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Magnetic and velocity fields over active regions

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dc.contributor.author Gosain, S
dc.contributor.author Choudhary, D. B
dc.date.accessioned 2008-07-16T06:23:37Z
dc.date.available 2008-07-16T06:23:37Z
dc.date.issued 2002-09
dc.identifier.citation BASI, Vol. 30, No. 3, pp. 579 - 581 en
dc.identifier.uri http://hdl.handle.net/2248/2707
dc.description.abstract In order to understand the nature of dynamics over an active region (AR) , it is necessary to study the velocity and magnetic fields simultaneously. We present the preliminary results from our analysis of spectropolarimetric observations of active region NOAA-8426 over two days. These observations were done using Advanced Stokes Polarimeter (ASP) instrument of HAO-NSO (Elmore et al. 1992, Lites 1996) with the Richard Dunn Vacuum Tower Telescope, USA. The line-of-sight (LOS) magnetic field information is derived using least squares fitting of the Stokes-V profiles, in a weak field approximation. Simultaneous LOS velocity information over these AR is obtained in two ways: (i) Zero-crossing (ZC) velocities using Stokes-V profiles, and (li) centre of gravity (COG) velocities using Stokes-I profiles. The former corresponds to the magnetised plasma whereas the latter to the gross plasma over the AR. Average relative velocities of isolated polarity regions of the AR are presented in this paper. en
dc.format.extent 97014 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.subject Centre of Gravity en
dc.subject Magnetic and Velocity Fields en
dc.title Magnetic and velocity fields over active regions en
dc.type Article en


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