What Can We Learn from the Geoeffectiveness of the Magnetic Cloud on 2012 July 15–17?  

作　　者：Gui-Ang Liu Ming-Xian Zhao Gui-Ming Le Tian Mao 

机构地区：[1]School of Physics Science and Technology,Lingnan Normal University,Zhanjiang 524048,China [2]Key Laboratory of Solar Activity,National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China [3]Key Laboratory of Space Weather,National Center for Space Weather,China Meteorological Administration,Beijing,100081,China

出　　处：《Research in Astronomy and Astrophysics》2022年第1期14-18,共5页天文和天体物理学研究（英文版）

基　　金：supported by Sino-South Africa Joint Research on Polar Space Environment (2021YFE0106400);International Cooperation Project on Scientific and Technological Innovation Between Governments;National Key Plans on Research and Development,Ministry of Science and Technology,China;CAS Key Laboratory of Solar Activity under number KLSA (grant No.KLSA202109);the National Natural Science Foundation of China (grant Nos.41074132,41274193,41474166,41774195 and 41874187)。

摘　　要：An interplanetary shock and a magnetic cloud(MC) reached the Earth on 2012 July 14 and 15 one after another.The shock sheath and the MC triggered an intense geomagnetic storm.We find that only small part of the MC from06:45 UT to 10:05 UT on 2012 July 15 made contribution to the intense geomagnetic storm,while the rest part of the MC made no contribution to the intense geomagnetic storm.The averaged southward component of interplanetary magnetic field(Bs) and duskward-electric fields(Ey) within the MC from 10:05 UT,2012 July 15 to09:08 UT,2012 July 16(hereafter MC2),are 15.11 nT and 8.01 my m-1,respectively.According to the empirical formula established by Burton et al.(hereafter Burton equation),the geoeffectiveness of MC2 should be-655.42 nT,while the geoeffectiveness of MC2 is-324.68 nT according to the empirical formula established by O’Brien & McPherron(hereafter OM equation).However,the real geoeffectiveness of MC2 is 39.74 nT.The results indicate that the Burton equation and the OM equation cannot work effectively.The geoeffectiveness of MC2 shows that large and long duration of Bs or Ey cannot guarantee the occurrence of an intense geomagnetic storm if the solar wind dynamic pressure is very low.If we use 0.52 as γ,the geoeffectiveness of MC2 is 40.36 nT according to the empirical formula established by Wang et al.,which is very close to the observed value,indicating that the empirical formula established by Wang et al.is much better than the Burton equation and the OM equation.

关 键 词：Solar coronal mass ejections Solar-terrestrial interactions Solar wind 

分 类 号：P182[天文地球—天文学] P353