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Magnetospheric Response to the Solar Wind as Indicated by the Cross-polar Potential Drop and the Low-latitude Asymmetric Disturbance Field : Volume 19, Issue 6 (30/11/-0001)

By Eriksson, S.

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Book Id: WPLBN0004000891
Format Type: PDF Article :
File Size: Pages 5
Reproduction Date: 2015

Title: Magnetospheric Response to the Solar Wind as Indicated by the Cross-polar Potential Drop and the Low-latitude Asymmetric Disturbance Field : Volume 19, Issue 6 (30/11/-0001)  
Author: Eriksson, S.
Volume: Vol. 19, Issue 6
Language: English
Subject: Science, Annales, Geophysicae
Collections: Periodicals: Journal and Magazine Collection (Contemporary), Copernicus GmbH
Historic
Publication Date:
-0001
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications

Citation

APA MLA Chicago

Blomberg, L. G., Karlsson, T., Ivchenko, N., Eriksson, S., & Marklund, G. T. (-0001). Magnetospheric Response to the Solar Wind as Indicated by the Cross-polar Potential Drop and the Low-latitude Asymmetric Disturbance Field : Volume 19, Issue 6 (30/11/-0001). Retrieved from http://www.ebooklibrary.org/


Description
Description: Alfvén Laboratory, Royal Institute of Technology, SE-10044 Stockholm, Sweden. The cross-polar potential drop Φpc and the low-latitude asymmetric geomagnetic disturbance field, as indicated by the mid-latitude ASY-H magnetic index, are used to study the average magnetospheric response to the solar wind forcing for southward interplanetary magnetic field conditions. The state of the solar wind is monitored by the ACE spacecraft and the ionospheric convection is measured by the double probe electric field instrument on the Astrid-2 satellite. The solar wind-magnetosphere coupling is examined for 77 cases in February and from mid-May to mid-June 1999 by using the interplanetary magnetic field Bz component and the reconnection electric field. Our results show that the maximum correlation between Φpc  and the reconnection electric field is obtained approximately 25 min after the solar wind has reached a distance of 11 RE from the Earth, which is the assumed average position of the magnetopause. The corresponding correlation for ASY-H shows two separate responses to the reconnection electric field, delayed by about 35 and 65 min, respectively. We suggest that the combination of the occurrence of a large magnetic storm on 18 February 1999 and the enhanced level of geomagnetic activity which peaks at Kp = 7- may explain the fast direct response of ASY-H to the solar wind at 35 min, as well as the lack of any clear secondary responses of Φpc  to the driving solar wind at time delays longer than 25 min.

Key words. Magnetospheric physics (solar wind-magnetosphere interactions; plasma convection) – Ionosphere (electric fields and currents)


Summary
Magnetospheric response to the solar wind as indicated by the cross-polar potential drop and the low-latitude asymmetric disturbance field


 

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