NASA/TP-2004-213281, Wilson, Robert M. and Hathaway, David H., Application of the Maximum Amplitude-Early Rise Correlation to Cycle 23, George C. Marshall Space Flight Center , Marshall Space Flight Center, AL 35812, National Aeronautics and Space Administration, Washington, DC 20546-0001, June 2004, pp. 24, Format(s): PDF 812k |
On the basis of the maximum amplitude-early rise correlation, cycle 23 could have been predicted to be
about the size of the mean cycle as early as 12 mo following cycle minimum. Indeed, estimates for the size of
cycle 23 throughout its rise consistently suggested a maximum amplitude that would not differ appreciably
from the mean cycle, contrary to predictions based on precursor information. Because cycle 23’s average
slope during the rising portion of the solar cycle measured 2.4, computed as the difference between the
conventional maximum (120.8) and minimum (8) amplitudes divided by the ascent duration in months
(47), statistically speaking, it should be a cycle of shorter period. Hence, conventional sunspot minimum
for cycle 24 should occur before December 2006, probably near July 2006 (±4 mo). However, if cycle 23
proves to be a statistical outlier, then conventional sunspot minimum for cycle 24 would be delayed until
after July 2007, probably near December 2007 (±4 mo). In anticipation of cycle 24, a chart and table are
provided for easy monitoring of the nearness and size of its maximum amplitude once onset has occurred
(with respect to the mean cycle and using the updated maximum amplitude-early rise relationship).
| Keywords: | sun, sunspot cycle, solar cycle, prediction |
|---|---|
| Subjects: | Space Sciences: Solar Physics |
| ID Code: | 674 |
| Deposited On: | 16 September 2004 |