from sub-meter to kilometer lengths. These shocks may be associated with coronal mass ejections (CMEs) and reach speeds higher than the local magnetosonic speed. Radio imaging of decameter wavelengths (20–90 MHz) is now possible with the Low Frequency Array (LOFAR), opening a new radio window in which to study coronal shocks that leave the inner solar corona and enter...[Show more]

CollectionsANU Research Publications
Date published: 2018
Type: Journal article
Source: Astronomy and Astrophysics
DOI: 10.1051/0004-6361/201732308
Access Rights: Open Access


File Description SizeFormat Image
01_Butcher_Shock_location_and_CME_3D_2018.pdf21.42 MBAdobe PDFThumbnail

Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  19 May 2020/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator