Issue |
A&A
Volume 407, Number 1, August III 2003
|
|
---|---|---|
Page(s) | L13 - L16 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361:20030977 | |
Published online | 17 November 2003 |
Letter to the Editor
Tilt and
of major flare-producing active regions
1
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, PR China
2
W.W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA 94305, USA
Corresponding author: L. R. Tian, tlr@ns.bao.ac.cn
Received:
21
March
2003
Accepted:
25
June
2003
We surveyed 86 active regions
in the years
from 1996 to 2002 in the 23rd solar cycle
that produced more than three
major flares.
We studied the
systematic tilt angle with respect to
the solar equator and
the
force-free parameter of the magnetic field of
the active regions,
and we
obtained the following results. (1) Only 46 (54%) of the active regions follow Joy's law. (2) 43 (50%) active
regions obey the hemispheric helicity rule. (3) 56 (65%) have the same sign for the tilt and the
, and the tilt and the
of all 86 regions are positively correlated. (4) 33 (60%) of the 55 active regions which have an
magnetic configuration show the same sign
for the tilt and
.
It is commonly
believed that the sign of the tilt and
obtained in the photosphere
can describe
the sign of
the twist and writhe
of
the flux tube rising from the convection zone.
Therefore, the results above appear to support
the kink hypothesis
for active regions that the sign of the twist and writhe
should be the same where a kink instability has developed
(Linton et al. [CITE]).
Key words: Sun: twist and writhe / Sun: major flares / Sun: active regions
© ESO, 2003
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