標(biāo)題: Titlebook: Astronomical Polarisation from the Infrared to Gamma Rays; Roberto Mignani,Andrew Shearer,Silvia Zane Book 2019 Springer Nature Switzerlan [打印本頁(yè)] 作者: 從未沮喪 時(shí)間: 2025-3-21 18:41
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays影響因子(影響力)
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays影響因子(影響力)學(xué)科排名
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays被引頻次
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays被引頻次學(xué)科排名
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays年度引用
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays年度引用學(xué)科排名
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays讀者反饋
書(shū)目名稱Astronomical Polarisation from the Infrared to Gamma Rays讀者反饋學(xué)科排名
作者: MUT 時(shí)間: 2025-3-21 20:31 作者: Lacunar-Stroke 時(shí)間: 2025-3-22 04:22 作者: 種子 時(shí)間: 2025-3-22 07:58 作者: 淺灘 時(shí)間: 2025-3-22 12:15
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 作者: cinder 時(shí)間: 2025-3-22 15:35 作者: 機(jī)密 時(shí)間: 2025-3-22 18:50
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作者: 侵略主義 時(shí)間: 2025-3-23 00:33 作者: pineal-gland 時(shí)間: 2025-3-23 02:28
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作者: Indent 時(shí)間: 2025-3-23 05:51 作者: Filibuster 時(shí)間: 2025-3-23 13:25
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作者: NIB 時(shí)間: 2025-3-23 14:01
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作者: ineluctable 時(shí)間: 2025-3-23 18:33
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作者: HEW 時(shí)間: 2025-3-24 01:11
,Pflanzenern?hrung 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 作者: 疾馳 時(shí)間: 2025-3-24 05:58
,Pflanzenern?hrung 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作者: acrimony 時(shí)間: 2025-3-24 10:18 作者: 花爭(zhēng)吵 時(shí)間: 2025-3-24 12:20 作者: 切割 時(shí)間: 2025-3-24 16:59 作者: Diverticulitis 時(shí)間: 2025-3-24 22:19 作者: Exclaim 時(shí)間: 2025-3-25 01:04 作者: 和平 時(shí)間: 2025-3-25 05:25
Forstliche Bodenkunde und Standortslehrervation. 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作者: Dri727 時(shí)間: 2025-3-25 09:49 作者: 謊言 時(shí)間: 2025-3-25 15:42 作者: SIT 時(shí)間: 2025-3-25 17:47
,Pflanzenern?hrung und Pflanzengifte,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作者: corpus-callosum 時(shí)間: 2025-3-25 22:03
,Pflanzenern?hrung und Pflanzengifte,We present a review on polarimetric properties of small Solar system bodies. The main results of polarimetric investigations of asteroids, comets, transneptunian objects and Centaurs are discussed focusing on recent findings. We also discuss the polarimetric observations of dust clouds in our Solar system.作者: BACLE 時(shí)間: 2025-3-26 02:15 作者: Fortify 時(shí)間: 2025-3-26 07:46
Roberto Mignani,Andrew Shearer,Silvia ZaneA state-of-the-art review of polarisation principles and astronomical instrumentation.Provides detailed background information suitable for graduate students.Reviews current and future instrumentation作者: SSRIS 時(shí)間: 2025-3-26 10:49
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/b/image/163603.jpg作者: ARBOR 時(shí)間: 2025-3-26 13:28
https://doi.org/10.1007/978-3-030-19715-5Multi-wavelength polarimetry; X-ray and gamma-ray polarization; Astronomical Instrumentation; Magnetic 作者: 平躺 時(shí)間: 2025-3-26 18:50
978-3-030-19717-9Springer Nature Switzerland AG 2019作者: crucial 時(shí)間: 2025-3-26 23:45 作者: 毛細(xì)血管 時(shí)間: 2025-3-27 02:51 作者: 金桌活畫(huà)面 時(shí)間: 2025-3-27 05:58 作者: 有罪 時(shí)間: 2025-3-27 11:04
0067-0057 imetric 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..978-3-030-19717-9978-3-030-19715-5Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 合乎習(xí)俗 時(shí)間: 2025-3-27 15:29 作者: vitreous-humor 時(shí)間: 2025-3-27 21:51 作者: 極肥胖 時(shí)間: 2025-3-28 01:01 作者: 不法行為 時(shí)間: 2025-3-28 06:02 作者: Notify 時(shí)間: 2025-3-28 07:55
