A new parameter of geomagnetic storms for the severity of space weather
Nanan Balan, Inez Staciarini Batista, S. Tulasi Ram, P. K. Rajesh
Abstract
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Nanan Balan, Inez Staciarini Batista, S. Tulasi Ram, P. K. Rajesh
Abstract
Open-access reader
Using the continuous Dst data available since 1957 and H component data for the Carrington space weather event of 1859, the paper shows that the mean value of Dst during the main phase of geomagnetic storms, called mean Dst MP , is a unique parameter that can indicate the severity of space weather. All storms having high mean Dst MP (≤−250 nT), which corresponds to high amount of energy input in the magnetosphere–ionosphere system in short duration, are found associated with severe space weather events that caused all known electric power outages and telegraph system failures.
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Using the continuous Dst data available since 1957 and H component data for the Carrington space weather event of 1859, the paper shows that the mean value of Dst during the main phase of geomagnetic storms, called mean Dst MP , is a unique parameter that can indicate the severity of space weather. All storms having high mean Dst MP (≤−250 nT), which corresponds to high amount of energy input in the magnetosphere–ionosphere system in short duration, are found associated with severe space weather events that caused all known electric power outages and telegraph system failures.
Key concepts: Space weather, Geomagnetic storm, Ionosphere, Storm, Earth's magnetic field, Meteorology, Magnetosphere, Environmental science