Relationship Between Sunspot and Solar Wind Parameters During the Ascending Phase

Abstract

The characteristics of the solar wind, such as the magnetic field and plasma velocity, are dependent on the sunspot activity cycle overall. One of the most significant indicators for determining the sun's overall activity levels is the sunspot cycle. In the plot, we examine solar wind measurements made during solar cycle 25's rising phase and contrast them with comparable information from cycles 24 before. To determine the association between solar wind plasma properties and sunspots, information collected by the ACE and STEREO A spacecraft and NOAA (National Oceanic and Atmospheric Administration) was utilised. Analysis was done on the solar wind details during the 24 and 25 solar increasing activity phases, including sunspot, magnetic field, temperature, density, and wind speed. Many correlations between different features of the sunspot cycle have been discovered. A softer form of the solar wind emerges from the corona during solar minimum due to the Sun's low activity.