Drop of solar wind at the end of the 20th century
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

TL;DR
The paper analyzes long-term variations in solar wind parameters over multiple solar cycles, revealing a significant decline at the end of the 20th century linked to decreased solar activity and space weather impacts.
Contribution
It provides a comprehensive analysis of solar wind parameter changes over 21-24 solar cycles using OMNI data, highlighting a notable decline at the end of the 20th century.
Findings
Noticeable drop (20-40%) in plasma parameters and magnetic field at cycle end.
Decrease in the number of ICMEs and associated Sheath types.
Persistent low levels of solar wind parameters in cycles 23-24.
Abstract
Variations in the solar wind (SW) parameters with scales of several years are an important characteristic of solar activity and the basis for a long-term space weather forecast. We examine the behavior of interplanetary parameters over 21-24 solar cycles (SCs) on the basis of OMNI database (https://spdf.gsfc.nasa.gov/pub/data/omni). Since changes in parameters can be associated both with changes in the number of different large-scale types of SW, and with variations in the values of these parameters at different phases of the solar cycle and during the transition from one cycle to another, we select the entire study period in accordance with the Catalog of large-scale SW types for 1976-2019 (See the site http://www.iki.rssi.ru/pub/omni, [Yermolaev et al., 2009]), which covers the period from 21 to 24 SCs, and in accordance with the phases of the cycles, and averaging the parameters at…
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