1. 1 Introduction The minimum mission requirement for “Project Icarus” is to receive first data from Alpha Centauri in 100 years. For maximum data-return the probe needs…
Slide 1Charge-Exchange Spectroscopy at the University of Wisconsin-Madison Mark Nornberg Santhosh Kumar, Daniel Den Hartog Alexis Briesemeister 2012 ADAS Workshop …
Slide 1 Chapter 3. Transport Equations The plasma flows in planetary ionospheres can be in equilibrium (d/dt = 0), like the midlatitude terrestrial ionosphere, or in noneqilibrium…
Slide 1 Solar Physics & Space Plasma Research Center (SP 2 RC) The role of partial ionisation in the stability of prominences structures Istvan Ballai SP 2 RC, School…
EISCAT-Cluster observations of quiet-time near-Earth magnetotail fast flows and their signatures in the ionosphere Nordic Cluster Meeting, Uppsala, Sweden, 24 – 25 August…
Lecture 9 Solar Wind-Magnetosphere Interaction Structure of the Magnetosphere Solar Wind-Magnetosphere Interaction: Reconnection and IMF Dependence The Magnetosphere The…
PROBA 2 Guest Investigator project (2010-2012) EUV imaging of the solar corona and study of slow solar wind streams V. Slemzin1, L. Harra2, S. Kuzin1, A. Urnov1, F. Goryaev1,…