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- W2094557132 abstract "A quantitative model of geomagnetic activity is developed and utilized to investigate the causes of the diurnal, seasonal, and IMF sector variations in the AL index records. This auroral index was chosen for study because of its high sensitivity to the strength of the westward electrojet and, hence, magnetospheric substorm activity. After the introduction of corrections for processes not related to substorms, ability of the function B s 0.85 V ² to produce the observed variations in AL was examined. The annual variation of B s was determined by superposing the contributions to B s due to the inclination of the magnetic axis (Russell and McPherron, 1973) on an empirical mean distribution of B z . V was assumed constant. The predicted values of AL c have been compared with observed averages for 9 years of solar cycle 20. The predicted annual variation of AL c for toward and away sectors are in good agreement with observation. While the predicted semi‐annual component of AL c is in phase with observation, it is less than half the observed amplitude. The predicted diurnal variation of AL c for June is in satisfactory agreement with observation." @default.
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- W2094557132 date "1982-11-01" @default.
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- W2094557132 title "A quantitative model of geomagnetic activity" @default.
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- W2094557132 doi "https://doi.org/10.1029/ja087ia11p09054" @default.
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