Radio astronomy of the sun has reached a high level of maturity, while radio astronomy of
the stars is now a burgeoning new field of study. The present review is mainly concerned …

We review the physical processes of particle acceleration, injection, propagation, trapping,
and energy loss in solar flare conditions. An understanding of these basic physical …

Few phenomena have stirred the imaginations of solar scientists as much as the explosive
energy of solar flares. In The Physics of Solar Flares, first published in 1988, Einar Tandberg …

Observations and physical concepts are interwoven to give basic explanations of
phenomena and also show the limitations in these explanations and identify some …

Abstract Contents:(1) Introduction.(2) Observational status (solar gamma rays and neutrons):
Identification and analysis of gamma-ray events. Comparison of GRS gamma rays with other …

Incoherent solar radio radiation comes from the free-free, gyroresonance, and
gyrosynchrotron emission mechanisms. Free-free is primarily produced from Coulomb …

We offer a coherent plasma-emission mechanism for intense microwave radiation of a flare
in the impulsive phase. The radiation arises because of a loss-cone instability of plasma …

A numerical investigation is carried out of the gas dynamical response of the solar
atmosphere to a flare energy input in the form of precipitating nonthermal electrons. Rather …

We review recent progress on our understanding of radio emission from solar flares and
coronal mass ejections (CMEs) with emphasis on those aspects of the subject that help us …

Microwave observations with exceptionally high spectral resolution are described for a set of
49 solar flares observed between May and October 1981. Total power data were obtained at …