太阳活动周期及其数学描述
Research and Description about the Cycle of Solar Active by Mathematics
查看参考文献71篇
文摘
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概述和分析了太阳活动周期的研究进展,太阳活动呈现非常复杂的周期性,其周期性范围从几天至上百年,11年周期意义比较大,也比较明显;几天至几个月的周期性可能发生在太阳活动高峰期,155天或更短的周期存在,对中期预报有帮助;几年左右的周期对气象学的研究有作用;"蒙德极小期"是否存在至今还没有定论.对太阳活动11年周期的数学描述虽然很多,从效果上看,一般情况下,参数较多的函数计算量很大,误差相对较小;参数少的函数相比参数多的函数误差大,但计算量小;目前还没有一个非常理想的函数.能够对每个活动周都能很好的描述且误差很小. |
其他语种文摘
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In this paper,the progress of research on the cycle of solar activety is summarized and analyzed.The length of the one cycle of solar activity has ranged from only a few day to nearly hundred years,but the sunspot cycle has a prominent mean period of 11 years.The cycle length from a few days to several monthes is possible in the peak period of solar activety,the cycle and is helpful for the medium-term predictions of solar activity and research on the weather.The various kinds of mathematical description for the prominent mean period in the 11 years of solar cycle are also introduced in tihs paper. |
来源
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天文研究与技术
,2008,5(2):106-115 【核心库】
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关键词
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太阳
;
太阳活动-太阳
;
黑子-太阳
;
耀斑
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地址
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1.
景德镇陶瓷学院, 江西, 景德镇, 333001
2.
景德镇高等专科学校, 江西, 景德镇, 333000
3.
景德镇第一中等专业学校, 江西, 景德镇, 333000
4.
中国科学院国家天文台云南天文台, 云南, 昆明, 650011
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语种
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中文 |
文献类型
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研究性论文 |
ISSN
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1672-7673 |
学科
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天文学 |
基金
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江西省自然科学基金
;
景德镇陶瓷学院博士科研基金资助
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文献收藏号
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CSCD:3327712
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参考文献 共
71
共4页
|
1.
Wilson R M. On the behavior of the sunspot cycle near minimum.
J Goophys Ras,1996,101(9):19967
|
被引
1
次
|
|
|
|
2.
王家龙. 第22和23太阳周太阳活动预测.
天体物理学报,1992,12:369
|
被引
6
次
|
|
|
|
3.
Bogart R S. Recurrence of solar activity-Evidence for active longitudes.
Solar Physics,1982,76:155
|
被引
1
次
|
|
|
|
4.
Prabhakaran Nayar S R. Wavelet Analysis of solar solar wind and geomagnetic parameters.
Solar Physics,2002,208:359
|
被引
13
次
|
|
|
|
5.
Zhan L S. The wavelet analysis of the period of solar activity.
Chinese Astronomy and Astrophysics,2006,30:393
|
被引
2
次
|
|
|
|
6.
Kane R P. Maximum entropy spectral analysis of some artificial samples.
J Geophys Res,1979,84:965
|
被引
1
次
|
|
|
|
7.
Kane R P. Prediction of the sunspot maximum of solar cycle 23 by extrapolation of spectral components.
Solar Physics,1999,189:217-224
|
被引
9
次
|
|
|
|
8.
Svalgaard L. Long-term evolution of solar sector structure.
Solar Physics,1975,41:461
|
被引
3
次
|
|
|
|
9.
Gosling J T. Preferred solar wind emitting longitudes on the sun.
J Geophys Res,1977,82:2371
|
被引
1
次
|
|
|
|
10.
Neugebauer M. The solar magnetic field and the solar wind:Existence of preferred longitudes.
J Geophys Res,2000,105(2):2315
|
被引
3
次
|
|
|
|
11.
Javaraiah J. Short-term periodicities of the sun's mean and differential rotation.
Solar Physics,1999,184:41
|
被引
2
次
|
|
|
|
12.
Bolton S J. One year variations in the near earth solar wind ion density and bulk flow velocity.
Geophys Res,1990,17:37
|
被引
1
次
|
|
|
|
13.
Paularena K I. 3-year periodicities in the ap geomagnetic index and the solar wind.
Geophys Res,1995,22:3001
|
被引
1
次
|
|
|
|
14.
Rieger E. A 154-day periodicity in the occurrence of hard solar flares.
Nature,1984,312:623
|
被引
17
次
|
|
|
|
15.
Bai T. Evidence for a fundamental period of the sun and its relation to the 154day complex of periodicities.
ApJ,1993,409:476
|
被引
4
次
|
|
|
|
16.
Lean J L. Intermediate-term solar periodicities 100-500 days.
ApJ,1989,337:568
|
被引
8
次
|
|
|
|
17.
Lean J. Evolution of the 155 day periodicity in sunspot areas during solar cycles 12 to 21.
ApJ,1990,363:718
|
被引
3
次
|
|
|
|
18.
Gonzalez A L C. Periodicities in the interplanetary magnetic field polarity.
Geophys Res,1987,92:4357
|
被引
1
次
|
|
|
|
19.
Mursula K. Solar excursion phases during the last 14 solar cycles.
Geophys Res,1998,25:1851
|
被引
1
次
|
|
|
|
20.
Attolini M R. On the persistence of the 22 Y solar cycle.
Solar Physics,1990,125:389
|
被引
1
次
|
|
|
|
|