Ionization states and the origin of low energy /1-30 MeV/amu/ cosmic ray nuclei

Details Ionization states and the origin of low energy /1-30 MeV/amu/ cosmic ray nuclei Ionization states and the origin of low energy /1-30 MeV/amu/ cosmic ray nuclei

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ijrsp...6..218d&link_type=abstract

(Space Sciences Symposium, Trivandrum, India, Jan. 18-21, 1977.) Indian Journal of Radio and Space Physics, vol. 6, Sept. 1977,

Physics

Nuclear Physics

Cosmic Rays, Electron States, Ionization Potentials, Nuclei (Nuclear Physics), Abundance, Interplanetary Medium, Interstellar Space, Particle Energy

Scientific paper

The origin and the ionization states of the anomalous component of cosmic-ray nuclei in the energy region from 1 to 30 MeV/amu recently observed in interplanetary space are investigated in detail. It was assumed that this component originated from nearby sources, e.g., from nova-type explosions (which have peculiar C, N, and O compositions) and are further accelerated in the interplanetary medium. Modulation of these ions is also calculated, and a comparison is made of the demodulated composition of C-Si ions with available abundance data for some novae.

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