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Forward-scattering Hanle effect in the solar Ca i 4227 Å line

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dc.contributor.author Frisch, H
dc.contributor.author Anusha, L. S
dc.contributor.author Bianda, M
dc.contributor.author Holzreuter, R
dc.contributor.author Nagendra, K. N
dc.contributor.author Ramelli, R
dc.contributor.author Sampoorna, M
dc.contributor.author Smitha, H. N
dc.contributor.author Stenflo, J. O
dc.date.accessioned 2012-07-18T14:58:57Z
dc.date.available 2012-07-18T14:58:57Z
dc.date.issued 2012-06
dc.identifier.citation EAS Publications Series, Vol. 55, pp. 59-63 en
dc.identifier.issn 1633-4760
dc.identifier.uri http://hdl.handle.net/2248/5797
dc.description Restricted Access en
dc.description.abstract High sensitivity spectropolarimetric observations of the four Stokes parameters of the solar Ca i 4227 Å line have been performed in October 2010 at IRSOL with the ZIMPOL polarimeter, near the disk center, outside an active region (Bianda et al. 2011). They were analyzed in Anusha et al. 2011 with a combination of detailed radiative transfer modelling of the Hanle effect for the linear polarization and weak field Zeeman approximation for the circular polarization. This approach made possible a unique determination of the magnetic field vector at various positions along the slit of the spectrograph. A summary of the observations and of their analysis is presented here. en
dc.language.iso en en
dc.publisher Cambridge University Press en
dc.relation.uri http://dx.doi.org/10.1051/eas/1255007 en
dc.rights © EDP Sciences en
dc.subject Magnetic field en
dc.subject Polarization MeasurementsTheory en
dc.subject Polarization theory en
dc.title Forward-scattering Hanle effect in the solar Ca i 4227 Å line en
dc.type Article en


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