By Mario Livio, Keith Noll, Massimo Stiavelli
Precis of the achievements of the Hubble house Telescope in its first decade of operation.
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Additional resources for A Decade of Hubble Space Telescope Science (2003)(en)(270s)
Gibson, E. , Thomas-Keprta, K. , Romanek, C. , 24 J. F. Bell III: HST studies of Mars Clemett, S. , Chiller, X. D. , Maechling, C. , & Zare, R. N. 1996 Science, 273, 924. McKim, R. 1999 History of Mars Dust Storms. British Astron. Assoc. , Bell III, J. , James, P. B. & Crisp, D. 1998 Geophys. Res. , 25, 611. Moersch, J. E. D. thesis, Cornell University. Morris, R. , Golden, D. , Bell III, J. , H. V. 1995 J. Geophys. , 100, 5319. , & Erard, S. 1993 Icarus, 105, 454. , et al. 2000 Icarus, in press.
Improvement in knowledge of Jupiter’s magnetic ﬁeld geometry. An updated ﬁeld model was constructed by forcing ﬁeld lines from Io’s orbit to pass through the observed latitudes of the footprints. The longitudes were left unconstrained due to uncertainties in both the magnitude of the Alfv´en wing near Io and the travel time of Alfv´en waves from Io to Jupiter. The change in magnetic ﬁeld geometry as a result of ﬁtting to ﬂyby data from the Pioneer and Voyager spacecraft, in addition to ﬁtting WFPC2 and near-IR H+ 3 measured locations of the Io footprint (the VIP4 model, Connerney et al.
James (U. Toledo); D. Crisp and J. Trauger (JPL); P. Smith (LPL), R. T. Clancy (SSI), S. Lee (LASP), M. Mischna (Penn State), and the rest of the WF/PC and WF/PC2 science teams for sharing their results and insights. HST observations of Mars often place substantial demands on both spacecraft and personnel resources. The hard work and dedication of many people have helped to make these observations successful over the past decade. Speciﬁcally, those of us involved in HST Mars science thank the following people for critical support: S.