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Diagnosing the Source Region of a Solar Burst on 26 September 2011 by Using Microwave Type-III Pairs
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SYSNO ASEP 0470082 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Diagnosing the Source Region of a Solar Burst on 26 September 2011 by Using Microwave Type-III Pairs Author(s) Tan, B.-L. (CN)
Karlický, Marian (ASU-R) RID, ORCID
Mészárosová, Hana (ASU-R) RID, ORCID
Kashapova, L. K. (RU)
Huang, J. (CN)
Yan, Y. (CN)
Kontar, E. P. (GB)Source Title Solar Physics. - : Springer - ISSN 0038-0938
Roč. 291, č. 8 (2016), s. 2407-2418Number of pages 12 s. Publication form Print - P Language eng - English Country NL - Netherlands Keywords Sun ; microwave emission ; magnetic reconnection Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics Institutional support ASU-R - RVO:67985815 UT WOS 000385207200011 EID SCOPUS 84986322635 DOI https://doi.org/10.1007/s11207-016-0986-y Annotation 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. Workplace Astronomical Institute Contact Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2017
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