LOFAR observations of fundamental and harmonic type III emission during an M class flare

Jul 8, 2021, 6:48 PM
4m
Virtual

Virtual

Connection details will be available soon
Working Group 2: Particle acceleration Working Group 2: Particle acceleration

Speaker

Christian Vocks (Leibniz-Institute for Astrophysics Potsdam)

Description

We present observations of an M class flare with the LOw Frequency ARray (LOFAR) in the morning hours of 7 September 2017. The flare was accompanied by strong type III radio bursts. LOFAR interferometric images in the low band frequency range of 20 - 80 MHz show distinct sources that show variations in their positions, and intermittent dual source structures. We identify these as fundamental and harmonic emission, with the one or other being dominant at times. These distinct sources and their evolution allow for obtaining separate lightcurves for both fundamental and harmonic emission. The data show that transport effects due to refraction and scattering play a significant role, both in source separation and drift of their apparent positions.
Comparing the light curves of fundamental and harmonic pairs, e.g. 35 MHz fundamental and 70 MHz harmonic, enables studies of radio wave propagation in the solar corona. Observations of harmonic emission can provide information on source locations high in the corona, where fundamental emission would be near or below the ionospheric cutoff at 10 MHz. These are relevant for the transition into the solar wind, and for joint observing campaigns with Parker Solar Probe and Solar Orbiter that are currently investigating the inner heliosphere.

Email cvocks@aip.de

Primary author

Christian Vocks (Leibniz-Institute for Astrophysics Potsdam)

Co-authors

Prof. Andrzej Krankowski (University of Warmia and Mazury in Olsztyn) Dr Barbara Matyjasiak (Space Research Centre of Polish Academy of Sciences) Dr Bartosz Dabrowski (University of Warmia and Mazury in Olsztyn) Dr Christophe Marque (Royal Observatory of Belgium) Dr Diana E. Morosan (Department of Physics, University of Helsinki, P.O. Box 64, FI-00014 Helsinki, Finland.) Dr Eoin Carley (Dublin Institute for Advanced Studies) Dr Gottfried Mann (Leibniz-Institut für Astrophysik Potsdam (AIP), Potsdam, Germany) Prof. Hanna Rotkaehl (Space Research Centre of Polish Academy of Sciences) Dr Jasmina Magdalenic (Solar-Terrestrial Centre of Excellence—SIDC, Royal Observatory of Belgium, 3 Avenue Circulaire, B-1180 Uccle, Belgium. /Center for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, Celestijnenlaan 200B, B-3001 Leuven, Belgium) Dr Mario Bisi (STFC - Rutherford Appleton Laboratory (RAL Space)) Prof. Peter Gallagher (Dublin Institute for Advanced Studies) Dr Pietro Zucca (AASTRON Netherlands Institute for Radio Astronomy) Dr Richard Fallows (ASTRON, The Netherlands Institute for Radio Astronomy, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands.)

Presentation materials