Conveners
AP-9/AE-9 Business Meeting
- PAUL OBRIEN (The Aerospace Corporation)
AP-9/AE-9 Business Meeting: Session #2
- PAUL OBRIEN (The Aerospace Corporation)
AP-9/AE-9 Business Meeting: Session #3
- PAUL OBRIEN (The Aerospace Corporation)
Dr
PAUL OBRIEN
(The Aerospace Corporation)
30/06/2013, 14:00
AP-9, AE-9 International Collaboration
Oral
Dr
PAUL OBRIEN
(The Aerospace Corporation)
30/06/2013, 14:30
AP-9, AE-9 International Collaboration
Oral
Dr
PAUL OBRIEN
(The Aerospace Corporation)
30/06/2013, 15:00
AP-9, AE-9 International Collaboration
Oral
Dr
Sebastien Bourdarie
(ONERA)
30/06/2013, 16:00
AP-9, AE-9 International Collaboration
Oral
Prof.
Ioannis Daglis
(National Observatory of Athens)
30/06/2013, 16:30
AP-9, AE-9 International Collaboration
Oral
Dr
PAUL OBRIEN
(The Aerospace Corporation)
30/06/2013, 17:00
AP-9, AE-9 International Collaboration
Oral
(by Dave Sibeck)
Dr
Sylvie Benck
(Center for Sapce Radiations / UCL)
01/07/2013, 09:00
AP-9, AE-9 International Collaboration
Oral
Accurate measurements of electron and proton fluxes are required for studies of the physical processes that lead to variations of energetic particle spectra at a given position in space, but also for radiation environment modeling and space weather applications. Such measurements can be provided by the Energetic Particle Telescope (EPT) which presently measures energy spectra of electrons (0.5...
Mikhail Rashev
(Max-Planck Institute for Solar System Research)
01/07/2013, 09:30
AP-9, AE-9 International Collaboration
Oral
The RAPID spectrometer for the Cluster mission is an advanced particle detector for the analysis of suprathermal plasma distributions in the energy range from 20-400 keV for electrons, 40-1500 keV (4000 keV) for hydrogen, and 10 keV/nuc - 1500 keV (4000 keV) for heavier ions.
We present data products which can be used in Radiation Belt study and the corresponding caveats.
Our data...
Dr
Alessandro Bruno
(INFN, Bari, Italy)
01/07/2013, 10:00
AP-9, AE-9 International Collaboration
Oral
We present a precise measurement of the under-cutoff proton fluxes with kinetic energy > 63 MeV performed by the PAMELA mission at low Earth orbits (350-610 km). The analyzed proton sample was classified into four categories: stably-trapped protons from the inner radiation belt; quasi-trapped protons near the magnetic equator; short-lived un-trapped protons, spreading over all latitudes; and...
Dr
Daniel Heynderickx
(DH Consultancy BVBA)
01/07/2013, 10:30
AP-9, AE-9 International Collaboration
Oral
Since the beginning of the space age, considerable effort was invested in building models of the trapped proton and electron populations, culminating in the NASA AP-8 and AE-8 models which have been the de facto standards since the seventies. In the intervening years, there have been several new models created, but none with the coverage in energy or space provided by these original models....
Dr
PAUL OBRIEN
(The Aerospace Corporation)
01/07/2013, 11:30
AP-9, AE-9 International Collaboration
