How Does the Solar Wind Drive Jupiter.s X-ray AuroraquestionMark

The Juno spacecraft.s approach to Jupiter presents the opportunity to utilisesimultaneous remote Xray and in situ observations to address three fundamentalopen questions in Xray and magnetospheric physics: 1) What processes atJupiter.s magnetopause (the source for ions that generate Jupiter.s soft Xrayaurora) drive the Xray emission? 2) What is the nature of the globalinteraction between Jupiter and the solar wind? 3) How does the Xray emissionconnect with UV and Radio emissions? To address these longstanding questions,we propose XMMNewton EPIC and RGS observations of Jupiter during May and June2016 when Juno is in the solar wind and crossing the magnetopause. The nextopportunity to conduct observations like these will not be until 2030. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]