Volume 41 Issue 5
Sep.  2021
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SUN Xiaoying, DUAN Suping, LIU Weining. Correlation Analysis between Magnetic Storms and Solar Extreme Ultraviolet Radiation during the 23rd Solar Cycle[J]. Chinese Journal of Space Science, 2021, 41(5): 697-703. doi: 10.11728/cjss2021.05.697
Citation: SUN Xiaoying, DUAN Suping, LIU Weining. Correlation Analysis between Magnetic Storms and Solar Extreme Ultraviolet Radiation during the 23rd Solar Cycle[J]. Chinese Journal of Space Science, 2021, 41(5): 697-703. doi: 10.11728/cjss2021.05.697
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Correlation Analysis between Magnetic Storms and Solar Extreme Ultraviolet Radiation during the 23rd Solar Cycle

doi: 10.11728/cjss2021.05.697 cstr: 32142.14.cjss2021.05.697

  • 1. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190;

  • 2. University of Chinese Academy of Sciences, Beijing 100049

  • Received Date: 2020-04-29
  • Rev Recd Date: 2020-12-11
  • Publish Date: 2021-09-15
    Abstract
  • The statistics of magnetic storms with moderate and higher intensity during the 23rd solar cycle are presented, and investigated the correlation by linear analysis between the intensity of the magnetic storm Dstmin and the solar Extreme Ultraviolet Radiation (EUV) intensity by using the observation of F10.7 index before the maximum of the storm main phase. Our statistical analysis results show that during the 23rd solar cycle:firstly, with an increase in solar EUV input, the number of moderate or higher intensity storms increases. There are 56 moderate or higher intensity storms under low solar extreme ultraviolet radiation activity, 85 storms under intermediate solar extreme ultraviolet radiation activity, and 80 events under high solar extreme ultraviolet radiation activity. Secondly, with increasing EUV input, the number and the probability of strong (-200nT ≤ Dstmin<-100nT) and big (Dstmin< -200nT) storms occurring also show an increasing trend, especially the number (1, 4, 12) and the probability (1.79%, 4.76%, 14.12%) of big storms. Thirdly, there is a moderate positive correlation of big storm (|Dstmin|) with F10.7, where the correlation coefficient is 0.532, and the correlation of big storm (|Dstmin|) with F10.7 is more significantly under high solar extreme ultraviolet radiation activity, where the coefficient is 0.582. Our results that there exists the moderate positive correlation of big storm with high solar extreme ultraviolet radiation activity can provide foundation information for space weather forecasting.

     

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