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

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發(fā)表于 2025-3-21 18:41:46 | 只看該作者 |倒序瀏覽 |閱讀模式
期刊全稱Astronomical Polarisation from the Infrared to Gamma Rays
影響因子2023Roberto Mignani,Andrew Shearer,Silvia Zane
視頻videohttp://file.papertrans.cn/164/163603/163603.mp4
發(fā)行地址A state-of-the-art review of polarisation principles and astronomical instrumentation.Provides detailed background information suitable for graduate students.Reviews current and future instrumentation
學科分類Astrophysics and Space Science Library
圖書封面Titlebook: Astronomical Polarisation from the Infrared to Gamma Rays;  Roberto Mignani,Andrew Shearer,Silvia Zane Book 2019 Springer Nature Switzerlan
影響因子.This book serves as both a primer to astronomical polarimetry and an authoritative overview of its application to various types of astronomical objects from AGN, compact stars, binary systems, stars across the HR diagram, transients, the interstellar medium and solar system bodies. It starts with an historical perspective, a discussion of polarimetric theory, instrumentation and techniques in wave bands from the near infrared to gamma rays. .The book presents the state of the art in astronomical polarimetry. It is motivated by the new X-ray polarimeters due to be launched in the next four years and improved optical polarimeters on large telescopes requiring a new analysis of polarimetric theory, methodology and results.This book will be suitable as advanced undergraduate companion text, a primer for graduate students and all researchers with an interest in astronomical polarimetry..
Pindex Book 2019
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Gamma-Ray Polarimetry,c nuclei, gamma-ray bursts, black hole binaries, pulsars, etc. The linear polarisation information of gamma-ray sources is measured usingCompton scattering up to a few MeV and the conversion of high-energy photons to electron–positron pairs at higher energies. Thanks to the development of gamma-ray
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Spectropolarimetry of Stars Across the H-R Diagram,o understand the origin, evolution, and structure of stellar magnetic fields in stars of different mass at different evolutionary stages. In this chapter we discuss recent measurements together with the underlying assumptions in the interpretation of data and the requirements, both observational and
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Polarimetry of Binary Systems: Polars, Magnetic CVs, XRBs,rvation. Indeed, radiation processes such as scattering by free electrons in the hot plasma above accretion discs, cyclotron emission by mildly relativistic electrons in the accretion shocks on the surface of highly magnetic white dwarfs and the optically thin synchrotron emission from jets can be o
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