Hubble Space Telescope and New-Horizons simultaneous observations: Evidence of particle acceleration in the Jovian magnetotail

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The Hubble Space Telescope (HST) observed periodic isolated spots on the Jovian aurora, during the HST-ACS (Advanced Camera of Surveys) 2007 campaign. The auroral spots occurwith 2- to 3- day quasi-periodicity (Figure 1), and they magnetically map to the dawn sector of the magnetosphere. Because of their periodic cycle and observed location, it had been suggested that the polar dawn spots are related to the precipitated, heated plasma during reconnection process taking place in the Jovian magnetotail [1]. The New-Horizons spacecraft traversed the length of the Jovian magnetotail to > 2500 RJ in early 2007. The spacecraft's PEPSSI (Pluto Energetic Particle Spectrometer Science Investigation) instrumentmeasured velocity dispersions, anisotropies and compositional variations in the Jovian magnetotail (> 500 RJ ) with a 3 day periodicity. They reported signatures of energetic particle streaming away from the planet and injection sites in the near-tail region, possibly associated with magnetic reconnection events [2]. In the present study we compare a set of simultaneous HST and New-Horizons observations. During this period HST observes isolated auroral dawn spots and New- Horizons detects energetic ions exhibiting velocity dispersion streaming away from the planet on the same day, evidence of particle acceleration in the Jovian magnetotail. Based on this unique set of simultaneous observations we examine to what extent the Jovian ionosphere is supplied with accelerated plasma from the magnetotail and discuss the properties of the process. References [1] Radioti, A., D. Grodent, J.-C. Ǵerard, B. Bonfond and J.T. Clarke (2008), GRL, 35, L03104, doi:10.1029/2007GL032460. [2] McNutt R. L., Jr. , et al. (2007), Science, 318, 220.

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