Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4191
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dc.contributor.authorBalasubramaniam, K. S-
dc.contributor.authorVenkatakrishnan, P-
dc.contributor.authorBhattacharyya, J. C-
dc.date.accessioned2008-12-29T12:29:29Z-
dc.date.available2008-12-29T12:29:29Z-
dc.date.issued1985-09-
dc.identifier.citationSolar Physics, Vol. 99, No. 1 - 2, pp. 333 - 348en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/4191-
dc.description.abstractThe observations of Stokes line profiles require an accurate knowledge of the instrumental polarisation caused by optical components in the path of the light beam. In this context we present a theoretical approach to the instrumental polarisation caused by the 3-mirror coelostat system of the Kodaikanal Solar Tower.en
dc.language.isoenen
dc.publisherD. Reidel Publishing Co.en
dc.relation.urihttp://dx.doi.org/10.1007/BF00157317en
dc.relation.urihttp://adsabs.harvard.edu/abs/1985SoPh...99..333Ben
dc.subjectMagnetic Measurementen
dc.subjectOptical Polarizationen
dc.subjectPolarimetryen
dc.subjectSolar Instrumentsen
dc.subjectTelescopesen
dc.subjectZeeman Effecten
dc.subjectForce Vector Recordersen
dc.subjectLine Spectraen
dc.subjectOptical Reflectionen
dc.subjectPolarization Characteristicsen
dc.subjectSolar Spectrometersen
dc.subjectStokes Theorem (Vector Calculus)en
dc.titleMeasurement of vector magnetic fields. I - Theoretical approach to the instrumental polarisation of the Kodaikanal Solar Toweren
dc.typeArticleen
Appears in Collections:IIAP Publications
J.C.Bhattacharyya (1982 - 1990)

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