期刊文献+

日面高纬黑子与太阳活动 被引量:4

SUNSPOTS AT HIGH LATITUDES AND SOLAR ACTIVITY
下载PDF
导出
摘要 利用云南天文台太阳黑子观测资料,对太阳活动第19 周至第22 周日面高纬度( 高于40°) 的黑子群进行了统计.结果表明:高纬黑子面积绝大部分小于100 ,平均56 ,寿命大部分为1 ~3 天,平均4 天;黑子分类绝大部分为AXX、HSX、BXO,其中AXX 约占总数的一半.高纬黑子在日面南北半球上的不对称分布可用来预报该太阳周内的太阳活动在南北半球上的主次.由此预报23 Based on the data of the sunspots observed at Yunnan Observatory, the sunspot groups at high latitudes (over 40°) during the solar cycles 19,20,21, and 22, and the rising period of the solar cycle 23 have been collected statistically in this paper. The results show that for most of the sunspots at high latitudes, the sunspot classes are AXX, BXO or HSX, the areas are less than 100, the lifetimes are 1 to 3 days, and the relation between lifetime and the maximum area is T=0.07×A. If sunspots at high latitides are found to dominate in one hemisphere (the northern or southern) in a solar cycle, then we can predict that solar activities will dominate in this hemisphere for the entire cycle. According to this finding, the dominance of solar activity in the southern hemisphere will continue during the coming cycle 23.
出处 《天文学报》 CSCD 北大核心 1999年第4期435-438,共4页 Acta Astronomica Sinica
关键词 太阳活动 黑子 日面高纬 黑子分类 Sun, solar activity, sunspots
  • 相关文献

参考文献2

  • 1章振大,太阳物理学,1992年,227页
  • 2张元东,太阳黑子,1989年,5368页

同被引文献27

  • 1孙小青,叶宗海.由环电流的宇宙线效应验证二维对称环电流模型[J].空间科学学报,1993,13(2):140-145. 被引量:1
  • 2郭维吉,章公亮.强磁场扰动对宇宙线调制的统计研究[J].空间科学学报,1995,15(4):295-300. 被引量:4
  • 3多尔曼 朱岗昆(译).宇宙线强度变化[M].北京:科学出版社,1965..
  • 4普雷斯 王璞(译).数值方法大全——科学计算的艺术[M].兰州大学出版社,1991..
  • 5Newton H W, Milson A S. Distribution of sunspot areas. Monthly Not. Roy. Astron. Soc., 1995,115:398---413
  • 6Carbonell M, Oliver R, Ballester J C. On the asymmetry of solar activity. Astron. Astrophvs., 1993,274:497--504
  • 7Atac T, Ozguc A. Time variation of flare index during the 21st solar cycle. Astrophys Sapce Sci., 1987,i12:341--346
  • 8Atac T, Ozguc A. North-south asymmetry in the solar flare index 1996. Solar Phys., 166:201--208
  • 9Oliver R, ballester J L. The N-S asymmetry in of sunspot areas during solar cycle 22. Solar Phys.,1994, 152:481--485
  • 10Howard A G. Evidence for solar-cycle evolution of N-S flare asymmetry during cycles 20 and 21. SolarPhys., 1990, 127:185--197

引证文献4

二级引证文献10

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部