期刊
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
卷 55, 期 2, 页码 365-370出版社
SCIENCE PRESS
DOI: 10.1007/s11433-011-4612-6
关键词
solar physics; solar activity; sun spots; solar cycles
资金
- National Natural Science Foundation of China [10973020, 40890161, 10921303]
- National Basic Research Program of China [2011CB811406]
- China Meteorological Administration [GYHY201106011]
The growth rate of solar activity in the early phase of a solar cycle has been known to be well correlated with the subsequent amplitude (solar maximum). It provides very useful information for a new solar cycle as its variation reflects the temporal evolution of the dynamic process of solar magnetic activities from the initial phase to the peak phase of the cycle. The correlation coefficient between the solar maximum (R (max)) and the rising rate (beta (a)) at Delta m months after the solar minimum (R (min)) is studied and shown to increase as the cycle progresses with an inflection point (r = 0.83) at about Delta m = 20 months. The prediction error of R (max) based on beta (a) is found within estimation at the 90% level of confidence and the relative prediction error will be less than 20% when Delta m a (c) 3/4 20. From the above relationship, the current cycle (24) is preliminarily predicted to peak around October, 2013 with a size of R (max) = 84 +/- 33 at the 90% level of confidence.
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