๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Harmonic ratios of inverted-U type III bursts

โœ Scribed by R. T. Stewart


Publisher
Springer
Year
1974
Tongue
English
Weight
381 KB
Volume
39
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Harmonic structure of type IIIb and III
โœ E. P. Abranin; L. L. Baselyan; N. Yu. Goncharov; V. A. Zinichev; V. O. Rapoport; ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 349 KB

A decameter solar radio storm of type IIIb and III bursts has been analysed, using single frequency records at frequencies 12.5 and 25.0 MHz. Several kinds of burst associations are classified. As a result it is shown that in double oblique burst-traces of type IIIb +III on the frequency-time plane

Pairs of non fundamental-harmonic type I
โœ C. Caroubalos; J. Heyvaerts; M. Pick; G. Trottet ๐Ÿ“‚ Article ๐Ÿ“… 1974 ๐Ÿ› Springer ๐ŸŒ English โš– 512 KB

Different forms of pairs of type III bursts have been discussed in the literature. We report here a new aspect revealed by high time resolution radioheliography. In some groups of these bursts, each element appears to be split into two components. These pairs recur with a characteristic time, and in

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.

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,

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