The Effect of Midnight Temperature Maximum Winds on Post‐Midnight Equatorial Spread F
Abstract The SAMI3/equatorial spread F (Sami3 is also a model of the ionosphere/ESF) code is used to simulate the growth of equatorial plasma bubbles in the presence of a background wind field based on measured winds. The measured winds exhibit the well‐known “midnight temperature maximum” (MTM) pat...
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Main Authors: | J. Krall, D. Hickey, J. D. Huba, P. B. Dandenault |
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Format: | Article |
Language: | English |
Published: |
Wiley
2021-08-01
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Series: | Space Weather |
Subjects: | |
Online Access: | https://doi.org/10.1029/2021SW002728 |
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