Spectral Reflectivities of the Galilean Satellites and Titan.

[1]  B. Hapke,et al.  Possible correlation of Io's posteclipse brightening with major solar flares , 1978 .

[2]  F. Witteborn,et al.  Observations of the Near Infrared Spectra of the Galilean Satellites. , 1977 .

[3]  J. Bergstralh,et al.  Io Sodium Emission: 1976 Patrol and Multislit Observations , 1977 .

[4]  D. B. Nash,et al.  Io's surface composition based on reflectance spectra of sulfur/salt mixtures and proton-irradiation experiments , 1977 .

[5]  D. Morrison,et al.  Photometry of the Galilean Satellites , 1977 .

[6]  T. V. Johnson,et al.  Io's surface and the histories of the Galilean satellites , 1977 .

[7]  T. Johnson,et al.  Satellite spectrophotometry and surface compositions , 1977 .

[8]  Aharon Eviatar,et al.  Detection of ionized sulfur in the Jovian magnetosphere , 1976 .

[9]  R. L. Millis,et al.  UBV photometry of the Galilean satellites , 1975 .

[10]  L. Trafton.  Detection of a potassium cloud near Io , 1975, Nature.

[11]  B. Hapke,et al.  Evidence for an Elemental Sulfur Component of the Clouds from Venus Spectrophotometry , 1975 .

[12]  B. Hapke,et al.  Relative Spectrophotometry of Venus from 3067 to 5960 Å , 1975 .

[13]  R. Cess,et al.  Methane absorption in the visible spectra of the outer planets and Titan , 1975 .

[14]  T. Johnson,et al.  Io: A Surface Evaporite Deposit? , 1974, Science.

[15]  D. Morrison,et al.  Four-color photometry of the Galilean satellites , 1974 .

[16]  W. Wamsteker,et al.  On the surface composition of Io , 1974 .

[17]  T. Johnson,et al.  Sodium D-line emission from Io - Sputtering and resonant scattering hypothesis , 1974 .

[18]  D. Morrison,et al.  Physical properties of the natural satellites , 1974 .

[19]  R. L. Younkin.  The Albedo of Titan , 1974 .

[20]  F. Owen,et al.  Surface color variations of the Galilean satellites , 1973 .

[21]  J. Salisbury,et al.  Comparisons of meteorite and asteroid spectral reflectivities , 1973 .

[22]  W. Irvine,et al.  Monochromatic phase curves and albedos for the lunar disk. , 1973 .

[23]  G. Kuiper.  Comments on the Galilean satellites , 1973 .

[24]  S. Ridgway,et al.  Galilean Satellites: Identification of Water Frost , 1972, Science.

[25]  M. Gouterman,et al.  The Spectrum of Sulfur and its Allotropes , 1972 .

[26]  T. McCord,et al.  Spectral geometric albedo of the Galilean satellites - 0.3 to 2.5 . , 1971 .

[27]  T. McCord,et al.  Saturn and its satellites - Narrow-band spectrophotometry, 0.3-1.1 micron , 1971 .

[28]  Larry A. Lebofsky,et al.  Lunar spectral types. , 1971 .

[29]  T. Johnson.  Galilean satellites - Narrowband photometry 0.30 to 1.10 microns , 1971 .

[30]  T. Stroyer‐Hansen,et al.  Color of liquid sulfur , 1970 .

[31]  T. McCord,et al.  Galilean satellites the spectral reflectivity 0.30–1.10 micron☆ , 1970 .

[32]  T. Johnson.  Albedo and spectral reflectivity of the Galilean satellites of Jupiter , 1970 .

[33]  T. McCord,et al.  Time Dependence of Lunar Differential Color , 1969 .

[34]  T. Owen.  An Identification of the 6800-Å Methane Band in the Spectrum of Uranus and a Determination of Atmospheric Temperature , 1966 .

[35]  T. Gehrels,et al.  Wavelength dependence of polarization. iii - the lunar surface. , 1964 .

[36]  J. B. Oke.  Photoelectric Spectrophotometry of Stars Suitable for Standards. , 1964 .

[37]  R. Gurney,et al.  Electronic Processes in Ionic Crystals , 1964 .

[38]  B. Stroemgren.  Problems of internal constitution and kinematics of main sequence stars , 1963 .

[39]  H. Radford,et al.  Green and Purple Sulfur: Electron‐Spin Resonance Studies , 1960 .

[40]  Gerard P. Kuiper,et al.  Titan: a Satellite with an Atmosphere. , 1944 .