The Hinode (Solar-B) mission:: An overview

The Hinode (Solar-B) mission:: An overview
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DOI:
10.1007/s11207-007-9014-6
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发表时间:
2007-06-01
期刊:
影响因子:
2.8
通讯作者:
Golub, L.
Golub, L.
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
Kosugi, T.;Matsuzaki, K.;Golub, L.

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2006年9月成功发射了日本宇宙航空研究开发机构空间和宇宙航行科学研究所(ISAS/JAXA)的Hinode卫星(原Solar-B)。作为Yohkoh使命的后继者,它旨在了解磁能如何从光球层转移到高层大气,并导致爆炸性能量释放。Hinode是一个天文台式的使命,所有的仪器都是为了共同努力实现科学目标而设计和建造的。船上有三个仪器:太阳光学望远镜(SOT),EUV成像光谱仪(EIS)和X射线望远镜(XRT)。本文概述了该使命,详细介绍了卫星、科学有效载荷和操作。最后将讨论国际科学界如何参与使命数据的分析。
The Hinode satellite (formerly Solar-B) of the Japan Aerospace Exploration Agency's Institute of Space and Astronautical Science (ISAS/JAXA) was successfully launched in September 2006. As the successor to the Yohkoh mission, it aims to understand how magnetic energy gets transferred from the photosphere to the upper atmosphere and results in explosive energy releases. Hinode is an observatory style mission, with all the instruments being designed and built to work together to address the science aims. There are three instruments onboard: the Solar Optical Telescope (SOT), the EUV Imaging Spectrometer (EIS), and the X-Ray Telescope (XRT). This paper provides an overview of the mission, detailing the satellite, the scientific payload, and operations. It will conclude with discussions on how the international science community can participate in the analysis of the mission data.