TIME CORRELATION BETWEEN SOLAR STRUCTURAL PARAMETERS - P-MODE FREQUENCIES, RADIUS, AND NEUTRINO FLUX

被引：38

作者：

DELACHE, P

GAVRYUSEV, V

GAVRYUSEVA, E

LACLARE, F

REGULO, C

CORTES, TR

机构：

[1] UNIV MOSCOW,INST NUCL PHYS,MOSCOW,RUSSIA

[2] RUSSIAN ACAD SCI,INST NUCL RES,MOSCOW,RUSSIA

[3] OBSERV COTE DAZUR,CNRS LAB,URA 1360,CERGA,F-06460 ST VALLIER THIEY,FRANCE

[4] INST ASTROFIS CANARIAS,E-38205 LA LAGUNA,SPAIN

来源：

ASTROPHYSICAL JOURNAL | 1993年 / 407卷 / 02期

关键词：

ELEMENTARY PARTICLES; SUN; FUNDAMENTAL PARAMETERS; OSCILLATIONS;

D O I：

10.1086/172561

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present an analysis of time correlations between measurements of solar radius, neutrino flux data, and acoustic mode frequency shifts. We find significant anticorrelation of the first two quantities with the last one. Variations are found over time scales of order the 11 yr solar cycle and at shorter time scales. The shorter periods, of order 1 yr, are better detected during the period 1985-1991. These correlations strongly suggest the possibility that dynamical processes detected in upper solar layers are closely related with perturbations inside the Sun, down to the core.

引用

页码：801 / 805

页数：5

共 22 条

[1]

ANSELMAN P, 1992, UNPUB PHYS LETT B

[2] SOLAR STRUCTURE FROM GLOBAL STUDIES OF THE 5-MINUTE OSCILLATION [J].