IAGA Division IV - Solar Wind and Interplanetary Field
Turbulent motions inside the Sun supply energy to produce not only the magnetized atmosphere at 1 million Kelvin but also enormous energy release events, including coronal mass ejections and solar energetic particles acceleration. The solar wind and the heliosphere are thus a natural plasma laboratory energized by constant free energy input from the Sun. Division IV represents all research fields related to these phenomena.
IAGA Division IV Leaders
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EC Liaison Person: |
Anna Kelbert |
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Chair: |
Cynthia Lopez-Portela |
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Co-Chair: |
Laura Rodríguez García |
