Issue |
A&A
Volume 611, March 2018
|
|
---|---|---|
Article Number | A57 | |
Number of page(s) | 9 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361/201629017 | |
Published online | 27 March 2018 |
Tracking of an electron beam through the solar corona with LOFAR
1
Leibniz-Institut für Astrophysik Potsdam (AIP),
An der Sternwarte 16,
14482 Potsdam, Germany
e-mail: GMann@aip.de, frank.breitling@gmx.de
2
RAL Space, Science & Technology Facilities Council (STFC) – Rutherford Appleton Laboratory (RAL),
Harwell Oxford,
Oxfordshire,
OX11 0QX, UK
3
ASTRON, Netherlands Institute for Radio Astronomy,
Postbus 2,
7990 AA
Dwingeloo, The Netherlands
4
Astrophysics Research Group, School of Physics, Trinity College Dublin,
Dublin 2, Ireland
5
LESIA & USN, Observatoire de Paris, CNRS, PSL/SU/UPMC/UPD/SPC, Place J. Janssen,
92195
Meudon, France
6
SUPA, School of Physics and Astronomy, University of Glasgow,
Glasgow
G12 8QQ, UK
7
Solar-Terrestrial Center of Excellence, SIDC, Royal Observatory of Belgium,
Avenue Circulaire 3,
1180
Brussels, Belgium
8
Space Research Institute, Austrian Academy of Sciences,
Schmiedl Strasse 6,
8042
Graz, Austria
9
Helmholtz-Zentrum Potsdam, Deutsches GeoForschungs Zentrum GFZ, Department 1: Geodesy and Remote Sensing,
Telegrafenberg, A17,
14473 Potsdam, Germany
10
Shell Technology Center,
Bangalore, India
11
SRON Netherlands Insitute for Space Research,
PO Box 800, 9700 AV Groningen, The Netherlands
12
Kapteyn Astronomical Institute,
PO Box 800, 9700 AV Groningen, The Netherlands
13
CSIRO Australia Telescope National Facility,
PO Box 76, Epping NSW 1710, Australia
14
University of Twente,
Enschede, The Netherlands
15
Harvard-Smithsonian Center for Astrophysics,
60 Garden Street,
Cambridge,
MA 02138, USA
16
Institute for Astronomy, University of Edinburgh, Royal Observatory of Edinburgh,
Blackford Hill,
Edinburgh
EH9 3HJ, UK
17
Leiden Observatory, Leiden University,
PO Box 9513, 2300 RA
Leiden, The Netherlands
18
University of Hamburg,
Gojenbergsweg 112,
21029
Hamburg, Germany
19
School of Physics and Astronomy, University of Southampton,
Southampton
SO17 1BJ, UK
20
Research School of Astronomy and Astrophysics, Australian National University,
Mt Stromlo Obs., via Cotter Road, Weston,
A.C.T. 2611, Australia
21
Max Planck Institute for Astrophysics,
Karl Schwarzschild Str. 1,
85741
Garching, Germany
22
Department of Astrophysics/IMAPP, Radboud University Nijmegen,
P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
23
SmarterVision BV,
Oostersingel 5,
9401 JX
Assen, The Netherlands
24
Thüringer Landessternwarte,
Sternwarte 5,
07778
Tautenburg, Germany
25
Hamburger Sternwarte,
Gojenbergsweg 112,
21029
Hamburg, Germany
26
Astrophysics, University of Oxford,
Denys Wilkinson Building, Keble Road,
Oxford
OX1 3RH, UK
27
Laboratoire Lagrange, UMR7293, Université de Nice Sophia Antipolis, CNRS, Observatoire de la Côte d’Azur,
06300
Nice, France
28
LPC2E – Université d’Orléans/CNRS, France
29
Station de Radioastronomie de Nançay, Observatoire de Paris – CNRS/INSU, USR 704 – Univ. Orléans, OSUC, route de Souesmes,
18330
Nançay, France
30
Anton Pannekoek Institute, University of Amsterdam,
Postbus 94249, 1090 GE
Amsterdam, The Netherlands
31
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69,
53121
Bonn, Germany
32
Astronomisches Institut der Ruhr-Universität Bochum,
Universitaetsstrasse 150,
44780
Bochum, Germany
33
Astro Space Center of the Lebedev Physical Institute,
Profsoyuznaya str. 84/32,
117997
Moscow, Russia
34
Jodrell Bank Center for Astrophysics, School of Physics and Astronomy, The University of Manchester,
Manchester
M13 9PL, UK
35
Sodankylä Geophysical Observatory, University of Oulu,
Tähteläntie 62,
99600
Sodankylä, Finland
36
STFC Rutherford Appleton Laboratory, Harwell Science and Innovation Campus,
Didcot
OX11 0QX, UK
37
Center for Information Technology (CIT), University of Groningen,
Groningen, The Netherlands
38
Centre de Recherche Astrophysique de Lyon, Observatoire de Lyon,
9 Av. Charles André,
69561 Saint-Genis-Laval Cedex, France
39
Fakultät für Physik, Universität Bielefeld,
Postfach 100131,
33501
Bielefeld, Germany
40
Department of Physics and Elelctronics, Rhodes University,
PO Box 94,
Grahamstown 6140, South Africa
41
SKA South Africa,
3rd Floor, The Park, Park Road,
Pinelands
7405, South Africa
Received:
27
May
2016
Accepted:
14
November
2017
The Sun’s activity leads to bursts of radio emission, among other phenomena. An example is type-III radio bursts. They occur frequently and appear as short-lived structures rapidly drifting from high to low frequencies in dynamic radio spectra. They are usually interpreted as signatures of beams of energetic electrons propagating along coronal magnetic field lines. Here we present novel interferometric LOFAR (LOw Frequency ARray) observations of three solar type-III radio bursts and their reverse bursts with high spectral, spatial, and temporal resolution. They are consistent with a propagation of the radio sources along the coronal magnetic field lines with nonuniform speed. Hence, the type-III radio bursts cannot be generated by a monoenergetic electron beam, but by an ensemble of energetic electrons with a spread distribution in velocity and energy. Additionally, the density profile along the propagation path is derived in the corona. It agrees well with three-fold coronal density model by (1961, ApJ, 133, 983).
Key words: acceleration of particles / instrumentation: interferometers / techniques: interferometric / Sun: radio radiation / Sun: flares / Sun: corona
© ESO 2018
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