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第23至24周太阳质子事件的统计特征

白铁男 乐贵明 赵浩峰

空间科学学报2017,Vol.37Issue(6):649-658,10.
空间科学学报2017,Vol.37Issue(6):649-658,10.DOI:10.11728/cjss2017.06.649

第23至24周太阳质子事件的统计特征

Statistical Properties of Solar Proton Events during Solar Cycle 23 and 24

白铁男 1乐贵明 2赵浩峰3

作者信息

  • 1. 南京信息工程大学数学与统计学院 南京210044
  • 2. 中国气象局空间天气重点开放实验室 北京100081
  • 3. 国家空间天气监测预警中心 北京100081
  • 折叠

摘要

Abstract

There were totally 128 Solar Proton Events (SPEs) from 1997 to 2016.Their peak flux ranges are from 10pfu to 99pfu,100 to 999pfu,1000 to 2999pfu and greater than 3000pfu,and the percentage is 55.15%,27.94%,9.56% and 7.35% respectively.The results show that SPEs with different peak flux have different asymmetry.The SPEs with peak flux ranged from 1000pfu to 2999 pfu have the largest asymmetry,while those with peak flux greater than 3000 pfu have smallest asymmetry.In Solar Cycle 23,the SPEs mainly occurred during the period from the first peak to the second peak and after the second peak of the smoothed monthly mean sunspot numbers.In Solar Cycle 24,the SPEs mainly occurred during the period before maximum of smoothed monthly mean sunspot numbers.

关键词

太阳黑子/质子事件/不对称性/太阳活动周

Key words

Sunspots/Proton events/Asymmetry/Solar activity cycle

分类

天文与地球科学

引用本文复制引用

白铁男,乐贵明,赵浩峰..第23至24周太阳质子事件的统计特征[J].空间科学学报,2017,37(6):649-658,10.

基金项目

国家自然科学基金项目(41074132,41274193,41474166)和质检总局行业专项(200710123)共同资助 (41074132,41274193,41474166)

空间科学学报

OA北大核心CSCDCSTPCD

0254-6124

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