Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6731
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dc.contributor.authorPanini, S. S-
dc.contributor.authorSreekumar, P-
dc.contributor.authorMarshall, H. L-
dc.contributor.authorNarendranath, S-
dc.contributor.authorNayak, M-
dc.contributor.authorAthiray, P. S-
dc.date.accessioned2020-11-10T02:30:24Z-
dc.date.available2020-11-10T02:30:24Z-
dc.date.issued2018-01-
dc.identifier.citationJournal of Astronomical Telescopes, Instruments, and Systems, Vol. 3, No. 4, pp. 011002-1 - 011002-9en_US
dc.identifier.issn2329-4221-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6731-
dc.descriptionRestricted Access © SPIE--The International Society for Optical Engineering; https://doi.org/10.1117/1.JATIS.4.1.011002en_US
dc.description.abstractA simple design of a soft x-ray polarimeter using multilayer mirrors is presented. A multilayer mirror acts as a linear polarization analyzer for x-rays at incidence angles close to the Brewster angle. The instrument consists of an x-ray concentrator, a set of multilayer mirrors placed at 45 deg from the optical axis, and a detector at Nasmyth focus. The instrument rotating about its optical axis during observations can measure the linear polarization of 0.2- to 0.7-keV x-rays from astronomical sources. The use of a soft x-ray concentrator with geometrical area ∼630  cm2 provides sufficient sensitivity to address key scientific questions. Five different multilayer mirrors placed on a rotating wheel provide the option to measure polarization in any of the five narrow bands spanning the 0.2- to 0.7-keV range. Design and estimated performance of the design are discussed.en_US
dc.language.isoenen_US
dc.publisherSPIE-The International Society for Optical Engineeringen_US
dc.subjectMultilayer mirrorsen_US
dc.subjectSoft x-raysen_US
dc.subjectPolarimeteren_US
dc.titleMultilayer mirror-based soft x-ray polarimeter for astronomical observationsen_US
dc.typeArticleen_US
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