Original title: Estimation of the Apparent Source Size of Solar Radio Emissions Using SVD: An Application to Type III Radio Bursts at Long Wavelengths Observed by STEREO and Wind
Authors: Krupař, Vratislav ; Santolík, Ondřej ; Cecconi, B. ; Maksimovic, M.
Document type: Papers
Conference/Event: Week of Doctoral Students 2010. Annual Student Conference /19./, Prague (CZ), 2010-06-01 / 2010-06-04
Year: 2010
Language: eng
Abstract: Type III radio bursts are intense solar radio emissions. They are frequently observed by the S/Waves instruments on-board the STEREO spacecraft. We describe a wave propagation analysis using the Singular Value Decomposition (SVD) which can be directly applied to spectral matrices measured by the High Frequency Receiver (HFR; a part of the S/Waves experiment). We have found an empirical relation between the decomposed spectral matrices and apparent source sizes for waves with a low degree of polarization. We present a joint observation of a type III radio burst by the STEREO and Wind spacecraft during small separation distances. We obtain consistent results for the apparent source size and k-vector direction using different analysis method for the measurements of the STEREO and Wind spacecraft. We demonstrate that SVD can be an effective tool for the wave analysis of radio emissions with very extended sources.
Keywords: Solar Radio; STEREO; SVD; Wavelengths
Project no.: CEZ:AV0Z30420517 (CEP), ME09107 (CEP), IAA301120601 (CEP)
Funding provider: GA MŠk, GA AV ČR
Host item entry: WDS’10 Proceedings of Contributed Papers: Part II – Physics of Plasmas and Ionized Media, ISBN 978-80-7378-140-8

Institution: Institute of Atmospheric Physics AS ČR (web)
Document availability information: Fulltext is available at the institute of the Academy of Sciences.
Original record: http://hdl.handle.net/11104/0195832

Permalink: http://www.nusl.cz/ntk/nusl-42632


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Research > Institutes ASCR > Institute of Atmospheric Physics
Conference materials > Papers
 Record created 2011-07-04, last modified 2024-01-26


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