IAE
Maurizio Candidi Istituto di Fisica dello Spazio Interplanetario – IFSI Istituto Nazionale di AstroFisica - INAF Relazioni Sole-Terra… … verso una meteorologia.
Coestimating models of the large-scale internal, external, and corresponding induced Hermean magnetic fields Michael Purucker and Terence Sabaka Raytheon.
OMI Science Team Meeting KNMI, De Bilt, the NetherlandsMarch 12, 2014 Results from the OMPS Nadir Instruments on Suomi NPP Satellite Richard McPeters NASA.
Space Weather. Coronal loops Intense magnetic field lines trap plasma 203911main_TRACE_loop_arcade_lg.jpg.
21 ECRS, Kosice, 12/09/2008 Trapped charge particles measurements in the radiation belt by PAMELA instrument Vladimir V. Mikhailov (MEPHI) for PAMELA collaboration.
STScI TIPS 19 January 2006 Removing SAA-Persistent Cosmic Ray Flux from NICMOS Anton Koekemoer (INS) 1 Removing SAA-Persistent Cosmic Ray Flux from NICMOS.
PAMELA Payload for Antimatter Matter Exploration and Light Nuclei Astrophysics.
Institutes Royal Observatory of Belgium (Brussels, BE) Principal Investigator, overall design, onboard software specification, science operations PMOD/WRC.
© NERC All rights reserved Chris Turbitt Observatories Manager Geomagnetism Team British Geological Survey BGS Observatory Network.
Particle moving in uniform magnetic field: Coordinate analysis
STScI 2010 Calibration Workshop The NICMOS Legacy Archival Recalibration Project
