Response of Jupiter’s UV auroras to interplanetary conditions as observed by the Hubble Space Telescope during the Cassini fly-by campaign

نویسندگان

  • J. D. Nichols
  • E. J. Bunce
  • J. T. Clarke
  • S.W.H. Cowley
  • J.-C. Gérard
  • D. Grodent
  • W. R. Pryor
چکیده

s, p. 129, University of Leicester, Leicester, UK. Grodent, D., J.T. Clarke, J.H. Waite Jr., S.W.H. Cowley, J.-C. Gérard, and J. Kim (2003a), Jupiter’s695polar auroral emissions, J. Geophys. Res., 108(A10), 1366, doi:10.1029/2003JA010017. Grodent, D., J.T. Clarke, J. Kim, J.H. Waite Jr, and S.W.H. Cowley (2003b), Jupiter’s main ovalobserved with HST-STIS, J. Geophys. Res., 108(A11), 1389, doi:10.1029/2003JA009921.700Grodent, D., J.-C. Gérard, J.T. Clarke, G.R. Gladstone, and J.H. Waite Jr. (2004), A possibleauroral signature of a magnetotail reconnection process on Jupiter, J. Geophys. Res., 109,A05201, doi:10.1029/2003JA010341.

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تاریخ انتشار 2006