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dc.contributor.authorHough, J.
dc.contributor.editorMishchenko, M.I.
dc.contributor.editorYatskiv, Y.S.
dc.contributor.editorRosenbush, V.K.
dc.contributor.editorVideen, G.
dc.identifier.citationHough , J 2010 , High sensitivity polarimetry : techniques and applications . in M I Mishchenko , Y S Yatskiv , V K Rosenbush & G Videen (eds) , Polarimetric Detection, Characterization and Remote Sensing . Springer , pp. 177-204 .
dc.identifier.otherPURE: 162528
dc.identifier.otherPURE UUID: 3b6c364c-e91a-4497-8165-f5238cba459e
dc.identifier.otherdspace: 2299/5936
dc.identifier.otherScopus: 84883343794
dc.description“The original publication is available at” Copyright Springer [Due to publisher restrictions the full text of this book chapter is not available in the UHRA]
dc.description.abstractHigh sensitivity polarimetry will refer to fractional polarizations of below, and often significantly below, 103. Measuring low fractional polarization requires a large number of photons and also special techniques are needed to remove systematic effects. The highest sensitivities have been achieved using very fast modulation with single-element detectors, giving sensitivities of 106, or better, in fractional polarization. However, it is often important to have good spatial and/or spectral information and to provide this efficiently requires the use of area detectors which bring their own problems, particularly for the highest sensitivities. Applications of highly sensitive polarimetry described here, include observing the reflected light from exoplanets, the properties of dust in the Earth’s atmos-phere, and the remote sensing of biomarkers.en
dc.relation.ispartofPolarimetric Detection, Characterization and Remote Sensing
dc.subjectstokes parameters
dc.subjecttemporal and spatial modulation
dc.subjectatmospheric dust
dc.titleHigh sensitivity polarimetry : techniques and applicationsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research

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