Abstract
The magnetic field variations observed at Ahmedabad during the magnetic storm of August 4 to 6, 1972 are subjected to power Spectrum Analysis. The storm is divided in five parts depending upon its morphology and phase. Prominent peaks are observed in the range of 60–300 sec periods. The prominent periods and their respective power are studied in relation to the progress and phase of the storm. These are then related to the condition of the magnetosphere and the interplanetary medium observed at the time of the storm.
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