2007
DOI: 10.1002/cjg2.1131
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The Significance of Solar Magnetic Field Direction Variation on Anomalous Variability of the Atmosphere Temperature on the Earth

Abstract: Based on 11‐year's period data of the sunspot and the periodic variation of the magnetic field of the sunspot, the time series of the magnetic index of the sunspot magnetic field (MI) is established. The analysis indicates that the average period of the solar magnetic activity is about 22.2 years, but it is not a constant. In most cases, when the period is short, the magnetic index is large, corresponding to strong solar activity; when the period is long the magnetic index is small, corresponding to weak solar… Show more

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Cited by 5 publications
(5 citation statements)
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“…This means that the 88 year cycle of the volcanic activities closely correlates to the 88 year cycle of the NASH, which reveals that the periodic surge of global strong volcanic activities inspires the same century periodicity surge in NASH. Similar to (12) and (13), we have obtained the variance contribution of 88 year cycle of NASH, which is 25.94%. This means that the strong volcanic activities have more than 25% variance contribution to inspire SLP of the 88 year cycle of the NASH.…”
Section: North Atlantic Subtropical Highmentioning
confidence: 73%
“…This means that the 88 year cycle of the volcanic activities closely correlates to the 88 year cycle of the NASH, which reveals that the periodic surge of global strong volcanic activities inspires the same century periodicity surge in NASH. Similar to (12) and (13), we have obtained the variance contribution of 88 year cycle of NASH, which is 25.94%. This means that the strong volcanic activities have more than 25% variance contribution to inspire SLP of the 88 year cycle of the NASH.…”
Section: North Atlantic Subtropical Highmentioning
confidence: 73%
“…In other words, a little while after the magnetism of the solar magnetic field moves from the minimum to the maximum, the air temperature anomaly follows a little behind the solar magnetism change. Previous studies in solar physics and sun-earth space physics (Qu et al, 2007;Wei, 2007;Liu Z X, 2005;Zhang and Wang, 2003;Cao et al, 2003;Xu, 2003;Li, 2001;Liu Y, 2001;Zhang D H, 2000;Zhang Z D, 1998;Dong, 1997;Shi and Wang, 1994) have proved that, at the two poles of the sun, the polarity of the large-scale magnetic field is contrary to each other as a dipole field and has an 11-year-period change in solar activity. Therefore, the 22-year-period change is explained.…”
Section: Effect Of Solar Magnetic Field Direction On July Temperaturementioning
confidence: 99%
“…一定的贡献. 众多研究表明, 太阳活动具有周期性变 化规律 [5,6] ; 其中以太阳黑子约11 a的周期 [7,8] 和太阳 磁场极性约22 a的周期性 [9] 变化最为显著. 赵明宇等 人 [10] 、杨若文等人 [11] 对太阳黑子与太阳活动之间的 关系进行了深入的研究, Haigh [12] , Friis-Christensen和 Lassen [13] 、赵新华和冯学尚 [14] 、刘立波等人 [15] 、赵 平等人 [16] 在太阳活动对全球气候及地表环境的影响 取得了可喜的成果; 太阳活动的周期性变化导致了 地球表层环境和全球气候也具有类似的周期性变化 规律 [17] .…”
Section: 也试图在行星运动对太阳活动产生的影响方面做出unclassified