Issue |
A&A
Volume 497, Number 2, April II 2009
|
|
---|---|---|
Page(s) | 551 - 555 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/200811038 | |
Published online | 18 February 2009 |
Sub-hour modulation of non-Io Jovian decametric emission
1
Institute of Radio Astronomy, National Academy of Sciences of Ukraine, Chervonopraporna 4, 61002 Kharkiv, Ukraine e-mail: alexeyarkhipov@rambler.ru
2
Department of Space Radio Physics, Kharkiv V. N. Karazin National University, Svoboda Square 4, 61077 Kharkiv, Ukraine
3
Space Research Institute, Austrian Academy of Sciences, Schmiedlstrasse 6, 8042 Graz, Austria e-mail: rucker@oeaw.ac.at
Received:
25
September
2008
Accepted:
8
January
2009
The variability of Jovian decametric emission (DAM), which is not
controlled by the Io satellite (non-Io), was studied of timescales
of between 1 min and 1 h with DAM records of 1991–2007 from
the archive of Nançay Radio Observatory. We found that the
internal structure of the non-Io radio storms has the dominating
periodicity on of average min . This estimate is in
close agreement with the periodicity of Io-related emission and with
fundamental eigenoscillations of transversal magnetic pulsations in
the Io's plasma torus. The average duration of an arc in non-Io DAM
dynamic spectra was estimated to be
min, although the
most probable value was
min, which corresponds to
Io-related arcs and 3rd and 4th harmonics of torus
proper-oscillations. Our results could be interpreted in terms of
electron acceleration in parallel electric fields of standing
Alfvén waves generated by Io and trapped in the Io torus. This
interpretation agrees with previous arguments that the location of
some sources of non-Io emission are in the magnetic shell of the Io
plasma torus. However, the aurora component of non-Io DAM is not
excluded, since the suggested DAM modulation by the fundamental mode
of eigenoscillations inherent in aurora magnetic-lines is
undetectable in our analysis because of the short duration of non-Io
radio storms.
Key words: planets and satellites: individual: Jupiter / radio continuum: solar system / magnetohydrodynamics (MHD) / waves / radiation mechanisms: non-thermal
© ESO, 2009
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