Aso-S Mission: Inflight Performance and First Results
暫譯: Aso-S 任務：飛行性能與初步結果
Gan, Weiqun, Leibacher, John, Mandrini, Cristina H.
- 出版商: Springer
- 出版日期: 2025-10-30
- 售價: $8,520
- 貴賓價: 9.5 折 $8,094
- 語言: 英文
- 頁數: 541
- 裝訂: Hardcover - also called cloth, retail trade, or trade
- ISBN: 9402423311
- ISBN-13: 9789402423310
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相關分類:
物理學 Physics
海外代購書籍(需單獨結帳)
相關主題
商品描述
The Advanced Space-based Solar Observatory (ASO-S) is China's first comprehensive mission dedicated to solar research. It was successfully launched on October 9, 2022. This book is a reprint of a collection of articles originally published in the journal of Solar Physics, comprising 30 papers that present the in-flight performance and early scientific results of ASO-S, with data collected up to March 15, 2024. Together, these papers provide an overview of the mission's progress during the first one and a half years after the launch. Earlier studies on the mission and its instruments, conducted prior to launch, can be found primarily in special issues of RAA (2019, Vol. 19, No. 11) and Acta Astronomica Sinica (2020, Vol. 61, No. 4). Additional related research has also appeared in journals such as ApJ, A&A, and MNRAS.
ASO-S aims to investigate the relationships between the solar magnetic field, solar flares, and coronal mass ejections (CMEs). It is equipped with three onboard instruments: the Full-disc vector MagnetoGraph (FMG), the Hard X-ray Imager (HXI), and the Lyman-alpha Solar Telescope (LST), which are designed to observe the solar magnetic field, solar flare hard X-ray emissions, and the formation and propagation of CMEs, respectively. The book is organized into four parts. Part One includes five papers detailing the mission's final technical configuration prior to launch, the first-light results, the in-flight performance and calibration of FMG, HXI, and LST, and the mission's data center. The remaining three parts are each devoted to scientific research based on observations from FMG, HXI, and LST, respectively.
Reprinted from Solar Physics, Topical Collection: ASO-S Mission: Inflight Performance and First Results.
商品描述(中文翻譯)
高級太空太陽觀測衛星（ASO-S）是中國首個專門針對太陽研究的綜合性任務。它於2022年10月9日成功發射。本書是對原刊登於《太陽物理學》期刊的一系列文章的重印，包含30篇論文，展示了ASO-S的在飛行性能和早期科學結果，數據收集截至2024年3月15日。這些論文共同提供了該任務在發射後一年半內的進展概述。關於該任務及其儀器的早期研究，主要可在《RAA》（2019年，第19卷，第11期）和《中國天文學報》（2020年，第61卷，第4期）的特刊中找到。其他相關研究也出現在《天體物理學雜誌》（ApJ）、《天文與天體物理學》（A&A）和《月刊天文學會》（MNRAS）等期刊中。
ASO-S旨在研究太陽磁場、太陽耀斑和日冕物質拋射（CME）之間的關係。它配備了三個在軌儀器：全盤向量磁圖儀（FMG）、硬X射線成像儀（HXI）和萊曼α太陽望遠鏡（LST），分別設計用於觀測太陽磁場、太陽耀斑的硬X射線輻射，以及CME的形成和傳播。本書分為四個部分。第一部分包括五篇論文，詳細介紹了發射前任務的最終技術配置、首次觀測結果、FMG、HXI和LST的在飛行性能和校準，以及任務的數據中心。其餘三部分則分別專注於基於FMG、HXI和LST觀測的科學研究。
重印自《太陽物理學》，專題集：ASO-S任務：在飛行性能和首次結果。
作者簡介
Dr. Weiqun Gan earned his PhD (1989) in the Department of Astronomy at Nanjing University. Following his education, he joined the Purple Mountain Observatory (PMO) of the Chinese Academy of Sciences (CAS) and was promoted to full professor in 1995. From 2004 to 2014, he served as Deputy Director of PMO. For many years, his research has focused on solar flares through modeling the atmosphere, hydrodynamics, spectroscopy, and high-energy solar physics. He has been actively involved in nearly every project aimed at advancing space-based solar observations in China. In 2011, he proposed the mission concept for ASO-S and led its pre-study from 2011 to 2013. From 2014 to 2016, he led the background development of the mission. In late 2017, ASO-S was formally established by CAS, with Gan appointed as the Chief Scientist for the mission. To date, he has authored/co-authored around 300 publications, including the monograph titled High Energy Solar Physics (2002, Science Press, in Chinese).
