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Aug. 31, 2010 to Aug. 31, AU Voyagers VEPO MSSP-2 Protons Ions Stereo A HET Stereo B HET
Aug. 31, 2010 to Aug. 31, 2011 Stereo A HET Stereo B HET VEPO MSSP-4 Electrons
Stereo A HET: August 31, 2010 to August 31, 2011 Electrons 0.7 – 1.4 MeV Electrons 2.6 – 4.0 MeV
New VEPO Service Multi-Spectral Scatter Plots Aug. 31, 2010 to Aug. 31, 2011 Impulsive SEP Electron Event Single Spectrum
Stereo B HET: August 31, 2010 to August 31, 2011
Aug. 31, 2010 to Aug. 31, 2011 Electron Hysteresis ? Event/Time evolution of SEP electron spectra New VEPO Service Flux Scatter Plots 0.7 – 1.4 MeV e flux 2.8 – 4.0 MeV e flux
Aug. 31, 2009 to Aug. 31, 2010
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M. Mayer SEWG Fuel Retention June Sample Analysis for TS, AUG and JET: Depth Profiling of Deuterium M. Mayer Max-Planck-Institut für Plasmaphysik,
15-19 November, Brugge 7 th European Space Weather Week Creating an SEP flux database from ESA/SREM measurements I. Sandberg, I.A. Daglis and A.
The Life Cycles of Stars Dr. Jim Lochner, NASA/GSFC.
NUCP 2371 Radiation Measurements II. Since electromagnetic radiation does not cause any direct ionization Detector system needs to do several things Reasonable.
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Control of Magnetic Chaos & Self-Organization John Sarff for MST Group CMSO General Meeting Madison, WI August 4-6, 2004.
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