Tracking of an electron beam through the solar corona with LOFAR Article Swipe
G. Mann
,
F. Breitling
,
C. Vocks
,
H. Auraß
,
Matthias Steinmetz
,
K. G. Strassmeier
,
M. M. Bisi
,
R. A. Fallows
,
P. T. Gallagher
,
A. Kerdraon
,
A. L. MacKinnon
,
Jasmina Magdalenić
,
H. O. Rucker
,
J. M. Anderson
,
A. Asgekar
,
I. M. Avruch
,
M. E. Bell
,
Mark Bentum
,
G. Bernardi
,
P. N. Best
,
L. Bırzan
,
A. Bonafede
,
J. W. Broderick
,
M. Brüggen
,
H. R. Butcher
,
B. Ciardi
,
A. Corstanje
,
F. de Gasperin
,
E. de Geus
,
Adam T. Deller
,
S. Duscha
,
J. Eislöffel
,
D. Engels
,
H. Falcke
,
R. P. Fender
,
C. Ferrari
,
W. Frieswijk
,
M. A. Garrett
,
J.‐M. Grießmeier
,
A. W. Gunst
,
Michiel van Haarlem
,
T. E. Hassall
,
G. Heald
,
J. W. T. Hessels
,
M. Hoeft
,
J.R. Hörandel
,
A. Horneffer
,
E. Juette
,
A. Karastergiou
,
Wouter Klijn
,
V. I. Kondratiev
,
M. Krämer
,
M. Kuniyoshi
,
G. Küper
,
P. Maat
,
Sera Markoff
,
R. McFadden
,
D. McKay‐Bukowski
,
J. P. McKean
,
D. D. Mulcahy
,
H. Munk
,
A. Nelles
,
M. J. Norden
,
E. Orrú
,
H. Paas
,
M. Pandey-Pommier
,
V. N. Pandey
,
R. Pizzo
,
A. G. Polatidis
,
D. A. Rafferty
,
W. Reich
,
H. J. A. Röttgering
,
A. Scaife
,
Dominik J. Schwarz
,
M. Serylak
,
J. Sluman
,
O. Smirnov
,
B. W. Stappers
,
M. Tagger
,
Y. Tang
,
C. Tasse
,
S. ter Veen
,
S. Thoudam
,
M. C. Toribio
,
R. C. Vermeulen
,
R. J. van Weeren
,
M. W. Wise
,
O. Wucknitz
,
S. Yatawatta
,
P. Zarka
,
J. A. Zensus
·
YOU?
·
· 2017
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/201629017
YOU?
·
· 2017
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/201629017
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).
Related Topics
Concepts
Physics
LOFAR
Astrophysics
Corona (planetary geology)
Nanoflares
Electron
Magnetic field
Solar physics
Coronal loop
Astronomy
Solar flare
Computational physics
Coronal mass ejection
Solar wind
Radio telescope
Quantum mechanics
Astrobiology
Venus
Metadata
- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.1051/0004-6361/201629017
- https://www.aanda.org/articles/aa/pdf/2018/03/aa29017-16.pdf
- OA Status
- hybrid
- Cited By
- 41
- References
- 31
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W2768467969
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W2768467969Canonical identifier for this work in OpenAlex
- DOI
-
https://doi.org/10.1051/0004-6361/201629017Digital Object Identifier
- Title
-
Tracking of an electron beam through the solar corona with LOFARWork title
- Type
-
articleOpenAlex work type
- Language
-
enPrimary language
- Publication year
-
2017Year of publication
- Publication date
-
2017-11-24Full publication date if available
- Authors
-
G. Mann, F. Breitling, C. Vocks, H. Auraß, Matthias Steinmetz, K. G. Strassmeier, M. M. Bisi, R. A. Fallows, P. T. Gallagher, A. Kerdraon, A. L. MacKinnon, Jasmina Magdalenić, H. O. Rucker, J. M. Anderson, A. Asgekar, I. M. Avruch, M. E. Bell, Mark Bentum, G. Bernardi, P. N. Best, L. Bırzan, A. Bonafede, J. W. Broderick, M. Brüggen, H. R. Butcher, B. Ciardi, A. Corstanje, F. de Gasperin, E. de Geus, Adam T. Deller, S. Duscha, J. Eislöffel, D. Engels, H. Falcke, R. P. Fender, C. Ferrari, W. Frieswijk, M. A. Garrett, J.‐M. Grießmeier, A. W. Gunst, Michiel van Haarlem, T. E. Hassall, G. Heald, J. W. T. Hessels, M. Hoeft, J.R. Hörandel, A. Horneffer, E. Juette, A. Karastergiou, Wouter Klijn, V. I. Kondratiev, M. Krämer, M. Kuniyoshi, G. Küper, P. Maat, Sera Markoff, R. McFadden, D. McKay‐Bukowski, J. P. McKean, D. D. Mulcahy, H. Munk, A. Nelles, M. J. Norden, E. Orrú, H. Paas, M. Pandey-Pommier, V. N. Pandey, R. Pizzo, A. G. Polatidis, D. A. Rafferty, W. Reich, H. J. A. Röttgering, A. Scaife, Dominik J. Schwarz, M. Serylak, J. Sluman, O. Smirnov, B. W. Stappers, M. Tagger, Y. Tang, C. Tasse, S. ter Veen, S. Thoudam, M. C. Toribio, R. C. Vermeulen, R. J. van Weeren, M. W. Wise, O. Wucknitz, S. Yatawatta, P. Zarka, J. A. ZensusList of authors in order
- Landing page
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https://doi.org/10.1051/0004-6361/201629017Publisher landing page
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https://www.aanda.org/articles/aa/pdf/2018/03/aa29017-16.pdfDirect link to full text PDF
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YesWhether a free full text is available
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hybridOpen access status per OpenAlex
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https://www.aanda.org/articles/aa/pdf/2018/03/aa29017-16.pdfDirect OA link when available
- Concepts
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Physics, LOFAR, Astrophysics, Corona (planetary geology), Nanoflares, Electron, Magnetic field, Solar physics, Coronal loop, Astronomy, Solar flare, Computational physics, Coronal mass ejection, Solar wind, Radio telescope, Quantum mechanics, Astrobiology, VenusTop concepts (fields/topics) attached by OpenAlex
- Cited by
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41Total citation count in OpenAlex
- Citations by year (recent)
-
2025: 7, 2024: 4, 2023: 6, 2022: 2, 2021: 9Per-year citation counts (last 5 years)
- References (count)
-
31Number of works referenced by this work
- Related works (count)
-
10Other works algorithmically related by OpenAlex
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