Diagnosing the Source Region of a Solar Burst on 26 September 2011 by Using Microwave Type-III Pairs
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00470082" target="_blank" >RIV/67985815:_____/16:00470082 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1007/s11207-016-0986-y" target="_blank" >http://dx.doi.org/10.1007/s11207-016-0986-y</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1007/s11207-016-0986-y" target="_blank" >10.1007/s11207-016-0986-y</a>
Alternative languages
Result language
angličtina
Original language name
Diagnosing the Source Region of a Solar Burst on 26 September 2011 by Using Microwave Type-III Pairs
Original language description
We report a peculiar and interesting train of microwave Type-III pair bursts in the impulsive rising phase of a solar flare on 26 September 2011. The observations include radio spectrometers at frequencies of 0.80 -aEuroe2.00 GHz from the OndA (TM) ejov radiospectrograph in the Czech Republic (ORSC), hard X-ray from the Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) and Gamma-Ray Burst Monitor onboard the Fermi Space Telescope (Fermi/GRB), EUV images from the Sun Watcher using APS detectors and image Processing instrument onboard the Project for Onboard Autonomy 2 (SWAP/PROBA2), and magnetograms from the Helioseismic and Magnetic Imager onboard the Solar Dynamic Observatory (SDO/HMI). By using a recently developed method (Tan et al., Res. Astron. Astrophys. 16, 82, 2016a), we diagnosed the plasma density, temperature, plasma-, magnetic field near the source region, the energy of energetic electrons, and the distance between the acceleration region and the emission start sites of Type-III bursts.
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Solar Physics
ISSN
0038-0938
e-ISSN
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Volume of the periodical
291
Issue of the periodical within the volume
8
Country of publishing house
NL - THE KINGDOM OF THE NETHERLANDS
Number of pages
12
Pages from-to
2407-2418
UT code for WoS article
000385207200011
EID of the result in the Scopus database
2-s2.0-84986322635