Titlebook: Radio Continua During Solar Flares; Selected Contributio Arnold O. Benz Book 1986 Springer Science+Business Media Dordrecht 1986 Corona.Pla

annexation

A Model of Ultra-Fast Fine Structures of Microwave Bursts electron cyclotron frequency and electron velocity as well as Landau damping and cyclotron damping) to excite the UFFS (Ultra-Fast Fine Structures) of microwave bursts and adopting a nonlinear density wave as a trigger mechanism to explain the millisecond time structure of the UFFS.

战胜

irritation

Radio Observations of the Solar Neutron Flare of 3 June, 1982re had an impulsive character. A strong shock wave (.. ≥ 2.9) was observed unusually soon after the impulsive phase of the flare. The radio spectrum of this event shows that the primary acceleration process probably occurred in the region with an electron density of .. = 4.4 × 10. m.. The pulsations

赦免

讽刺

慢慢啃

The Relation Between Flare-Related Metric Continuum Bursts and Coronal Mass Ejectionsontinuum (FC II) or a Slow Drift Continuum (SDC). Comparing properties for the events it was found that the continuum radio bursts were preferentially associated with the broader, more rapidly moving CME transients.

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信任

Millisecond Radio Spikeservations is summarized and brought into the perspective of recent models. It is concluded that spikes yield a considerable potential for the diagnostics of energetic particles, their origin, and history in astrophysical plasmas.

Cervical-Spine

弯腰

Hollow Beam Distribution of Energetic Electrons and Higher Harmonics of Electron Cyclotron Maserly if 2 ≲ ξ ≲ 2.2 and 3 ≲ ξ ≲ 3.2, respectively, so it would not be a competition in most cases. It is suggested that the ECM emission at these harmonics in .-mode is a possible mechanism to produce solar spike emissions with high brightness temperature at shorter and longer decimetric wavelengths.