Pole Heliophysique et Plasmas Astrophysiques » Wind Waves Public

This brainstorming, from 4 to 8 March 2016, was mostly dedicated to the study of the electron suprathermal particles in the solar wind from the QTN method. We discussed on recent studies on QTN from WIND/WAVES data, taking into account in particular the angle between the antenna and the solar wind speed on the proton thermal noise. We also focused on the anisotropy determination and discuss implications for applying the QTN method for future solar wind and coronal exploration missions Solar Orbiter and Solar Probe Plus.