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双通道辐射量计算太阳极紫外辐射E10.7指数方法初探

范磊 韦飞 符养 赵伟 费增坪

范磊, 韦飞, 符养, 赵伟, 费增坪. 双通道辐射量计算太阳极紫外辐射E10.7指数方法初探[J]. 空间科学学报, 2013, 33(4): 403-409. doi: 10.11728/cjss2013.04.403
引用本文: 范磊, 韦飞, 符养, 赵伟, 费增坪. 双通道辐射量计算太阳极紫外辐射E10.7指数方法初探[J]. 空间科学学报, 2013, 33(4): 403-409. doi: 10.11728/cjss2013.04.403
FAN Lei, WEI Fei, FU Yang, ZHAO Wei, FEI Zengping. Use Double Channel Solar Irradiance Flux to Compute the E10.7 Index[J]. Chinese Journal of Space Science, 2013, 33(4): 403-409. doi: 10.11728/cjss2013.04.403
Citation: FAN Lei, WEI Fei, FU Yang, ZHAO Wei, FEI Zengping. Use Double Channel Solar Irradiance Flux to Compute the E10.7 Index[J]. Chinese Journal of Space Science, 2013, 33(4): 403-409. doi: 10.11728/cjss2013.04.403

双通道辐射量计算太阳极紫外辐射E10.7指数方法初探

doi: 10.11728/cjss2013.04.403
基金项目: 国家自然科学基金项目资助(40574081)
详细信息
    作者简介:

    范磊, fanlei_zc@163.com

  • 中图分类号: P352

Use Double Channel Solar Irradiance Flux to Compute the E10.7 Index

  • 摘要: 从太阳极紫外辐射研究的重要性出发, 介绍了太阳极紫外辐射E10.7指 数及其作用, 详细阐述了利用两个能道的太阳辐射观测值计算极紫外辐射E10.7指数的计算方法. 利用该方法对实测太阳辐射数据进行处理, 计算获得了2000-2005年的每日E10.7指数, 并将计算结果 与Solar2000模式的输出结果进行对比分析, 验证了该计算方法的可行性, 对比结果表明, 最大相对误差在20%以内, 平均相对误差均在10%以内.

     

  • [1] Paul Withers, Michael Mendillo. Response of peak electron densities in the martian ionosphere to day-to-day changes in solar flux due to solar rotation[J]. Planet. Space Sci., 2005, 53:1401-1418
    [2] Allen J H, Wilkinson D C. Solar-terrestrial activity affecting systems in space and on Earth[J]. Solar Terr. Pred., 1993, IV:75-107
    [3] Pardini C, Tobiska W K, Anselmo L. Analysis of the orbital decay of spherical satellites using different solar flux proxies and atmospheric density models[J]. Adv. Space Res., 2006, 37:392-400
    [4] Li Baoquan, Zhu Guangwu, Wang Shijin, et al. The solar X-EUV imaging telescope[J]. Chin. J. Geophys., 2005, 48(2):235-242. In Chinese (李保权, 朱光武, 王世金, 等. 太 阳X-EUV成像望远镜. 地球物理学报, 2005, 48(2):235-242)
    [5] Peng Jilong, Zhu Guangwu, Wei Fei, et al. Solar Extreme Ultraviolet Multichannel Imager[J]. Chin. J. Space Sci., 2009, 29(4):417-421). In Chinese (彭吉龙, 朱光武, 韦飞, 等. 太阳极紫外多波段成像仪[J]. 空间科学学报, 2009, 29(4):417-421)
    [6] Miao Juan, Liu Siqing, Xue Bingsen, et al. Primary research on prediction method of 10.7cm solar radio flux[J]. Chin. J. Space Sci., 2003, 23(1):50-54. In Chinese (苗娟, 刘四清, 薛炳森, 等. 太阳10.7cm射电辐射流量预报方法初探[J]. 空间科学学报, 2003, 23(1):50-54)
    [7] Liao Hairen, Wang Jingsong. Modification and application of E10.7 index in the band of soft X-ray[J]. Chin. J. Space Sci., 2006, 26(2):98-103
    [8] Tobiska W K. Validating the Solar EUV Proxy E10.7[J]. J. Geophys. Res., 2001, 106(A12):29969-29978
    [9] Tobiska W K, Woods Tom. The SOLAR2000 empirical solar irradiance model and forecast tool[J]. Atm. Solar Terr. Phys., 2000, 62:1233-1250
    [10] Tobiska W K, Bouwer S D. New developments in SOLAR2000 for space research and operations[J]. Adv. Space Res., 2006, 37:347-358
    [11] TobiskaW K. SOLAR2000 irradiances for climate change research, aeronomy and space system engineering[J]. Adv. Space Res., 2004, 34:1736-1746
    [12] Modolo R, Chanteur G M, Dubinin E, Matthews A P. Influence of the solar EUV flux on the Martian plasma environment[J]. Ann. Geophys., 2005, 23:1-12
    [13] Fox J L, Zhou P, Bougher S W. The Martian thermosphere/ionosphere at high and low solar activity[J]. Adv. Space Res., 1996, 17(11):203-218
    [14] Tobiska W K. Measurement and modeling of solar EUV/UV radiation[J]. Phys. Chem. Earth, 2000, 25(5-6):371-374
    [15] Stanley C. Solomon, Scott M. Bailey, Thomas N Woods. Effect of solar soft X-rays on the lower ionosphere[J]. Geophys. Res. Lett., 2001, 28(11):2149-2152
    [16] TobiskaW K. Validating the solar EUV proxy E10.7[J]. J. Geophys. Res., 2001, 106(A12):29969-29978
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出版历程
  • 收稿日期:  2012-05-17
  • 修回日期:  2013-03-13
  • 刊出日期:  2013-07-15

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