Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7589
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dc.contributor.authorNagendra, K. N (editor)-
dc.contributor.authorBagnulo, S (editor)-
dc.contributor.authorCenteno, R (editor)-
dc.contributor.authorMartinez Gonzalez, M. J (editor)-
dc.date.accessioned2021-02-07T04:36:20Z-
dc.date.available2021-02-07T04:36:20Z-
dc.date.issued2015-
dc.identifier.citationxxxv, 409p.en_US
dc.identifier.isbn978-1-107-07855-0-
dc.identifier.issn1743-9213-
dc.identifier.urihttp://hdl.handle.net/2248/7589-
dc.description© International Astronomical Union https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/issue/5B1813DE1E0E284744CF3F3ED11E5F85en_US
dc.description.abstractThe advances in solar, planetary, and extrasolar science employing polarimetric tools are far-reaching, and the pace of discovery is accelerating rapidly. In the last three decades, the emphasis of solar polarimetry has been to achieve simultaneously high spectral, spatial, and temporal resolution for all four Stokes parameters. In the field of stellar polarimetry the developments have been equally impressive, in allowing the detection and surface mapping of magnetic fields across the Hertzsprung–Russell diagram. This volume, arising from IAU Symposium 305, is devoted to sharing advances in science, data analysis, modeling, and instrumentation between solar and non-solar polarimetry communities. Given the relevance of polarimetric measurements to many aspects of astrophysics, the techniques and physical interpretations addressed within the book will be of interest to a wide audience of researchers and advanced students, in addition to those from solar and stellar communities.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.relation.ispartofseriesInternational Astronomical Union Symposium; Vol. 305-
dc.titlePolarimetry: from the sun to stars and stellar environmentsen_US
dc.typeBooken_US
Appears in Collections:Books Publication by IIAP

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