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Does a low solar cycle minimum hint at a weak upcoming cycle? View all abstracts by submitter

Z. L. Du   Submitted: 2010-08-14 04:58

The maximum amplitude (Rm) of a solar cycle, in the term of mean sunspot numbers, is well-known to be positively correlated with the preceding minimum (Rmin). So far as the long term trend is concerned, a low level of Rmin tends to be followed by a weak Rm, and vice versa. In this paper, we found that the evidence is insufficient to infer a very weak Cycle 24 from the very low Rmin in the preceding cycle. This is concluded by analyzing the correlation in the temporal variations of parameters for two successive cycles.

Authors: Z. L. Du & H. N. Wang
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Publication Status: accepted by RAA
Last Modified: 2010-08-23 12:55
Go to main E-Print page  Laboratory Simulation of Arched Magnetic Flux Rope Eruptions in the Solar Atmosphere  Acoustic Power Absorption and its Relation with Vector Magnetic Field of a Sunspot  Edit Entry  Download Preprint  Delete Entry 

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