首页> 外文会议>International Cosmic Ray Conference >Geoeffectiveness of Halo CMEs during different phases of solar activity cycle 23
【24h】

Geoeffectiveness of Halo CMEs during different phases of solar activity cycle 23

机译:晕圈CMES在太阳能循环循环的不同阶段的Geoeffective

获取原文

摘要

We studied the geoeffectiveness of a set of 397 halo CMEs during the ascending, maximum and descendi descending phases of ng solar cycle 23. In this study minimum Dst values occurring within 1 1-5 days after the CME onset are compiled. The distribution of such Dst values are compared for the following categ categories of halo CMEs disk halos limb halos and backside halo CMEs. We defined ries that these halo CMEs are geoeffective if it is followed by Dst 凾 -50 nT, mode moderately geoeffective if ately -50n < Dst < -100 nT, and strongly geoeffective if Dst 凾 -100 nT. We find that Disk halos are followed by strong storms, limb halos are followed by moderately storms and backside halos are about near to moderate storms. The Frontside halos (Disk +F F-limb) are most geoeff geoeffective (~71%). ective Intense storms are o occurred in maximum phase of solar cycle and the few are occurred in declining phase. Most intense storms occur, curred when there are successive CMEs and occurred near the disk center towards western hem hemisphere. The long term pr sphere. profile of Dst index is ofile positively related with CME occurrence rate. Most of the geoeffective halos are confined between the maximum and descending phases. The delay time between CME onset and minimum Dst values is the smallest for Limb halos. Most of the g geoma eomagnetic storms netic are occurred between 48 hours to 72 hours after CME onset.
机译:在NG太阳循环23的上升,最大和Descendi下降期间,我们研究了一组397晕CME的地质切口。在编译CME发作后1-5天内发生的最小DST值。将这种DST值的分布进行了比较,以完成以下几类Halo CMES盘晕晕光环和背面光晕CMES。我们定义了这些光环CME是Geoeffective的原因,如果它是DST凾-50NT,则在适度的地质接近,如果ILF-50N

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号