期刊文献+
共找到6篇文章
< 1 >
每页显示 20 50 100
1997年1月7—10日广州台站银河宇宙线强度变化特征 被引量:2
1
作者 乐贵明 叶宗海 +3 位作者 余绍华 李润森 肖少瑜 龚菊红 《空间科学学报》 CAS CSCD 北大核心 2002年第4期309-313,共5页
1997年1月7—10日的CME事件虽然只引起了中等强度的磁暴,但引起了很强的地球物理效应.这次CME事件影响了银河宇宙线的强度.本文给出了CME在行星际传播期间广州多方向闪烁望远镜观测台站在几个方向记录的银河宇宙线强度变化的特征,并做... 1997年1月7—10日的CME事件虽然只引起了中等强度的磁暴,但引起了很强的地球物理效应.这次CME事件影响了银河宇宙线的强度.本文给出了CME在行星际传播期间广州多方向闪烁望远镜观测台站在几个方向记录的银河宇宙线强度变化的特征,并做了简要的分析. 展开更多
关键词 1997年 强度 CME 银河宇宙线 各向异性 地磁暴 日冕物质抛射 天气预报
下载PDF
Variations in Solar Cycles 22, 23 &24 and Their Effect on Earth’s Climate 被引量:1
2
作者 Prithvi Raj Singh Chandra Mani Tiwari Ajay Kumar Saxena 《International Journal of Astronomy and Astrophysics》 2016年第1期8-13,共6页
In the present work, the study of influence of solar activity, cosmic ray intensity and geomagnetic activity on Earth’s climate during solar cycles 22, 23 and 24 has been done. The change in Earth’s climate, specifi... In the present work, the study of influence of solar activity, cosmic ray intensity and geomagnetic activity on Earth’s climate during solar cycles 22, 23 and 24 has been done. The change in Earth’s climate, specifically the change in the global mean temperature has been associated with the variation of some solar activity indices, cosmic ray intensity and geomagnetic activity indices in the period of 1986-2014 (Till Dec.). The important solar indices that are total solar irradiance (TSI), Sunspot Number (SSN), F10.7 index, Cosmic Ray Intensity (CRI) Kiel (NM), geomagnetic activity indices Auroral Electrojet Index (AE) and aa index, have been presented. The study of the Earth’s climate in relationship with solar activity, cosmic ray intensity and geomagnetic activity has been analysed with variations and correlations. The variations of SSN with CRI are in anti-phase;SSN with F10.7, SSN with TSI, SSN with AE, SSN with aa are in same phase. The correlation of SSN with CRI is strongly negatively correlated;SSN with F10.7, SSN with TSI is strongly positively and SSN with AE, SSN with aa positively correlated to averaging solar cycles 22, 23 and 24. The Earth’s climate will be affected by the solar activity, cosmic ray intensity and geomagnetic activity. 展开更多
关键词 Solar Activity Geomagnetic Activity cosmic ray intensity
下载PDF
地磁暴前地面宇宙线强度变化Morlet小波特征分析 被引量:1
3
作者 苗娟 薛炳森 叶宗海 《空间科学学报》 CAS CSCD 北大核心 2003年第6期452-458,共7页
用Morlet小波变换对Oulu台站和Apatity台站(主要是Apatity台站)1998-2002年间宇宙线静日和地磁暴前的地面宇宙线强度变化特征进行分析,得到:在宇宙线静日期间普遍存在准24 h周期变化特征,并且在当地时间0200,1400左右分别出现最小值和... 用Morlet小波变换对Oulu台站和Apatity台站(主要是Apatity台站)1998-2002年间宇宙线静日和地磁暴前的地面宇宙线强度变化特征进行分析,得到:在宇宙线静日期间普遍存在准24 h周期变化特征,并且在当地时间0200,1400左右分别出现最小值和最大值;对12个例子的分析可以看到地面宇宙线强度在地磁暴之前1-2天均出现了不同于宇宙线静日期间变化特征,或有小尺度周期出现,或周期变化完全消失,或有异常24h周期变化,这种变化特征在一定程度上可作为地磁预报的先兆特征之一. 展开更多
关键词 地磁暴 宇宙线强度 MORLET小波 小波变换 数据分析 宇宙射线
下载PDF
Cosmic Ray Associated with Coronal Index and Solar Flare Index during Solar Cycle 22 - 23
4
作者 Prithvi Raj Singh Shabir Ahmad +3 位作者 A. C. Pandey Ajay Kumar Saxena Chandra Mani Tiwari A. P. Mishra 《International Journal of Astronomy and Astrophysics》 2017年第3期162-173,共12页
