Duskside F-region dynamo currents: its relationship with prereversal enhancement of vertical plasma drift

From magnetic field observations by CHAMP we estimate F-region dynamo current densities near the sunset terminator during solar maximum years from 2001 to 2002. The dynamo currents are compared with the pre-reversal enhancement (PRE) of vertical plasma drift as observed by ROCSAT-1. The seasonal...

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Bibliographic Details
Main Authors: J. Park, H. Lühr, B. G. Fejer, K. W. Min
Format: Article
Language:English
Published: Copernicus Publications 2010-11-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/28/2097/2010/angeo-28-2097-2010.pdf
Description
Summary:From magnetic field observations by CHAMP we estimate F-region dynamo current densities near the sunset terminator during solar maximum years from 2001 to 2002. The dynamo currents are compared with the pre-reversal enhancement (PRE) of vertical plasma drift as observed by ROCSAT-1. The seasonal-longitudinal variation of PRE can be largely related to the F-region dynamo current density, with the correlation coefficient reaching 0.74. The correlation can be further improved if we consider a zonal gradient of the E-region Pedersen conductivity, which also depends on season and longitude. It is widely accepted that the F-region dynamo drives PRE near sunset. For the first time, our observations provide confirmation for the close relationship between the F-region dynamo current density and PRE.
ISSN:0992-7689
1432-0576