Input of the interstellar medium neutrals into cosmic rays - Acceleration by the solar wind turbulence

Details Input of the interstellar medium neutrals into cosmic rays - Acceleration by the solar wind turbulence Input of the interstellar medium neutrals into cosmic rays - Acceleration by the solar wind turbulence

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ge%26ae..33..101p&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 33, no. 1, p. 101-108.

Physics

3

Interplanetary Medium, Interstellar Matter, Magnetohydrodynamic Turbulence, Neutral Gases, Solar Protons, Solar Wind Velocity, Distribution Functions, Photoionization

Scientific paper

Results are presented of calculations of the flow and spatial gradients
of protons formed as a result of hydrogen ionization and accelerated by
small-scale and large-scale solar wind turbulence. It is shown that the
cosmic ray background can be formed by ionized hydrogen in interstellar
space, after its acceleration by large-scale turbulence in solar wind.

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