Unstable Solar, Interplanetary, and Geomagnetic Fields During Solar Cycles 23 and 24

Abstract

Short-term and long-term shifts in cosmic ray intensity (CR1) are caused by the sun's outputs and fluctuations. The observed correlation between solar activity and sunspots, solar radio radiation at 10.7 centimeters, coronal mass ejections (CM Es), and solar flares is strong. Furthermore, coronal mass ejections are linked to several plasma and field disturbances in the interplanetary medium. The data used to create this visualization comes from neutron monitors in Moscow, Oulu, and Keil, and it is based on monthly mean count rate variations in cosmic ray intensity (CRI) observed by the Omni web data center for solar-interplanetary data activities between 1996 and 2017.During the lowest of solar cycle 23 and the ascending part of solar cycle 24, we measured a record high value of cosmic ray intensity with low values of solar interplanetary activity parameters.