During geomagnetic quiet conditions, Indian Antarctic stations are considered to be located
outside the auroral oval: Maitri (CGM coordinates: 63.3° S, 54.2° E) is equatorward and …

Variations in the Solar quiet (Sq) current are typically attributed to the changes in
atmospheric tides. In this study, we analyzed the ground‐based observations of the …

The present study investigated the variability in Equatorial electrojet (EEJ) and Counter
electrojet (CEJ) extracted at the Indian equatorial station Tirunelveli (TIR) using low‐latitude …

Equinoctial asymmetry of the range of the solar quiet day variation (Sq) of the horizontal
geomagnetic field (H) has been found in some low latitude geomagnetic observatories. This …

Studies made earlier using ground‐based observations of geomagnetic field over the Indian
longitudes revealed that the occurrence of equatorial counter electrojet (CEJ) events in …

The Himalayas are a region of geomagnetic importance, as they impact the geomagnetic
field of Earth and space weather, as it is one of the largest mountain belts in the world. Due …

The interannual variation of the ionospheric solar quiet (Sq) current system is examined. A
dense magnetometer network over Japan enables the accurate determination of the central …

It was known that the Solar quiet (Sq) current is important for the ionosphere dynamics,
which can cause variations in the geomagnetic fields recorded on the ground. Using a north …

Pc5 ULF (ultra-low frequency) waves can energize electrons to relativistic energies of> 2
MeV in geostationary orbits. Enhanced fluxes of such electrons can induce operational …

Solar quiet variation (Sq) generated from ionospheric currents are among the most important
type of geomagnetic variations. In this paper, the correlation between the geomagnetic Z …