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Magnetosphere Modelling.pdf

EGU2012-5471.pdf
Preview of Magnetosphere Modelling
🔗 Source: meetingorganizer.copernicus.org
📊 Size: 34 KB
📄 Pages: 1 page
⬇️ Downloads: 119

Summary

Modelling the high-latitude magnetosphere-ionosphere-thermosphere system is done using the Upper Atmosphere Model (UAM) for various solar wind/IMF conditions. The UAM calculates upper ionosphere convection and 3-D neutral wind circulation patterns. Key factors influencing the system include electromagnetic stresses from field-aligned currents (FACs) and energy deposition via Joule heating and particle precipitations. The model results are compared with observations, including CHAMP accelerometer measurements of neutral wind and density for stable solar wind/IMF conditions. The study aims to understand the complex, mutually dependent system driven by solar wind and IMF conditions.

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Description

Modelling the high-latitude magnetosphere-ionosphere-thermosphere system.
The UAM model is used to simulate various solar wind/IMF conditions.
Energy deposition via Joule heating is a key factor.

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  • File Format: PDF
  • File Size: 34 KB
  • Pages: 1
  • Language: EN
  • Total Downloads: 119
  • Last Updated: 1 week ago

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