Investigation of Joy's Law According to the Data of the Ussuriisk Astrophysical Observatory

被引:0
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作者
Erofeev, D. V. [1 ]
Erofeeva, A. V. [1 ]
机构
[1] Russian Acad Sci, Inst Appl Astron, St Petersburg, Russia
关键词
AXIAL TILT ANGLES; SUNSPOT; REGIONS;
D O I
10.1134/S001679322307006X
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Based on the 66-year series of observations of the Ussuriisk Astrophysical Observatory, the angles of inclination of the bipolar axes of sunspot groups (tilt angles) have been studied. It is found that the average tilt angle is 6.8 degrees +/- 0.2 degrees, and the angles of inclination of sunspot groups in the northern hemisphere of the Sun, on average, are 1.0 degrees larger than for the southern one. It was also found that the average tilt angles are practically independent of the maximum area of the sunspot group. The dependence of the tilt angles averaged in 5-degree latitudinal zones T-m from the heliographic latitude F in the first approximation is described by a linear function T-m = 0.16 degrees + 0.43 divided by F divided by. However the dependence T-m(F) also demonstrates significant deviations from the linear function, which look like two almost horizontal sections ("plateaus"). One of them is located near F = 15 degrees and the second is at F > 25 degrees. Dependencies T-m(F) calculated for groups of sunspots with small, medium, and large areas do not reveal significant systematic differences. These results are compared with the previously published results of the study of five series of data on the tilt angles of sunspot groups.
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页码:1007 / 1014
页数:8
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