EVIDENCE FOR A FUNDAMENTAL PERIOD OF THE SUN AND ITS RELATION TO THE 154 DAY COMPLEX OF PERIODICITIES

被引:89
作者
BAI, T
STURROCK, PA
机构
关键词
SUN; FLARES; FUNDAMENTAL PARAMETERS; INTERIOR;
D O I
10.1086/172680
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have analyzed the longitude distributions of major flares observed in the 1955-1991 interval, referring them to coordinate systems rotating about axes tilted with respect to the rotation axis of the solar envelope. We find that the longitude distribution exhibits the largest modulation in the coordinate system with the following parameters: rotation period, 25.50 days; tilt angle of the rotation axis, 40-degrees; tilt direction, toward the position of the Earth on December 4 in its orbit around the Sun. We interpret this as being due to an obliquely rotating structure (or a wave pattern rotating about an oblique axis) which has two exciters. We identify the period of 25.50 days as the fundamental period of the hypothetical ''clock'' proposed by Bai & Sturrock (1991). The periods of the subharmonics are 51.0, 76.5, 102.0, 127.5, and 153.0 days, in agreement with periodicities found from analysis of flare occurrence times.
引用
收藏
页码:476 / 486
页数:11
相关论文
共 33 条
[1]   CHLORINE AND GALLIUM SOLAR NEUTRINO EXPERIMENTS [J].
BAHCALL, JN ;
CLEVELAND, BT ;
DAVIS, R ;
ROWLEY, JK .
ASTROPHYSICAL JOURNAL, 1985, 292 (02) :L79-L82
[2]   PERIODICITIES OF THE FLARE OCCURRENCE RATE IN SOLAR CYCLE-19 [J].
BAI, T .
ASTROPHYSICAL JOURNAL, 1987, 318 (02) :L85-L91
[3]   THE 77-DAY PERIODICITY IN THE FLARE RATE OF CYCLE-22 [J].
BAI, T .
ASTROPHYSICAL JOURNAL, 1992, 388 (02) :L69-&
[4]   A 154 DAY PERIODICITY IN THE OCCURRENCE RATE OF PROTON FLARES [J].
BAI, T ;
CLIVER, EW .
ASTROPHYSICAL JOURNAL, 1990, 363 (01) :299-309
[5]   THE 154-DAY AND RELATED PERIODICITIES OF SOLAR-ACTIVITY AS SUBHARMONICS OF A FUNDAMENTAL PERIOD [J].
BAI, T ;
STURROCK, PA .
NATURE, 1991, 350 (6314) :141-143
[6]   METHODS OF PERIODICITY ANALYSIS - RELATIONSHIP BETWEEN THE RAYLEIGH ANALYSIS AND A MAXIMUM-LIKELIHOOD METHOD [J].
BAI, T .
ASTROPHYSICAL JOURNAL, 1992, 397 (02) :584-590
[8]   THE 152-DAY PERIODICITY OF THE SOLAR-FLARE OCCURRENCE RATE [J].
BAI, T ;
STURROCK, PA .
NATURE, 1987, 327 (6123) :601-604
[9]   SOLAR HOT-SPOTS ARE STILL HOT [J].
BAI, T .
ASTROPHYSICAL JOURNAL, 1990, 364 (01) :L17-L20
[10]  
BAI T, 1993, UNPUB NATURE