Gong p-mode frequency changes with solar activity

被引:41
作者
Bhatnagar, A [1 ]
Jain, K [1 ]
Tripathy, SC [1 ]
机构
[1] Udaipur Solar Observ, Phys Res Lab, Udaipur 313001, India
关键词
Sun : activity; Sun : oscillations;
D O I
10.1086/307600
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a correlation analysis of GONG p-mode frequencies with nine solar activity indices for the period from 1995 August to 1997 August. This study includes spherical harmonic degrees in the range 2-150 and the frequency range of 1500-3500 mu HZ. Using three statistical tests, the measured mean frequency shifts show strong to good correlation with activity indices. A decrease of 0.06 mu HZ in frequency during the descending phase of solar cycle 22 and an increase of 0.04 mu Hz in the ascending phase of solar cycle 23 are observed. These results provide the first evidence for change in p-mode frequencies around the declining phase of cycle 22 and the beginning of new cycle 23. This analysis further confirms that the temporal behavior of the solar frequency shifts closely follow the phase of the solar activity cycle.
引用
收藏
页码:885 / 888
页数:4
相关论文
共 16 条
[1]  
ANDERSON ER, 1998, ESA, P901
[2]  
[Anonymous], 1991, THEORY SOLAR OSCILLA
[3]   P-MODE FREQUENCY VARIATION IN RELATION TO GLOBAL SOLAR-ACTIVITY [J].
BACHMANN, KT ;
BROWN, TM .
ASTROPHYSICAL JOURNAL, 1993, 411 (01) :L45-L48
[4]   Solar cycle onset seen in SOHO Michelson Doppler Imager seismic data [J].
Dziembowski, WA ;
Goode, PR ;
DiMauro, MP ;
Kosovichev, AG ;
Schou, J .
ASTROPHYSICAL JOURNAL, 1998, 509 (01) :456-460
[5]   IMPLICATIONS OF SOLAR P-MODE FREQUENCY-SHIFTS [J].
GOLDREICH, P ;
MURRAY, N ;
WILLETTE, G ;
KUMAR, P .
ASTROPHYSICAL JOURNAL, 1991, 370 (02) :752-762
[6]  
GUBAU MA, 1992, ASTRON ASTROPHYS, V255, P363
[7]  
HARVEY JW, 1984, WORKSHOP SOLAR IRRAD, P197
[8]   The solar acoustic spectrum and eigenmode parameters [J].
Hill, F ;
Stark, PB ;
Stebbins, RT ;
Anderson, ER ;
Antia, HM ;
Brown, TM ;
Duvall, TL ;
Haber, DA ;
Harvey, JW ;
Hathaway, DH ;
Howe, R ;
Hubbard, RP ;
Jones, HP ;
Kennedy, JR ;
Korzennik, SG ;
Kosovichev, AG ;
Leibacher, JW ;
Libbrecht, KG ;
Pintar, JA ;
Rhodes, EJ ;
Schou, J ;
Thompson, MJ ;
Tomczyk, S ;
Toner, CG ;
Toussaint, R ;
Williams, WE .
SCIENCE, 1996, 272 (5266) :1292-1295
[9]  
Jimenez-Reyes SJ, 1998, ASTRON ASTROPHYS, V329, P1119
[10]  
KUHN JR, 1988, APJ, V331, P131, DOI DOI 10.1086/185251