留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码

中法天文卫星(SVOM)伽玛暴联合探测任务

余舜京 GONZALEZ François 魏建彦 张双南 CORDIER Bertrand

余舜京, GONZALEZ François, 魏建彦, 张双南, CORDIER Bertrand. 中法天文卫星(SVOM)伽玛暴联合探测任务[J]. 空间科学学报, 2019, 39(6): 800-808. doi: 10.11728/cjss2019.06.800
引用本文: 余舜京, GONZALEZ François, 魏建彦, 张双南, CORDIER Bertrand. 中法天文卫星(SVOM)伽玛暴联合探测任务[J]. 空间科学学报, 2019, 39(6): 800-808. doi: 10.11728/cjss2019.06.800
YU Shunjing, GONZALEZ Francois, WEI Jianyan, ZHANG Shuangnan, CORDIER Bertrand. SVOM: a Joint Gamma-ray Burst Detection Mission[J]. Journal of Space Science, 2019, 39(6): 800-808. doi: 10.11728/cjss2019.06.800
Citation: YU Shunjing, GONZALEZ Francois, WEI Jianyan, ZHANG Shuangnan, CORDIER Bertrand. SVOM: a Joint Gamma-ray Burst Detection Mission[J]. Journal of Space Science, 2019, 39(6): 800-808. doi: 10.11728/cjss2019.06.800

中法天文卫星(SVOM)伽玛暴联合探测任务

doi: 10.11728/cjss2019.06.800
基金项目: 

国家重点基础研究发展计划项目(2014CB845800)和国家民用航天专项共同资助

详细信息
    作者简介:

    余舜京,E-mail:yusj@microsate.com

  • 中图分类号: P171

SVOM: a Joint Gamma-ray Burst Detection Mission

  • 摘要: 中法天文卫星SVOM是中法两国合作的伽玛暴探测任务,由中国国家航天局(CNSA)和法国国家空间研究中心(CNES)批准立项,中国科学院负责总体研制.SVOM是继美国SWIFT任务之后最重要的伽玛暴多波段探测项目,是一颗功能强大的天文卫星,具有多波段观测、快速机动、灵活操作及地面后随观测能力.SVOM将开创一个非常广阔的探测领域.本文介绍了项目组织、任务目标、卫星和有效载荷、地面段以及运控概念.

     

  • [1] WEI J Y, CORDIER B, ANTIER S, et al. The deep and transient universe:new challenges and opportunities-scientific prospects of the SVOM mission[OL]. arXiv:1610.06892[astro-ph.IM],[2016-10-21]. https://lanl.arxiv.org/
    [2] WEI J Y, CORDIER B, ANTIER S, et al. The SVOM Gamma-ray Burst Mission[OL]. arXiv:1512.03323[astro-ph.IM],[2015-12-10], https://lanl.arxiv.org/
    [3] PAUL J, WEI J Y, BASE S, et al. The Chinese-French SVOM mission for gamma-ray burst studies[J]. Compt. Rendus Phys., 2011, 12(3):298-308
    [4] KLEBESADEL R W, STRONG I B, OLSON R A. Observations of gamma-ray burst of cosmic origin[J]. Astrophys. J., 1973, 182:85
    [5] FRAIL D A, KULKARNI S R, SARI R, et al. Beaming in gamma-ray bursts:evidence for a standard energy reservoir[J]. Astrophys. J., 2001, 562:55-58
    [6] REES M J, MESZAROS P. Relativistic fireballs:energy conversion and time-scales[J]. Mon. Not. R. Astron. Soc., 1992, 258(1):41-43
    [7] PIRAN T. Gamma-ray bursts and the fireball model[J]. Phys. Rep., 1999, 314(6):575-667
    [8] WEI Jianyan. SVOM has been approved by CNSA[J]. Chin. Natl. Astron., 2011, 6:40-41(魏建彦. SVOM天文卫星通过国家立项[J]. 中国国家天文, 2011, 6:40-41)
    [9] LACOMBE K, DEZALAY J P, HOURET B, et al. Spectral performance of ECLAIRs flight detectors on SVOM mission[J]. Astrop. Phys., 2018, 103:131-141
    [10] GODET O, PAUL J, WEI J Y, et al. The Chinese-French SVOM mission:studying the brightest astronomical explosions[C]//Proceeding SPIE 8443, Space Telescopes and Instrumentation 2012:Ultraviolet to Gamma Ray, 2012
    [11] PAUL J, WEI J Y, BASA S, et al. The Chinese-French SVOM mission for gamma-ray burst studies[J]. C R Phys., 2011(12):298-308
    [12] MERCIER K, GONZALEZ F,JOURET M, et al. The French payload on-board the SVOM French-Chinese mission[C]//Proceeding SPIE 9144, Space Telescopes and Instrumentation, Ultraviolet to Gamma Ray, 2014
    [13] WAN M, WU C, WANG J, et al. Column Store for GWAC:a high-cadence, high-density, large-scale astronomical light curve pipeline and distributed shared-nothing database[J]. Pub. Astron. Soc. Pacific, 2016, 128(969):114501
    [14] GONZALEZ F, YU S J. A French/Chinese cooperation for a Gamma-Ray burst mission[C]//Proc. SPIE 10699, Space Telescopes and Instrumentation, Ultraviolet to Gamma Ray, 2018
    [15] ZHAO Tonghua. Research on the Performance of SVOM Satellite High Energy Scientific Payload[D]. Beijing:Institute of High Energy, Chinese Academy of Sciences, 2012(赵佟华, SVOM卫星高能科学载荷性能研究[D]. 北京:中国科学院高能物理研究所, 2012)
    [16] MERCIER K, GONZALEZ F,JOURET M, et al. The French payload on-board the SVOM French-Chinese mission[C]//Proceeding SPIE 9144, Space Telescopes and Instrumentation, Ultraviolet to Gamma Ray, 2014
    [17] WU C, QIU Y L, CAI H B. SVOM Visible telescope:performance and data process scheme[J]. Proc. IAU Symp., 2013(279):421-422
  • 加载中
计量
  • 文章访问数:  1312
  • HTML全文浏览量:  15
  • PDF下载量:  177
  • 被引次数: 0
出版历程
  • 收稿日期:  2018-07-02
  • 修回日期:  2019-02-18
  • 刊出日期:  2019-11-15

目录

    /

    返回文章
    返回