Shocks and Fermi-I Acceleration. Non-Relativistic Shocks p 1, 1, T 1 p 0, 0, T 0 vsvs p 1, 1, T 1 p 0, 0, T 0 v 0 = -v s Stationary Frame Shock Rest Frame.
G. Marklund Space & Plasma Physics, School of Electrical Engineering, KTH Stockholm, Cluster multi-probing of the aurora above and within the acceleration.
The Focusing Optics X-ray Solar Imager (FOXSI) Steven Christe 1, S. Krucker 2, L. Glesener 2, S. Ishikawa 3, B. Ramsey 4, T. Takahashi 3, R.P. Lin 2 1.
Mass Spectrometry Andrew Rouff and Ben Berger. A Brief History 1897- JJ Thomson recorded first mass-to-charge ratio of electrons 1951- W. Pauli and H.
M-I Coupling Scales and Energy Conversion Processes Gerhard Haerendel Max Planck Institute for Extraterrestrial Physics 04 July 2013 MPE-JUB Symposium.
David Smith CENBG Plans for Radio Pulsar Timing GLAST collaboration meeting, Stockholm, 30 August 2006 1 Radio Timing for GLAST Pulsars Radio Timing for.
Investigation of the source region of ionospheric oxygen outflow in the cusp using multi-spacecraft observations by CIS onboard Cluster COSPAR, 2002, Houston,
Imaging spectroscopy in electron space Marco Prato Pure and Applied Mathematics Department University of Modena and Reggio Emilia, Italy CNR – INFM LAMIA,
Collective effects of stellar winds and unidentified gamma-ray sources Diego F. Torres THE MULTI-MESSENGER APPROACH TO UNIDENTIFIED GAMMA-RAY SOURCES [email protected].
The GRB literature has been convolved with my brain
ROPA/REIMEI show ~300eV inverted-V type spatial structures Collocated with region of patches but not correlated with individual patches Low energy precipitation.
Mariano Andrenucci Professor, Department of Aerospace Engineering, University of Pisa, Italy Chairman and CEO, Alta S.p.A, Via A. Gherardesca 5, 56121.