ELECTRON-CYCLOTRON MASER EMISSION AT OBLIQUE ANGLES

Citation
Db. Melrose et Ga. Dulk, ELECTRON-CYCLOTRON MASER EMISSION AT OBLIQUE ANGLES, Planetary and space science, 41(5), 1993, pp. 333-339
Citations number
29
Categorie Soggetti
Geosciences, Interdisciplinary
Journal title
ISSN journal
00320633
Volume
41
Issue
5
Year of publication
1993
Pages
333 - 339
Database
ISI
SICI code
0032-0633(1993)41:5<333:EMEAOA>2.0.ZU;2-3
Abstract
Observations of elliptically polarized bursts of decametric radio emis sion from Jupiter with axial ratios of the polarization ellipse 0.2 le ss than or similar T less than or similar 0.7 imply emission at angles 45-degrees- less than or similar theta less than or similar 80-degree s to the magnetic field. Emission at oblique angles less than or simil ar 60-degrees is not expected in the conventional theory of electron c yclotron maser emission. It is argued that electron cyclotron emission at a given theta requires electrons with parallel velocity concentrat ed around upsilon(parallel-to) = upsilon cos alpha = c cos theta. A me chanism is proposed that might produce an appropriate ''spiraling beam '' distribution, with a peak in velocity space at speed upsilon = upsi lon0 and pitch angle alpha = alpha0 not-equal 0.