Magnetic Signatures of Ionospheric Disturbance Dynamo for CME and HSSWs Generated Storms
Abstract Ionospheric disturbance dynamo is one of the main processes that causes perturbations in the upper atmosphere during a magnetic storm. We present a new method, based on the least square fitting, for estimation of the magnetic signatures associated with ionospheric disturbance currents. Usin...
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| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Wiley
2021-09-01
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| Series: | Space Weather |
| Online Access: | https://doi.org/10.1029/2021SW002825 |
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