Observations of high energy primary electrons and their astrophysical significance
- 1 January 1997
- journal article
- Published by Elsevier in Advances In Space Research
- Vol. 19 (5) , 767-770
- https://doi.org/10.1016/s0273-1177(96)00144-5
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Very low braking index for the Vela pulsarNature, 1996
- ROSAT Survey Observations of the Monogem RingThe Astrophysical Journal, 1996
- ROSAT PSPC observations of the remnant of SN 1006Monthly Notices of the Royal Astronomical Society, 1996
- Evidence for shock acceleration of high-energy electrons in the supernova remnant SN1006Nature, 1995
- The inverse Compton scattering of cosmic ray electrons in the GalaxyMonthly Notices of the Royal Astronomical Society, 1991
- The energy spectrum of electrons and cosmic-ray confinement A new measurement and its interpretationThe Astrophysical Journal, 1984
- Earth's magnetic field as a radiator to detect cosmic ray electrons of energy >1012eVJournal of Geophysical Research, 1983
- Emulsion chamber observations of primary cosmic-ray electrons in the energy range 30-1000 GeVThe Astrophysical Journal, 1980
- Are Cosmic Electrons Anisotropic?The Astrophysical Journal, 1969
- Electron Component of the Primary Cosmic Radiation at Energies ≳15 GeVPhysical Review Letters, 1965