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. 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, 2015-2019
EC Liaison Person |
Pieter Kotze |
|
Divison |
Spiros Patsourakos |
spatsour@cc.uoi.gr |
Division |
Bogdan Hnat |
B.Hnat@warwick.ac.uk |