Issue |
A&A
Volume 401, Number 2, April II 2003
|
|
---|---|---|
Page(s) | L9 - L12 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20030272 | |
Published online | 21 March 2003 |
Letter to the Editor
Predictions of strengths of long-term variations in sunspot activity
Indian Institute of Astrophysics, Bangalore – 560 034, India
Corresponding author: jj@iiap.ernet.in
Received:
13
November
2002
Accepted:
24
February
2003
Recently, using Greenwich data (1879–1976) and SOON/NOAA data (1977–2002) on
sunspot groups we found a big or a moderate drop
in the solar equatorial rotation rate, A, occurred after every four
solar cycles suggesting the existence of “double Hale cycle (DHC)"
and “Gleissberg cycle (GC)" in A. We also found the existence
of “Hale cycle (HC)" and GC in the latitude gradient of the
rotation, B (Javaraiah [CITE]). Using these results here we made
forecasts for the following: (i) epochs of the forthcoming big
and moderate drops in A; (ii) the epoch of maximum during
the current GC of B; (iii) the strengths of DHCs and HCs of sunspot
activity which follow the big and the moderate drops in A; (iv) violation of the Gnevyshev & Ohl rule during the current HC 11
which consists of cycles 22 and 23; and (v) deduced the
near complete absence of sunspot activity during
the deep Maunder minimum.
Key words: Sun: rotation / Sun: activity / Sun: sunspots
© ESO, 2003
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