Jovian Periodicities (~10 h, ~40, 20, 15 min) at ACE, Upstream from the Earth’s Bow Shock, on 25–27 November 2003

It is known that Jovian radio and high energy electron emissions are observed near Earth. The question we address in this study whether the quasi-periodic ~10 h ~40/15–20 min (QP-10 h, QP-40/15–20 min) energetic particle magnetic field periodicities by Ulysses during its distant encounter with Jupiter 2003 were also detectable as far Earth’s orbit. Surprisingly, found at end of extreme Halloween events, times a highly disturbed magnetosphere, inferred from strong bKOM Ulysses, connection Earth suggested simulation results interplanetary (IMF), ACE satellite observed, between least 25–27 November 2013 Lagrangian Point L1 (LPL1), all characteristic periodicities. In particular, using high-time resolution data (1/5 min), found, for first time, quasi-permanent electron, QP-10/5 QP-40 QP-15/20 variations LPL1 three days. These observations reasonably suggest low (~50–~300 keV) electrons reached environment; examined extend lowest limit spectrum 200 keV to ~50 keV. addition, an impressive series (≤0.05 MeV) ion bursts (EIBs) cross-field intensity gradients onset/decay phase events energy-dependent aligned anisotropy suggesting streaming anti-sunward direction their main phase. A comparison simultaneously obtained measurements Geotail upstream bow shock magnetosphere suggests EIBs inconsistent concept terrestrial origin. On contrary, indicate on was spatial effect caused ~10/5 approach large-scale sheet environment. source population forming sharp seems most probably ions accumulated space, although solar contribution possible. Based above results, it reasonable QP-10 due influence. Further research needed cause EIBs. This presents new which our view influence h/QP-40/QP-15/20 outer inner heliosphere 1 AU.