Erratum to “The Alpha Magnetic Spectrometer (AMS) on the International Space Station: Part I—results from the test flight on the space shuttle” [Physics Reports 366 (2002) 331–405]

Erratum to “The Alpha Magnetic Spectrometer (AMS) on the International Space Station: Part I—results from the test flight on the space shuttle” [Physics Reports 366 (2002) 331–405]
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“国际空间站上的阿尔法磁谱仪 (AMS):第一部分——航天飞机试飞结果”的勘误 [Physics Reports 366 (2002) 331–405]

DOI:
10.1016/s0370-1573(03)00138-8
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发表时间:
2003
期刊:
Physics Reports
影响因子:
--
通讯作者:
J. Allaby
J. Allaby
中科院分区:
--
文献类型:
--
作者:
J. Allaby

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第一次AMS使命的成功归功于许多个人和组织。NASA和美国能源部的支持对实验的启动、发展和运行至关重要。丹尼尔·S.当时的NASA局长戈尔丁对此表示感谢。美国能源部的John奥法伦博士、Peter罗森博士和PK威廉姆斯博士以及道格拉斯P.布兰查德博士、Mark J. Sistilli先生、James R.贝茨,肯尼思博尔韦格先生和美国宇航局和洛克希德马丁公司使命管理团队表示感谢。由于得到了马克斯-普朗克地外物理研究所的支持,得到了德国(德国航天中心)、意大利(意大利航天局)、法国(法国国家空间研究中心)、西班牙(中国空间技术研究所)和中国(中国空间技术研究院)等航天机构的支持,以及台湾科学技术研究中心的支持,才得以按时完成这项实验。在CERN和GSI达姆施塔特的支持下,特别是Hans Specht教授和Reinhard Simon博士的支持下,我们得以在航天飞机从轨道返回后校准探测器。意大利的INFN、法国的IN 2 P3、西班牙的CIEMAT和CICYT、葡萄牙的LIP、韩国的CHEP、中国科学院、台湾的中央研究院、麻省理工学院、苏黎世联邦理工学院、日内瓦大学、台湾国立中央大学、亚琛工业大学
The success of the first AMS mission is due to many individuals and organizations. The support of NASA and the US Department of Energy was vital to the inception, development and operation of the experiment. The interest and support of Mr. Daniel S. Goldin, then NASA Administrator, is gratefully acknowledged. The dedication of Dr. John O’Fallon, Dr. Peter Rosen and Dr. PK Williams of US DOE, as well as of Dr. Douglas P. Blanchard, Mr. Mark J. Sistilli, Mr. James R. Bates, Mr. Kenneth Bollweg and the NASA and Lockheed-Martin Mission Management team is acknowledged. The support of the Max-Planck Institute for Extraterrestrial Physics, the support of the space agencies from Germany (DLR), Italy (ASI), France (CNES), Spain (CDTI) and China (CALT) and the support of CSIST, Taiwan, made it possible to complete this experiment on time. The support of CERN and GSI-Darmstadt, particularly of Professor Hans Specht and Dr. Reinhard Simon made it possible for us to calibrate the detector after the shuttle returned from orbit. The support of INFN of Italy, IN2P3 of France, CIEMAT and CICYT of Spain, LIP of Portugal, CHEP of Korea, the Chinese Academy of Sciences, Academia Sinica of Taiwan, MIT, ETH-Z urich, the University of Geneva, National Central University of Taiwan, the RWTH-Aachen