๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Type III solar radio bursts and the fundamental-harmonic hypothesis

โœ Scribed by Hans Rosenberg


Publisher
Springer
Year
1975
Tongue
English
Weight
686 KB
Volume
42
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Type III solar radio bursts and the fund
โœ Hans Rosenberg ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 28 KB

## Discussion D. Smith: I know spontaneous emission maximizes at about 90 ~ However, if B is present, amplification maximizes at about 0 ~ with respect to B. Rosenberg: No. D. Smith: According to Yip the growth rate maximizes along the magnetic field. Rosenberg" Direction of B does not make that

Fundamental and harmonic radiation in so
โœ S. F. Smerd ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 583 KB

There are three kinds of observations that provide indirect evidence for the contentions that (a) some type III radiation is fundamental radiation; and (b) type III's are at times emitted simultaneously as fundamental and second-harmonic plasma radiation.

Fundamental wave of type III solar radio
โœ T. Takakura ๐Ÿ“‚ Article ๐Ÿ“… 1982 ๐Ÿ› Springer ๐ŸŒ English โš– 549 KB

It is demonstrated by a numerical simulation that both the whistler waves and plasma waves are excited by a common solar electron beam. The excitation of the whistler waves is ascribed to the loss-cone distribution which arises at a later phase of the passage of the beam at a given height due to a v

Generation of solar type III bursts at t
โœ P. J. Kellogg; R. P. Lin ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 47 KB

Using the data from our experiments on the IMP-6 (Explorer 43) satellite, we have examined over 200 type III bursts at kilometric wavelengths, including 16 bursts which were accompanied by >18 keV electron events with sharp onsets, in a search for the electrostatic waves which, according to theory,

Harmonic relation of type IIIb-III solar
โœ E. P. Abranin; L. L. Bazelyan; Ya. G. Tsybko ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Springer ๐ŸŒ English โš– 259 KB

This study of type IIIb-III events strongly supports their interpretation as fundamental-harmonic burst pairs. Type IIIb chains and the related type III bursts drift from 12.5 to 6.25 MHz and from 25.0 to 12.5 MHz, respectively, during similar time intervals of 11.1 and 11.0 s, on the average. This