Abstract
This paper presents results of observational and modeling work on the dynamics in the inner magnetosphere during geomagnetic storms. Using statistics from POLAR/CAMMICE/MICS instrument it is shown that the ring current energy density is a complex function of the solar wind input and substorm activity. These results are examined using time-varying models for the magnetic and electric fields during storm periods. It is shown that (even strong) stationary convection electric field does not produce a sufficiently high-energy ring current. The same is true for a single electric field pulse representing an isolated substorm. Our preliminary results indicate that a series of substorms with inward transport and acceleration of particles by inductive electric fields are required for the production of an intense ring current.
Original language | English |
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Title of host publication | PROCEEDINGS OF THE FIFTH INTERNATIONAL CONFERENCE ON SUBSTORMS |
Editors | A Wilson |
Publisher | European Space Agency |
Pages | 451-454 |
Number of pages | 4 |
ISBN (Print) | 92-9092-772-0 |
Publication status | Published - 2000 |
MoE publication type | A4 Conference publication |
Event | International Conference on Substorms - St. Petersburg, Russian Federation Duration: 16 May 2000 → 20 May 2000 Conference number: 5 |
Publication series
Name | ESA SPECIAL PUBLICATIONS |
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Publisher | ESA PUBLICATIONS DIVISION C/O ESTEC |
Volume | 443 |
ISSN (Print) | 0379-6566 |
Conference
Conference | International Conference on Substorms |
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Abbreviated title | ICS |
Country/Territory | Russian Federation |
City | St. Petersburg |
Period | 16/05/2000 → 20/05/2000 |