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

EC Liaison Person:

Alan Thomson
awpt@bgs.ac.uk

Chair:

Mari Paz Miralles
Center for Astrophysics / Harvard & Smithsonian
60 Garden Street
MS 16
Cambridge, MA 02138
USA
mmiralles@cfa.harvard.edu
Tel: +1 617 496 7925

Co-Chair:

NoƩ Lugaz
Space Science Center, Institute for the Study of Earth, Oceans, and Space
University of New Hampshire
Durham, NH, 03824
USA
noe.lugaz@unh.edu
+1 603-862-5045

 

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