Modulation in CRI Due to Solar-Interplanetary Causes during 1996–2018

Abstract

Abstract Solar outputs and their variations are responsible to produce modulation in cosmic ray intensity (CRI) both on short-term as well as on long–term basis. It is seen that sunspot number; 10.7 cm sun oriented radio transition, coronal mass launches (CMEs) and sunlight based flares are the causal connect to sun oriented movement (SA). In addition, coronal mass discharges are related with an assortment of interplanetary plasma and field aggravations. In view of the perception from Omniweb server farm for sun powered interplanetary information movement and month to month mean tally pace of enormous beam force (CRI) variety information from neutron screens (Moscow, Oulu,) during the time of 1996–2018. We observed a record high value of cosmic ray intensity with low values of solar interplanetary activity parameters during minimum of solar cycle 23/24. Statistical techniques are used to correlate data of solar interplanetary and count rate of cosmic ray intensity i.e. better anti-correlated with solar activity parameters. Keywords: Galactic cosmic ray (GCR), Coronal mass ejections (CMEs), solar Activity (SA) Solar Magnetic Field, Heliospheric Magnetic Field (HMF) Cite this Article B.K. Tiwari, B.R. Ghormare. Modulation in CRI Due to Solar-Interplanetary Causes during 1996-2018. Recent Trends in Electronics and Communication Systems . 2020; 7 (1): 21–25p.