There are theoretical and experimental arguments for a modulation of Jovian decametric S-emission by standing Alfvén waves in the regions of radio sources. One effect of such modulation is the concentration of S-burst emission around certain frequencies (S-bands) in dynamic spectra of radio emission. It is argued that S-bands are generated at the local electron cyclotron frequencies, around nodes of a standing Alfvén wave. To test this hypothesis, we derived several verifiable predictions: the anti-correlation of radio-flux in adjacent S-bands at short time scales (<0.1 s); the correlation of frequency shifts of S-bands at long time scales (>0.1 s); and the transformation of the broadband S-storm into S-bands. We searched for and found thes...
The variability of Jovian decametric emission (DAM) is studied at time scales from 1 min to 1 h with...
International audienceThe Io-Jupiter S-bursts are series of quasi-periodic impulsive decameter radio...
The variability of Jovian decametric emission (DAM), which is not controlled by the Io satellite (no...
The new mechanism for the formation of a fine structure in the dynamic spectra of the Jovian decamet...
Short (S) bursts and narrow-band events (NB) of Jovian decametric emission (DAM) form oscillating ba...
International audienceJupiter's radio emissions are dominated in intensity by decametric radio emiss...
Short (S-) bursts of Jovian decametric emission show random behavior with very complicated forms in ...
We present an analysis of several Jovian Io-related decametric radio storms recorded in 2004−2012 at...
Narrow-band (NB) events in dynamic spectra and their relation with short (S-) bursts are an unresolv...
System of periodic peaks is found in the power spectra of ULF flux oscillations of Jovian decametric...
The flux variability of Jovian decametric radio emission (DAM) is analyzed to search for its possibl...
International audienceJupiter's radio emissions are dominated in intensity by decametric radio emiss...
International audienceJovian millisecond (or S-) bursts are intense impulsive decametric radio burst...
International audienceWe analyze the records of Jupiter's decameter radio emissions obtained during ...
S-component of the sporadic radio emission of Jupiter decameter emission (DAM) is an extraordinary a...
The variability of Jovian decametric emission (DAM) is studied at time scales from 1 min to 1 h with...
International audienceThe Io-Jupiter S-bursts are series of quasi-periodic impulsive decameter radio...
The variability of Jovian decametric emission (DAM), which is not controlled by the Io satellite (no...
The new mechanism for the formation of a fine structure in the dynamic spectra of the Jovian decamet...
Short (S) bursts and narrow-band events (NB) of Jovian decametric emission (DAM) form oscillating ba...
International audienceJupiter's radio emissions are dominated in intensity by decametric radio emiss...
Short (S-) bursts of Jovian decametric emission show random behavior with very complicated forms in ...
We present an analysis of several Jovian Io-related decametric radio storms recorded in 2004−2012 at...
Narrow-band (NB) events in dynamic spectra and their relation with short (S-) bursts are an unresolv...
System of periodic peaks is found in the power spectra of ULF flux oscillations of Jovian decametric...
The flux variability of Jovian decametric radio emission (DAM) is analyzed to search for its possibl...
International audienceJupiter's radio emissions are dominated in intensity by decametric radio emiss...
International audienceJovian millisecond (or S-) bursts are intense impulsive decametric radio burst...
International audienceWe analyze the records of Jupiter's decameter radio emissions obtained during ...
S-component of the sporadic radio emission of Jupiter decameter emission (DAM) is an extraordinary a...
The variability of Jovian decametric emission (DAM) is studied at time scales from 1 min to 1 h with...
International audienceThe Io-Jupiter S-bursts are series of quasi-periodic impulsive decameter radio...
The variability of Jovian decametric emission (DAM), which is not controlled by the Io satellite (no...