Radio waves in the heliosphere

Details Radio waves in the heliosphere Radio waves in the heliosphere

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..191b&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 13, no. 6, p. 191-203.

Physics

1

Energetic Particles, Heliosphere, Plasma Waves, Shock Wave Propagation, Solar Radio Emission, Ulysses Mission, Electron Plasma, In Situ Measurement, Interplanetary Medium, Radio Waves

Scientific paper

Solar radio emissions at long wavelengths (wavelengths greater than 10 m or frequencies smaller than 30 MHz) are produced in the upper corona and in the interplanetary medium (the Heliosphere), sometimes at very large distances from the sun, up to the orbit of Jupiter and beyond. Solar radio emissions are produced by the passage of energetic particles and shock waves; they provide a unique means to detect perturbations originating from the solar activity and to track their progression through the interplanetary medium. Different aspects of current research are presented, essentially based on results of the URAP investigation on ULYSSES.

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