dc.contributor.author |
Gopalswamy, N |
|
dc.date.accessioned |
2009-02-02T17:01:48Z |
|
dc.date.available |
2009-02-02T17:01:48Z |
|
dc.date.issued |
1986-06 |
|
dc.identifier.citation |
Earth Moon, and Planet, Vol. 35, No. 2, pp. 93 - 115 |
en |
dc.identifier.issn |
0167-9295 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4309 |
|
dc.description.abstract |
The shadow events in the dynamic spectra of Jovian decametric emission are explained as the result of interaction between electron bunches responsible for S and L emissions. The relevant dispersion relation is derived for the fast extraordinary mode in the cold magnetospheric plasma in the presence of S and L electron bunches. The growth rate of the synchrotron maser instability is studied in the presence and absence of S-electrons. It is shown that the synchrotron maser instability responsible for L-emission can be temporarily quenched by the invasion of S-electrons, thereby stopping the L-emission. The theory accounts for various observed features of the shadow events. |
en |
dc.language.iso |
en |
en |
dc.publisher |
D. Reidel Publishing Co. |
en |
dc.relation.uri |
http://dx.doi.org/10.1007/BF00117270 |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/1986EM%26P...35...93G |
en |
dc.subject |
Jupiter Atmosphere |
en |
dc.subject |
Planetary Radiation |
en |
dc.subject |
Planetology |
en |
dc.subject |
Space Plasmas |
en |
dc.subject |
Synchrotron Radiation |
en |
dc.subject |
Decametric Waves |
en |
dc.subject |
Electron Bunching |
en |
dc.subject |
Maser Outputs |
en |
dc.subject |
Planetary Magnetospheres |
en |
dc.subject |
Superhigh Frequencies |
en |
dc.subject |
Ultrahigh Frequencies |
en |
dc.title |
A theory of Jovian shadow bursts |
en |
dc.type |
Article |
en |