%0 Journal Article %1 SMYTHE1995 %A SMYTHE, W. D. %A LOPESGAUTIER, R. %A OCAMPO, A. %A HUI, J. %A SEGURA, M. %A SODERBLOM, L. A. %A MATSON, D. L. %A KIEFFER, H. H. %A MCCORD, T. B. %A FANALE, F. P. %A CALVIN, W. M. %A SUNSHINE, J. %A BARBINIS, E. %A CARLSON, R. W. %A WEISSMAN, P. R. %D 1995 %J Journal of Geophysical Research-Planets %K CALLISTO; DISTRIBUTION; FLOWS; GANYMEDE; IOS LONGITUDINAL REFLECTANCE; SO2; SPECTRA; SULFUR SURFACE; VOLCANISM; VOYAGER-1 %N E9 %P 18957--18972 %T GALILEAN SATELLITE OBSERVATION PLANS FOR THE NEAR-INFRARED MAPPING SPECTROMETER EXPERIMENT ON THE GALILEO SPACECRAFT %V 100 %X On December 7, 1995, the Galileo spacecraft will begin observations of the Jovian system with orbit insertion and a satellite tour of 10 orbits. The Galilean satellites will be observed with four remote sensing instruments spanning the ultraviolet, visible, near infrared, and thermal infrared regions of the spectrum. The Galileo near-infrared mapping spectrometer will observe the satellites in the wavelength range 0.7-5.2 mu m, a region particularly well suited for analyzing volatile components. Planned observations include mapping most available longitudes at about 100-km resolution per pixel at full wavelength resolution, together with observing limited regions at high spatial resolution. The opportunity to affect the choice and design of observations for the Galileo tour ex-tends until June 1996.

@article{SMYTHE1995, abstract = {On December 7, 1995, the Galileo spacecraft will begin observations of the Jovian system with orbit insertion and a satellite tour of 10 orbits. The Galilean satellites will be observed with four remote sensing instruments spanning the ultraviolet, visible, near infrared, and thermal infrared regions of the spectrum. The Galileo near-infrared mapping spectrometer will observe the satellites in the wavelength range 0.7-5.2 mu m, a region particularly well suited for analyzing volatile components. Planned observations include mapping most available longitudes at about 100-km resolution per pixel at full wavelength resolution, together with observing limited regions at high spatial resolution. The opportunity to affect the choice and design of observations for the Galileo tour ex-tends until June 1996.}, added-at = {2009-11-03T20:21:25.000+0100}, author = {SMYTHE, W. D. and LOPESGAUTIER, R. and OCAMPO, A. and HUI, J. and SEGURA, M. and SODERBLOM, L. A. and MATSON, D. L. and KIEFFER, H. H. and MCCORD, T. B. and FANALE, F. P. and CALVIN, W. M. and SUNSHINE, J. and BARBINIS, E. and CARLSON, R. W. and WEISSMAN, P. R.}, biburl = {https://www.bibsonomy.org/bibtex/230a0ecc6decc33a785541f5cdaf47ee1/svance}, citedreferences = {BINZEL RP, 1993, Icarus, V106, P608 ; BLANEY DL, 1995, Icarus, V113, P220 ; BROADFOOT AL, 1979, Science, V204, P979 ; CALVIN WM, 1993, Icarus, V104, P69 ; CALVIN WM, 1995, J GEOPHYS RES-PLANET, V100, P19041 ; CARLSON RW, 1991, Science, V253, P1541 ; CARLSON RW, 1992, SPACE SCI REV, V60, P457 ; CLARK RN, 1993, 93592 US GEOL SURV O ; CLOW GD, 1980, Icarus, V44, P268 ; FANALE FP, 1979, Nature, V280, P761 ; FINK U, 1982, COMETS, P164 ; GOGUEN JD, 1988, Icarus, V76, P465 ; GRADIE J, 1983, LUN PLANET SCI, V14, P255 ; Greenberg R, 1989, NASA SP, V494, P100 ; HANEL R, 1979, Science, V204, P972 ; HAPKE B, 1989, Icarus, V79, P56 ; HOWELL RR, 1984, Icarus, V57, P53 ; JOHNSON TV, 1983, J GEOPHYS RES, V88, P5789 ; JOHNSON TV, 1984, Science, V226, P134 ; JOHNSON TV, 1988, Science, V242, P1280 ; KHANNA RK, 1993, ANAL THERMAL EMISSIO, P54 ; LANE AL, 1981, Nature, V292, P38 ; LELLOUCH E, 1992, Icarus, V98, P271 ; MATSON DL, 1981, J GEOPHYS RES, V86, P1664 ; MATSON DL, 1994, UNPUB GROUNDBASED OB ; MOORE JM, 1986, Icarus, V67, P181 ; MORABITO LA, 1979, Science, V204, P972 ; MURCHIE SL, 1990, J GEOPHYS RES-SOLID, V95, P10743 ; NASH DB, 1987, Icarus, V72, P1 ; NASH DB, 1989, Science, V244, P454 ; NASH DB, 1993, IO INT C SAN JUAN CA, P75 ; NELSON RM, 1980, Science, V210, P784 ; NELSON RM, 1987, Icarus, V72, P358 ; NOLL KS, 1995, J GEOPHYS RES-PLANET, V100, P19057 ; PEARL J, 1979, Nature, V280, P755 ; PIERI DC, 1984, Icarus, V60, P685 ; ROUSH TL, 1990, Icarus, V86, P355 ; SACK NJ, 1992, Icarus, V100, P534 ; SAGAN C, 1979, Nature, V280, P750 ; SALAMA F, 1990, Icarus, V83, P66 ; SALISBURY JW, 1991, INFRARED SPECTRA MIN ; SCHENK PM, 1985, J GEOPHYS RES S, V90, C775 ; SCHENK PM, 1993, J GEOPHYS RES-PLANET, V98, P7475 ; SCHENK PM, 1995, IN PRESS VANNOSTRAND ; SHOEMAKER EM, 1982, SATELLITES JUPITER, P435 ; SMITH BA, 1979, Science, V206, P927 ; SMYTHE WD, 1979, Nature, V280, P766 ; SPENCER JR, 1995, J GEOPHYS RES-PLANET, V100, P19049 ; THOMAS PJ, 1990, J GEOPHYS RES-SOLID, V95, P19161 ; VEEDER GJ, 1994, J GEOPHYS RES, V99, P17095 ; WAMSTEKER W, 1974, Icarus, V23, P417 ; WOLF AA, 1993, AUG ASTR SPEC C VICT ; YOUNG AT, 1984, Icarus, V58, P197}, interhash = {7c3721e127705a1dfc897dcac9263f8e}, intrahash = {30a0ecc6decc33a785541f5cdaf47ee1}, journal = {Journal of Geophysical Research-Planets}, keywords = {CALLISTO; DISTRIBUTION; FLOWS; GANYMEDE; IOS LONGITUDINAL REFLECTANCE; SO2; SPECTRA; SULFUR SURFACE; VOLCANISM; VOYAGER-1}, number = {E9}, owner = {svance}, pages = {18957--18972}, timestamp = {2009-11-03T20:22:15.000+0100}, title = {GALILEAN SATELLITE OBSERVATION PLANS FOR THE NEAR-INFRARED MAPPING SPECTROMETER EXPERIMENT ON THE GALILEO SPACECRAFT}, volume = 100, year = 1995 }