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Tracking of an electron beam through the solar corona with LOFAR

Abstract:

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 rev...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1051/0004-6361/201629017

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Funding agency for:
Ferrari, C
Grant:
ANR-09-JCJC-0001-01
Publisher:
EDP Sciences Publisher's website
Journal:
Astronomy and Astrophysics Journal website
Volume:
611
Article number:
A57
Publication date:
2018-03-27
Acceptance date:
2017-11-14
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
Source identifiers:
835118
Keywords:
Pubs id:
pubs:835118
UUID:
uuid:1ef64a3c-fa9f-4f92-a71c-f5c69edde3d4
Local pid:
pubs:835118
Deposit date:
2018-04-23

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