Solar Cycle Structure and Structure of Activity Cycles at Late-Type Stars

被引：0
|
作者：
Obridko, V. N. [1 ]
Sokoloff, D. D. [1 ,2 ]
Katsova, M. M. [3 ]
机构：
[1] IZMIRAN, Troitsk, Moscow, Russia
[2] Lomonosov Moscow State Univ, Moscow, Russia
[3] Lomonosov Moscow State Univ, Sternberg Astron Inst, Moscow, Russia
来源：
ASTRONOMY REPORTS | 2023年 / 67卷 / 12期
关键词：
solar cycle; late type stars; MAGNETIC-FIELD; SUN;
D O I：
10.1134/S1063772923120065
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
It is shown that a description of the solar cycle using the odd zonal harmonic of the solar magnetic field expands our capabilities in two important areas of solar research: first, in improving and expanding the forecast to the near future of evolution of the cyclic solar activity and, second, in developing a program for monitoring the spectrophotometric characteristics of radiation of solar-like stars, aimed at obtaining new information about their magnetic fields.
引用
收藏
页码：1442 / 1451
页数：10
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