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Meridional Motion and Reynolds Stress from Debrecen Photoheliographic Data

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    SYSNO ASEP0480935
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleMeridional Motion and Reynolds Stress from Debrecen Photoheliographic Data
    Author(s) Sudar, D. (HR)
    Brajša, R. (HR)
    Skokić, Ivica (ASU-R)
    Beljan, I.P. (HR)
    Woehl, H. (DE)
    Source TitleSolar Physics. - : Springer - ISSN 0038-0938
    Roč. 292, č. 7 (2017), 86/1-86/13
    Number of pages13 s.
    Publication formPrint - P
    Languageeng - English
    CountryNL - Netherlands
    Keywordssunspots ; rotation ; velocity fields
    Subject RIVBN - Astronomy, Celestial Mechanics, Astrophysics
    OECD categoryAstronomy (including astrophysics,space science)
    R&D Projects7E13003 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Institutional supportASU-R - RVO:67985815
    UT WOS000406304300004
    EID SCOPUS85021091545
    DOI10.1007/s11207-017-1105-4
    Annotationhe Debrecen Photoheliographic Data catalogue is a continuation of the Greenwich Photoheliographic Results providing daily positions of sunspots and sunspot groups. We analyse the data for sunspot groups focussing on meridional motions and transfer of angular momentum towards the solar equator. Velocities are calculated with a daily shift method including an automatic iterative process of removing the outliers. Apart from the standard differential rotation profile, we find meridional motion directed towards the zone of solar activity. The difference in measured meridional flow in comparison to Doppler measurements and some other tracer measurements is interpreted as a consequence of different flow patterns inside and outside of active regions. We also find a statistically significant dependence of meridional motion on rotation velocity residuals confirming the transfer of angular momentum towards the equator. Analysis of horizontal Reynolds stress reveals that the transfer of angular momentum is stronger with increasing latitude up to about 40 degrees, where there is a possible maximum in absolute value.
    WorkplaceAstronomical Institute
    ContactRadka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
    Year of Publishing2018
Number of the records: 1  

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