Dr. John Leibacher is a solar physicist, working primarily on atmospheric dynamics and helioseismology, who was previously at the National Solar Observatory (NSO), in Tucson, Arizona, USA for many years where he was director and director of the Global Oscillation Network Group (GONG), and he is currently at the Institut d'Astrophysique Spatiale, Université de Paris-Saclay, Orsay, France and the Lunar and Planetary Laboratory of the University of Arizona in Tucson, Arizona. He has been actively involved in a number of space missions. He served as Editor-in-Chief of the journal Solar Physics for 19 years and he previously served for a number of years on the Editorial Committee of the Annual Reviews of Astronomy and Astrophysics.
Dr. Cristina H. Mandrini is a Senior Researcher at the Instituto de Astronomía y Física del Espacio, Consejo Nacional de Investigaciones Científicas y Técnicas and Universidad de Buenos Aires, in Buenos Aires, Argentina. She has been the head of the Solar Physics Group in this institution for more than 20 years and Assistant and Associate Professor at the Universidad de Buenos Aires for 17 years. She is interested in solar active phenomena, their origin, magnetic field modelling, topology calculation, and their impact in the interplanetary medium. She is full member of the Academia Nacional de Ciencias Exactas, Físicas y Naturales since 2018, in which she is the present President of the Physics, Mathematics, and Astronomy Section, and a member of its Board of Directors, as well as full member of The World Academy of Sciences. She has been Editor in Chief of the journal Solar Physics since 2016.
Dr. Lidia van Driel-Gesztelyi is a solar physicist, working on the formation and evolution of solar active regions and their magnetic activity phenomena (e.g. flares and coronal mass ejections), magnetic helicity, coronal heating, elemental composition of the solar corona, and the origin of the solar wind. She is Emeritus Professor of Space and Climate Physics at University College London, UK, and Emeritus Researcher at Konkoly Observatory, Hungary. She has served in various leadership roles in the International Astronomical Union. She was awarded the Service Award of the Royal Astronomical Society, UK, Doctor Honoris Causa of Paris Observatory, France, and Order of Merit of Hungary. She has been Editor in Chief of the journal Solar Physics since 2005 and served for five years on the Editorial Committee of the Annual Reviews of Astronomy and Astrophysics.
作者簡介(中文翻譯)
甘維群博士於1989年在南京大學天文系獲得博士學位。完成學業後，他加入中國科學院紫金山天文台（PMO），並於1995年晉升為正教授。從2004年到2014年，他擔任PMO的副台長。多年來，他的研究專注於通過大氣建模、流體力學、光譜學和高能太陽物理學來研究太陽耀斑。他積極參與幾乎所有旨在推進中國太空太陽觀測的項目。2011年，他提出了ASO-S的任務概念，並於2011年至2013年領導其前期研究。從2014年到2016年，他負責該任務的背景開發。2017年底，ASO-S正式由中國科學院成立，甘博士被任命為該任務的首席科學家。至今，他已發表或共同發表約300篇論文，包括名為《高能太陽物理學》（2002年，科學出版社，中文）的專著。
約翰·萊巴赫博士是一位太陽物理學家，主要研究大氣動力學和日震學，曾在美國亞利桑那州圖森的國家太陽觀測站（NSO）工作多年，擔任該站的主任及全球振盪網絡小組（GONG）的主任，目前在法國巴黎薩克雷大學的太空天文學研究所及亞利桑那大學的月球與行星實驗室工作。他積極參與多個太空任務。曾擔任《Solar Physics》期刊的主編19年，並在《Annual Reviews of Astronomy and Astrophysics》的編輯委員會任職多年。
克里斯蒂娜·H·曼德里尼博士是阿根廷布宜諾斯艾利斯國立天文與空間物理研究所（Instituto de Astronomía y Física del Espacio）、國家科學技術研究委員會（Consejo Nacional de Investigaciones Científicas y Técnicas）及布宜諾斯艾利斯大學的高級研究員。她在該機構擔任太陽物理小組負責人已超過20年，並在布宜諾斯艾利斯大學擔任助理教授和副教授17年。她對太陽活動現象及其起源、磁場建模、拓撲計算及其對行星間介質的影響感興趣。自2018年以來，她是阿根廷國家科學、物理和自然科學學院的正式成員，並擔任物理、數學和天文學部門的現任主席及董事會成員，同時也是世界科學院的正式成員。自2016年以來，她一直擔任《Solar Physics》期刊的主編。
莉迪亞·范·德里爾-蓋斯特利博士是一位太陽物理學家，研究太陽活動區的形成和演化及其磁活動現象（例如耀斑和日冕物質拋射）、磁螺旋、日冕加熱、太陽日冕的元素組成及太陽風的起源。她是英國倫敦大學學院的太空與氣候物理名譽教授，以及匈牙利孔科利天文台的名譽研究員。她在國際天文聯合會擔任過多個領導職位。她曾獲得英國皇家天文學會的服務獎、法國巴黎天文台的榮譽博士學位及匈牙利的功勳勳章。自2005年以來，她一直擔任《Solar Physics》期刊的主編，並在《Annual Reviews of Astronomy and Astrophysics》的編輯委員會任職五年。
