Yu-Qing Lou, Huagang Song, Yinyu Liu, Meng Yang
In reference to Jupiter south polar quasi-periodic 40-50 min (QP-40)
activities and the model scenario for global QP-40 oscillations of the Jovian
inner radiation belt (IRB), we validate relevant predictions and confirmations
by amassing empirical evidence from Ulysses, Cassini, Chandra, Galileo,
XMM-Newton, and Advanced Composition Explorer for Jupiter north polar QP-40
activities. We report ground 6cm radio observations of Jupiter by Urumqi 25m
telescope for synchrotron intensity bursty variations of the Jovian IRB and
show their likely correlations with the recurrent arrival of high-speed solar
winds at Jupiter.
View original:
http://arxiv.org/abs/1201.1194
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