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Technology Magnetic sail braking vs two-stage fusion rockets

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…

Documents Plasma Wind Tunnel

1. 2A-1Overview of IRS Plasma Wind Tunnel Facilities Monika Auweter-Kurtz, Thomas WegmannUniversitat StuttgartInstitut fir Raumfahrtsysteme Pfaffenwaldring 3 1 70550 Stuttgart…

Documents Charge-Exchange Spectroscopy at the University of Wisconsin-Madison Mark Nornberg Santhosh Kumar,...

Slide 1Charge-Exchange Spectroscopy at the University of Wisconsin-Madison Mark Nornberg Santhosh Kumar, Daniel Den Hartog Alexis Briesemeister 2012 ADAS Workshop …

Documents STORM Annual Meeting - Graz, November 25-26, 2013 A brief overview of magnetosheath physics Maria...

Slide 1 STORM Annual Meeting - Graz, November 25-26, 2013 A brief overview of magnetosheath physics Maria Federica Marcucci INAF-IAPS STORM Annual Meeting - Graz, November…

Documents Chapter 3. Transport Equations The plasma flows in planetary ionospheres can be in equilibrium (d/dt...

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…

Documents Solar Physics & Space Plasma Research Center (SP 2 RC) The role of partial ionisation in the...

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…

Documents EISCAT-Cluster observations of quiet-time near-Earth magnetotail fast flows and their signatures in....

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…

Documents Lecture 9 Solar Wind-Magnetosphere Interaction Structure of the Magnetosphere

Lecture 9 Solar Wind-Magnetosphere Interaction Structure of the Magnetosphere Solar Wind-Magnetosphere Interaction: Reconnection and IMF Dependence The Magnetosphere The…

Documents The goal of the study : To localize sources of the quasi-stationary slow solar wind. Method:

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,…

Documents IKI, Feb. 2007 1 Новые сведения о структуре и динамике...

Новые сведения о структуре и динамике магнитосферных токовых слоев В. А. Сергеев (СПбГУ), Thanks to…