Vector magnetic field in solar polar region  

作　　者：邓元勇 汪景秀 艾国祥 

出　　处：《Science China Mathematics》1999年第10期1096-1102,共7页中国科学：数学（英文版）

基　　金：Project supported by the National Natural Science Foundation of China (Grant No. 19791090).

摘　　要：By means of ‘deep integration’ observations of a videomagnetograph the vector magnetic field was first systematically measured near the solar south polar region on April 12, 1997 when the Sun was in the minimal phase between the 22nd and 23rd solar cycle. It was found that the polar magnetic field deviated from the normal of solar surface by about 42.2° ± 3.2°, a stronger magnetic element may have smaller inclination, and that within the polar cap above heliolatitude of 50°, the unsigned and net flux densities were 7.8 × 10?4) T and ?3.4×10?4T, respectively, and consequently, the unsigned and net fluxes were about 5.5 × 1022 and ? 2.5 × 1022 Mx. The net magnetic flux, which belongs to the large-scale global magnetic field of the Sun, roughly appmaches the order of the interplanetary magnetic field (IMF) measured at distance of 1 AU.By means of ’deep integration’ observations of a videomagnetograph the vector magnetic field was first systematically measured near the solar south polar region on April 12, 1997 when the Sun was in the minimal phase between the 22nd and 23rd solar cycle. It was found that the polar magnetic field deviated from the normal of solar surface by about 42.2°±3.2°, a stronger magnetic element may have smaller inclination, and that within the polar cap above heliolatitude of 50°, the unsigned and net flux densities were 7.8×10^-4 T and -3.4×10^-4 T, respectively, and consequently, the unsigned and net fluxes were about 5.5×10²² and -2.5×10²² Mx. The net magnetic flux, which belongs to the large-scale global magnetic field of the Sun, roughly approaches the order of the interplanetary magnetic field （IMF） measured at distance of 1 AU.

关 键 词：VECTOR MAGNETIC FIELD POLAR FIELD MAGNETIC INCLINATION IMF. 

分 类 号：P182[天文地球—天文学]