Solar radio bursts and acceleration processes of energetic protons.

Details Solar radio bursts and acceleration processes of energetic protons. Solar radio bursts and acceleration processes of energetic protons.

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acaps..15..350l&link_type=abstract

Acta Astrophys. Sin., Vol. 15, No. 4, p. 350 - 358

Astronomy and Astrophysics

Astrophysics

Solar Radio Bursts: Particle Acceleration, Solar Protons: Solar Flares

Scientific paper

According to the data analysis of recent observations of solar radio bursts recorded by ground-based radio telescopes and solar proton streams by spaceborne instruments, it is shown in this paper: (1) the occurrences of solar proton events (or proton flares) are closely associated with abruptly fluctuating strong type IVμ bursts (or microwave impulsive bursts) or strong short decimetric-wave bursts. (2) About 24% - 30% of the proton events occur without associated type II bursts. This paper also argues that both energetic electrons (±500 keV) which generate strong type IVμ bursts and energetic protons (>10 MeV) in proton flares are accelerated by the stochastic MHD turbulences in the same magnetic loop during the impulsive phase of solar flares.

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