Solar radio blips and X-ray kernels

Details Solar radio blips and X-ray kernels Solar radio blips and X-ray kernels

May 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.291..210b&link_type=abstract

Nature, vol. 291, May 21-27, 1981, p. 210, 211. Research supported by the Deutsche Forschungsgemeinschaft.

Astronomy and Astrophysics

Astronomy

15

Solar Radio Emission, Solar X-Rays, X Ray Astronomy, High Resolution, Microwave Emission, Oscillographs

Scientific paper

High time resolution measurements from the Effelsberg telescope at 2.8 cm and simultaneous other measurements at decimetric and metric wavelengths indicate that a microwave signal of non-thermal electrons is not to be expected at frequencies below 10 GHz. Previous observations of thermal emission refer then to the hot plasma and not to the fast particles. Decimetric signatures by the ETH Zurich spectrometer prove the presence of non-thermal particles in at least the larger microwave blips.

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