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

EC Liaison Person:

Anna Kelbert

Chair:

Cynthia Lopez-Portela
NASA-Goddard Space Flight Center
Solar Physics Laboratory
Code 671
Greenbelt, MD 20771
USA
cynthia.lopezportela@nasa.gov

Co-Chair:

Laura Rodríguez García
European Space Agency
ESAC, Madrid
Spain
Laura.RodriguezGarcia@esa.int

 

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