In situ satellite observations of type III burst exciters at 1 AU show that the beam does not evolve into a plateau in velocity space, contrary to the prediction quasilinear theory. The observations can be explained by a theory that includes mode coupling effects due to excitation of the parametric
Relative timing of microwave bursts and metric type III bursts. Implication on the energy of type III burst exciter
β Scribed by A. Raoult; E. Correla; P. Lantos; P. Kaufmann; K. L. Klein; G. Genouillac
- Publisher
- Springer
- Year
- 1989
- Tongue
- English
- Weight
- 673 KB
- Volume
- 120
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
With 13 figurcs. (Keccived 1965 July 15) Thc phenomenological features of type V radiation arc discussed a t the basis of fine structure rccords taken a t the Astrophysical Observatory Potsdam since 1958. A phenomenological subclassification is derived from the various forms of appearance. It is bel
The time profile of two sets of isolated type III bursts, observed in the meter wavelength range at the Trieste Astronomical Observatory, was analyzed using a Fourier transform technique in order to accurately determine the decay constant of the exponential phase and to derive the exciter time profi
The suggestion is explored that the two-stream instability has little effect on the propagation of the electron streams which generate type III bursts because the time required (tO for development of the instability is comparable with or greater than the time available (At) for growth of the waves.
We compare evidence of coronal magnetic fields from polarized metric type III radio bursts with (a) global potential field models, (b) direct averages of the observed photospheric magnetic field, and (c) Ha synoptic charts. The comparison clearly indicates both that the principal aspects of type III