The trapped He flux dynamics observed on the TSUBASA satellite

Details The trapped He flux dynamics observed on the TSUBASA satellite The trapped He flux dynamics observed on the TSUBASA satellite

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsm51a0515m&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SM51A-0515

Physics

2118 Energetic Particles, Solar, 2720 Energetic Particles, Trapped, 2730 Magnetosphere: Inner, 6060 Radiation And Spectra

Scientific paper

TSUBASA satellite was launched on February 2002. TSUBASA is placed in a geostationary transfer orbit having roughly a perigee of 500 km, an apogee of 37,000km, a 28.5 inclination, and a 645 minute period. The Standard Dose Monitor (SDOM) onboard TSUBASA has carried out measurements of energetic electrons, protons, and alpha particles. He flux distribution greatly changed the substorm on April 19, 2001 event for the boundary. Possible source of the fluxes including remnants of solar particle population trapped during substroms, acceleration of hot plasma from the outer magnetosphere, and pitch-angle scattering from the top of the magnetic field line are discussed.

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