Dynamics of Large-Scale Solar-Wind Streams Obtained by the Double Superposed Epoch Analysis: 5. Influence of the Solar Activity Decrease

In solar cycles 23–24, solar activity noticeably decreased and, as a result, solar wind parameters decreased. Based on the measurements of the OMNI base for the period 1976–2019, the time profiles of the main solar wind parameters and magnetospheric indices for the main interplanetary drivers of mag...

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Bibliografische Detailangaben

Hauptverfasser:	Yuri I. Yermolaev, Irina G. Lodkina, Alexander A. Khokhlachev, Michael Yu. Yermolaev, Maria O. Riazantseva, Liudmila S. Rakhmanova, Natalia L. Borodkova, Olga V. Sapunova, Anastasiia V. Moskaleva
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	MDPI AG 2022-09-01
Schriftenreihe:	Universe
Schlagworte:	solar wind interplanetary phenomena interplanetary drivers solar-terrestrial physics
Online-Zugang:	https://www.mdpi.com/2218-1997/8/9/472
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