We study the relation between monthly average counting rates of the cosmic ray intensity (CRI) observed at Moscow Neutron Monitoring Station, solar flare index (SFI) and coronal index during the solar cycles 22 and 23... We study the relation between monthly average counting rates of the cosmic ray intensity (CRI) observed at Moscow Neutron Monitoring Station, solar flare index (SFI) and coronal index during the solar cycles 22 and 23, for the period 1986-2008. The long-term behaviour of various solar activity parameters: sunspot numbers (SSN), solar flare index (Hα flare index), coronal index (CI) in relation to the duration of solar cycles 22 and 23 is examined. We find that the correlation coefficient of CRI with the coronal index as well as Hα flare index is relatively large anti-correlation during solar cycle 22. However, the monthly mean values of sunspot number, Hα flare index, and coronal index are well positively correlated with each other. We have analyzed the statistical analysis of the above parameters using of linear model and second order polynomial fits model. 展开更多
关键词 SOLAR Activity SUNSPOT Number CORONAL INDEX SOLAR FLARE INDEX cosmic ray intensity
下载PDF
羊八井高度的超高能γ-线强度
5
作者 陆穗苓 任敬儒 +7 位作者 苏实 王承瑞 何瑁 张乃健 曹培园 李金玉 王士智 王明星 《山东大学学报(自然科学版)》 CAS CSCD 1996年第1期108-109,共2页
在西藏羊八井实验站高度(海拔4300m)建立了乳胶室,给出了这一高度的超高能γ线强度与能谱.结合以往在珠峰脚下、甘巴拉山、云南站等地观测的结果。
关键词 宇宙线 乳胶室 超高能γ线 垂向流强
原文传递
Comparative study of solar cycles 22 to 24 in relation to solar output variability
6
作者 Sham Singh Divya Shrivastava +1 位作者 Shri Ram Lahauriya Adya Prasad Mishra 《Natural Science》 2012年第6期349-354,共6页
The rate of increase in solar activity at the initiation of solar cycle 22 had led the activity during the solar maximum years 1990-1991, be the most severe of any period during the space age. Solar cycle 23 started i... The rate of increase in solar activity at the initiation of solar cycle 22 had led the activity during the solar maximum years 1990-1991, be the most severe of any period during the space age. Solar cycle 23 started in May 1996 and ended in December 2008. Total time period of this solar cycle is 12.6 years. The maximum smoothed sunspot number observed during the solar cycle was 120.8 and minimum was 1.7. It is apparent that solar cycle 23 is a long one. Solar cycle 24 (initiated in December 2008) seems to be weak, which will have a slow ramp up, much slower than the late 19th century cycles used for comparison. In the present work, we have considered Sunspot number (Rz) as an index of solar activity, which shows a predominant 11 year cycle. The strength of the solar cycle makes a huge difference to satellite operators. Each solar peak heats and expands the outer atmosphere. The strength of the solar-cycle length, annual average and temperature correlation enables solar cycle length to be used as a climate predictor tool. 展开更多
关键词 SOLAR ACTIVITY cosmic ray intensity andGeomagnetic ACTIVITY
下载PDF
上一页 1 下一页 到第
使用帮助 返回顶部