Dust Polarisation in the Interstellar Medium,n the observing beam as compared to attempts at analysing averages of the observing characteristics over multiple-clouds. The propagation of polarised light through dust enshrouded objects is solved by polarisation radiative transfer for which we outline the central methodology.作者: extrovert 時(shí)間: 2025-3-28 12:57 作者: Efflorescent 時(shí)間: 2025-3-28 15:42 作者: 肉身 時(shí)間: 2025-3-28 20:26
Forstliche Bodenkunde und Standortslehreion throughout the solar atmosphere. This chapter presents an overview of the main sources of light polarisation in the Sun along with some recent investigations of the polarisation produced in the solar atmosphere.作者: Ischemia 時(shí)間: 2025-3-29 02:17
https://doi.org/10.1007/978-3-642-92144-5n the observing beam as compared to attempts at analysing averages of the observing characteristics over multiple-clouds. The propagation of polarised light through dust enshrouded objects is solved by polarisation radiative transfer for which we outline the central methodology.作者: HARD 時(shí)間: 2025-3-29 05:13 作者: Inflamed 時(shí)間: 2025-3-29 09:07
Book 2019ts 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作者: Electrolysis 時(shí)間: 2025-3-29 13:02 作者: Medicare 時(shí)間: 2025-3-29 18:55
,Pflanzenern?hrung und Pflanzengifte,ision-of-time polarimetry. Thorough calibration of a polarimeter should be carried out so that reliable and accurate measurements are obtained. In this chapter we describe a number of robust calibration methods that do not require any assumptions to be made about the system.作者: Cardioversion 時(shí)間: 2025-3-29 20:55 作者: ablate 時(shí)間: 2025-3-30 00:08
,Pflanzenern?hrung und Pflanzengifte,hought to be powered by thermal emission from the cooling neutron star surface, has detected optical polarisation. This chapter will review the current multi-wavelength polarisation observations and the theoretical modelling by which we can probe the pulsar magnetosphere structure and emission mechanisms.作者: 反感 時(shí)間: 2025-3-30 07:52
Forstliche Bodenkunde und Standortslehrenternational theoretical and observational effort. Polarisation is one of characteristics of synchrotron emission, and polarimetric observations would allow us to study the magnetic field structure and energy distribution in GRB jets.作者: expound 時(shí)間: 2025-3-30 10:14
When Polarimetry Made History,space telescope observations of polarised X-radiation in the 1970s; the viewing-angle unification scheme of active galactic nuclei since the 1980s; and the hunt for B-mode polarisation in the cosmic microwave background.作者: 寬大 時(shí)間: 2025-3-30 13:47
Introduction to Polarisation and Polarimetry,ision-of-time polarimetry. Thorough calibration of a polarimeter should be carried out so that reliable and accurate measurements are obtained. In this chapter we describe a number of robust calibration methods that do not require any assumptions to be made about the system.作者: 冥界三河 時(shí)間: 2025-3-30 17:38
Optical Polarimetry: Methods, Instruments and Calibration Techniques,ion of black hole X-ray binaries and massive binary stars made with our DiPol-2 polarimeter, which allowed us to constrain the sources of optical emission in black hole X-ray binaries and measure orbital parameters of massive stellar binaries.作者: 令人作嘔 時(shí)間: 2025-3-30 21:55
Multi-Wavelength Polarimetry of Isolated Pulsars,hought to be powered by thermal emission from the cooling neutron star surface, has detected optical polarisation. This chapter will review the current multi-wavelength polarisation observations and the theoretical modelling by which we can probe the pulsar magnetosphere structure and emission mechanisms.
