天文学光学性3D光谱学 Optical 3D-Spectroscopy For Astronomy

基本信息

by R Bacon (Author)

Format:Hardback 296 pages

Publisher:Wiley-VCH Verlag GmbH

Imprint:Wiley-VCH Verlag GmbH

ISBN:9783527412020

Published:12 Apr 2017

Weight:788g

Dimensions:178 x 251 x 19 (mm)

页面数据仅供参考，具体以实物为准

书籍简介

在过去的50年里，人们开发了各种技术来为常规成像增加第三维度，在每个成像像素上都有一个扩展光谱。从其数据格式来看，它被称为三维光谱学，现在被广泛用于天体物理学领域，但也特别用于大气科学和遥感目的。这是一本处理这些新功能的书。它首先介绍了光谱仪器的基本原理，特别是它们的潜力和局限。然后，它回顾了各种已知的三维技术，特别强调指出它们不同的 "生态 "位置。本书将引导用户了解整个观测过程，从观测计划到广泛而关键的数据还原阶段。本书的总体目标是为非专业人员提供足够的实践知识，使他们在使用这种三维能力时能够快速学会如何正确使用和产生有意义的数据。

Over the last 50 years, a variety of techniques have been developed to add a third dimension to regular imaging, with an extended spectrum associated to every imaging pixel. Dubbed 3D spectroscopy from its data format, it is now widely used in the astrophysical domain, but also inter alia for atmospheric sciences and remote sensing purposes. This is the first book to comprehensively tackle these new capabilities. It starts with the fundamentals of spectroscopic instruments, in particular their potentials and limits. It then reviews the various known 3D techniques, with particular emphasis on pinpointing their different 'ecological? niches. Putative users are finally led through the whole observing process, from observation planning to the extensive ? and crucial - phase of data reduction. This book overall goal is to give the non-specialist enough hands-on knowledge to learn fast how to properly use and produce meaningful data when using such a 3D capability.

作者简介

罗兰-培根是天体物理学家，国家科学研究中心的研究主任和里昂天文台的前主任（1994-2004）。他作为地面望远镜的4个主要和创新仪器，在整体场光谱学的发展中发挥了先锋作用。在3.6米加拿大法国夏威夷望远镜的TIGER和OASIS，4.2米威廉赫歇尔望远镜的SAURON和8米欧空局甚大望远镜的MUSE。他的主要研究领域是银河系外天文学。自2014年起，他是欧洲研究委员会高级拨款的拥有者。盖伊-莫内是一位天体物理学家，在开发地面和太空的天文仪器方面有50年的经验，主要是3D光谱方面的经验。他先后担任马赛天文台、里昂天文台和加拿大法国夏威夷望远镜公司的主任。随后，他在欧洲南方天文台（1995-2009年）和澳大利亚天体物理观测站（2010-2011年）担任仪器主管一职。他的主要科学领域是星系中的恒星和电离气体的动力学。

Roland Bacon is astrophysicist, directeur de recherche au CNRS and former director of the Lyon Observatory (1994-2004). He has played a pioneering role in the development of integral field spectroscopy as leader of 4 major and innovative instruments for ground based telescope: TIGER and OASIS at the 3.6m Canada France Hawaii telescope, SAURON at the 4.2m William Herschel telescope and MUSE at the 8m ESO Very Large Telescope. His main research field is extragalactic astronomy. He is the owner since 2014 of an advanced grant from the European Research Commission. Guy Monnet is an astrophysicist, with 50-year experience of developing astronomical instrumentation, on the ground and in space, mostly with a 3D spectroscopic flavor. Successively, he was director of the Marseilles Observatory, Lyon Observatory and the Canada France Hawaii Telescope Corporation. He then took the position of Head of Instrumentation at the European Southern Observatory (1995-2009) and the Australian Astrophysical Observatory (2010-2011). His main scientific domain is the dynamics of stars and ionized gas in galaxies.