Titlebook: Astronomical Polarisation from the Infrared to Gamma Rays; Roberto Mignani,Andrew Shearer,Silvia Zane Book 2019 Springer Nature Switzerlan

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Magnetic Fields in Gamma-Ray Bursts and Their Polarised Emission,ed to be the dominant radiation process for the main emission components of GRBs, i.e. prompt gamma-rays, reverse shock emission and afterglow. Although the presence of strong magnetic fields in the emission regions is crucial to produce the bright emission, the origin and its role in the dynamics a

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The Panchromatic Polarisation Signatures of Active Galactic Nuclei,of complex yet fundamental signatures that helped to understand their true nature. Indeed, AGN exhibit a wide range of wavelength-dependent polarimetric features that are intrinsically related to their multi-scale emission mechanisms. Each waveband is characterised by a different set of polarimetric

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Hauptbodenarten, Bodenbeschreibung,mical literature has featured about one polarimetry-related work for every eight spectroscopy-related works. Important mile stones of astronomical polarimetry have been the observations of the solar corona since the 1840s; the theory and observation of polarised light reflected from solar system bod

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,Pflanzenernährung und Pflanzengifte,it propagates through a system can be modelled mathematically using Mueller orJones algebra. ThePoincaré sphere is another useful tool to describe the change in polarisation state due to the effects of a component. A polarimeter is an instrument that can be used to measure the polarisation state of

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,Pflanzenernährung und Pflanzengifte,avelengths. We describe the properties of various polarisation devices and detectors used for optical broadband, imaging and spectropolarimetry, and discuss their advantages and disadvantages. The necessity of a proper calibration of the raw polarisation data is emphasised and methods of the determi

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