Latitude dependence of co-rotating shock acceleration

Details Latitude dependence of co-rotating shock acceleration Latitude dependence of co-rotating shock acceleration

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..186g&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 186-189 (SEE N85-34729 23-92)

Physics

Energetic Particles, Heliosphere, Latitude, Particle Acceleration, Shock Waves, Flux (Rate), Interplanetary Medium, Voyager 1 Spacecraft, Voyager 2 Spacecraft

Scientific paper

Energetic particle observations in the outer heliosphere (approx 12 A. U.) by the LECP instruments on the Voyager 1 and Voyager 2 spacecraft are discussed that show a definite latitude dependence of the number and intensity of particle enhancements produced by corotating interplanetary regions during an interval when no solar energetic particle events were observed. The particle enhancements are fewer in number and less intense at higher (approx 20 deg.) heliolatitudes. However, the similar spectral shapes of the accelerated particles at the two spacecraft indicate that the acceleration process is the same at the two latitudes, but less intense at the higher latitude.

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