SOLAR WIND PARAMETERS IN RISING PHASE OF SOLAR CYCLE 25: SIMILARITIES AND DIFFERENCES WITH SOLAR CYCLES 23 AND 24

被引：1

作者：

Yermolaev, Yu, I ^{[1
]}

Lodkina, Lg ^{[1
]}

Khokhlachev, A. A. ^{[1
]}

Yermolaev, M. Yu ^{[1
]}

Riazantseva, M. O. ^{[1
]}

Rakhmanova, L. S. ^{[1
]}

Borodkova, N. L. ^{[1
]}

Sapunova, O., V ^{[1
]}

Moskaleva, A., V ^{[1
]}

机构：

[1] Space Res Inst RAS, Moscow, Russia

来源：

SOLAR-TERRESTRIAL PHYSICS | 2023年 / 9卷 / 04期

基金：

俄罗斯科学基金会;

关键词：

solar wind; solar cycle; AMPLITUDE; MINIMUM;

D O I：

10.12737/stp-94202307

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：

Solar activity and solar wind parameters decreased significantly in solar cycles (SCs) 23-24. In this paper, we analyze solar wind measurements at the rising phase of SC 25 and compare them with similar data from the previous cycles. For this purpose, we simultaneously selected the OMNI database data for 19762022, both by phases of the 11-year solar cycle and by large-scale solar wind types (in accordance with catalog [http://www.iki.rssi.ru/pub/omni]), and calculated the mean values of the plasma and magnetic field parame- ters for the selected datasets. The obtained results support the hypothesis that the continuation of this cycle will be similar to that of cycle 24, i.e. SC 25 will be weaker than SCs 21 and 22.

引用

页码：55 / 62

页数：8

共 36 条

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