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Meridional Motion and Reynolds Stress from Debrecen Photoheliographic Data
Authors:Davor Sudar  Roman Brajša  Ivica Skokić  Ivana Poljančić Beljan  Hubertus Wöhl
Affiliation:1.Hvar Observatory, Faculty of Geodesy,University of Zagreb,Zagreb,Croatia;2.Astronomical Institute of the Czech Academy of Sciences,Ond?ejov,Czech Republic;3.Department of Physics,University of Rijeka,Rijeka,Croatia;4.Kiepenheuer-Institut für Sonnenphysik,Freiburg,Germany
Abstract:The 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^{circ}), where there is a possible maximum in absolute value.
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