NASA/TP-3674, Wilson, Robert M. and Hathaway, David H. and Reichmann, Edwin J., Gauging the Nearness and Size of Cycle Minimum, Space Sciences Laboratory. NASA Marshall Space Flight Center, AL 35812, February 1997, pp. 20, Format(s): PDF 1511k |
By definition, the conventional onset for the start of a sunspot cycle is the time when smoothed sunspot number (i.e., the 12-month moving average) has decreased to its minimum value (called minimum amplitude) prior to the rise to its maximum value (called maximum amplitude) for the given sunspot cycle. On the basis of the modern era sunspot cycles 10-22 and on the presumption that cycle 22 is a short-period cycle having a cycle length of 120 to 126 months (the observed range of short-period modern era cycles), conventional onset for cycle 23 should not occur until sometime between September 1996 and March 1997, certainly between June 1996 and June 1997, based on the 95-percent confidence level deduced from the mean and standard deviation of period for the sample of six short-period modern era cycles. Also, because the first occurrence of a new cycle, high-latitude (-25 degrees) spot has always preceded conventional onset of the new cycle by at least 3 months (for the data-available interval of cycles 12-22), conventional onset for cycle 23 is not expected until about August 1996 or later, based on the first occurrence of a new cycle 23, high-latitude spot during the decline of old cycle 22 in May 1996. Although much excitement for an earlier-occurring minimum (about March 1996) for cycle 23 was voiced earlier this year, the present study shows that this exuberance is unfounded. The decline of cycle 22 continues to favor cycle 23 minimum sometime during the latter portion of 1996 to the early portion of 1997.
| Keywords: | sun, sunspot cycle, solar cycle, prediction, mg ii index |
|---|---|
| CASI Document ID Number: | 97N18137 |
| Subjects: | Space Sciences: Solar Physics |
| ID Code: | 366 |
| Deposited On: | 03 July 2002 |