On a geomagnetically quiet night of July 07, 2018, the allsky imager at Hanle, Leh Ladakh (32.7°N, 78.9°E; Mlat. ∼24.1°N), India captured a number of plasma structures in O (1D) 630.0 nm airglow emission. In a short observational period of around 3 h, two different medium scale traveling ionospheric disturbances and two different mid‐latitude plasma depletions were observed. The most interesting aspect of the night was the drastic difference in the behavior of the two plasma depletions, which simultaneously existed within the imager's field of view for a long time. One of the plasma depletions, which we have termed as mid‐latitude field‐aligned plasma depletion, was nearly field aligned, drifted westward very slowly and became more prominent later in the night. The other depletion showed a much more ambiguous behavior with large reduction in its drift as well as significant change in its orientation relative to the geomagnetic meridian. In the present study, we have tried to explain this contrasting behavior in two different scenarios and have discussed arguments supporting each scenario along with their limitations. These observations are particularly useful considering the location of Hanle, which lies at a transition of geomagnetically low‐mid latitudes, which are governed by different electrodynamics.
Solar energetic events, namely coronal mass ejections (CMEs) and Stream Interaction regions/corotating interaction regions (SIRs/CIRs), are the principal drivers of the major space weather phenomena in the planetary atmosphere. CMEs are defined as a huge burst of plasma and magnetic field originating from the outer surface of the sun (Gopalswamy, 2006;Gosling, 1990;Jian et al., 2006). CMEs traverse all the way from the solar corona to interplanetary space, preceded by forward shock (Chen, 2011;Tousey, 1973). They are commonly characterized by a strong rotating magnetic field, low β (ratio of plasma pressure and magnetic pressure), low ion temperature, high proton density, and enhancement in velocity (
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