We compare the cosmic-ray response to interplanetary coronal mass ejections (ICMEs) and
corotating interaction regions (CIRs) during their passage in near-Earth space. We study the …

Earth's magnetic field usually occurred due to abnormal conditions in the interplanetary
magnetic field (IMF) and solar wind plasma emissions caused by various solar …

We present a catalog of high-speed streams, along with their solar sources for solar
cycleá23. We study their distribution during different years and different phases of solar …

The flux rate of cosmic rays incident on the Earth's upper atmosphere is modulated by the
solar wind and the Earth's magnetic field. The amount of solar wind is not constant due to …

We study the transient modulation of galactic cosmic rays (GCRs) due to coronal mass
ejections (CMEs) and their associated structures detected during most part of solar cycle 24 …

Association of solar flares and coronal mass ejections (CMEs) with ground-level
enhancement (GLE) is a recognized fact, but questions arise when a similar association is …

We made an effort to understand the associations and relationships between ground level
enhancement (GLE) events and solar flares for the time period of 1986–2006. Our results …

The transport of charged energetic particles in the presence of strong intermittent
heliospheric turbulence is computationally analyzed based on known properties of the …

This work uses MODIS aerosol optical thickness (AOT) data observed over Kuwait during
the 7-year interval 2000–2007. The values of AOT and the Ångström wavelength exponent …

We study the geomagnetic disturbances and solar wind plasma/field properties during the
passage of High Speed Solar Wind Streams (HSS) emanating from the sun. We consider the …