Search Publications

The Contribution of Asteroid Dust to the Interplanetary Dust Cloud: The Impact of ULYSSES Results on the Understanding of Dust Production in the Asteroid Belt and of the Formation of the IRAS Dust Bands
DOI: 10.1006/icar.1996.0059 Bibcode: 1996Icar..120..399M

Mann, Ingrid; Grün, Eberhard; Wilck, Martin

Investigations of the zodiacal dust cloud give evidence for a significant contribution of asteroidal dust to the interplanetary dust cloud, a result which can now be compared to measurements of the ULYSSES dust detector during its passage of the asteroid belt. Especially we discuss the ULYSSES data with respect to the IRAS dust bands and consider …

1996 Icarus
Ulysses 18
The Structure of the Stratospheric Aerosol Layer in the Equatorial and South Polar Regions of Jupiter
DOI: 10.1006/icar.1996.0237 Bibcode: 1996Icar..124..632M

Moreno, Fernando

A one-dimensional code to study the microphysical processes affecting aerosol particles in the jovian stratosphere and upper troposphere has been developed. The algorithms are based on those developed by Turcoet al.(Turco, R. P., P. Hamill, O. B. Toon, R. C. Whitten, and C. S. Kiang 1979.J. Atmos. Sci.36, 699-717) and include the effects of partic…

1996 Icarus
eHST 14
Comet Shoemaker-Levy 9 Dust
DOI: 10.1006/icar.1996.0087 Bibcode: 1996Icar..121..291H

Mumma, Michael J.; Hahn, Joseph M.; Rettig, Terrence W.

Comet Shoemaker-Levy 9 (S-L 9) was imaged with the Hubble Space Telescope from January 1994, through solar opposition on April 29, and until impact in July 1994. As noted by several observers, no anti-sunward dust tails were detected east of the fragments after opposition (D. Jewitt and J. Chen 1994,Periodic Comet Shoemaker-Levy 9(1993e), IAU Circ…

1996 Icarus
eHST 12
The CO Abundance on Neptune from HST Observations
DOI: 10.1006/icar.1996.0140 Bibcode: 1996Icar..123...37C

Strobel, Darrell; Gautier, Daniel; Courtin, Régis

We have marginally detected two CO absorption bands in the UV reflection spectrum of Neptune measured by the HST Faint Object Spectrograph (FOS). They are the (1, 0) and (0, 0) Cameron bands at 1992 and 2063 Å. The interpretation of these features with a radiative transfer model-including Rayleigh, Raman, and particulate scattering processes-impli…

1996 Icarus
eHST 11
Dust Outflow Velocity of Comet Shoemaker-Levy 9
DOI: 10.1006/icar.1996.0086 Bibcode: 1996Icar..121..281R

Hahn, Joseph M.; Rettig, Terrence W.; Sobczak, Gregory J.

Tidal dispersal of the dust comae of the ∼21 fragments of Comet Shoemaker-Levy 9 (S-L 9) became very pronounced in Hubble Space Telescope observations during the weeks prior to impact with Jupiter (T. W. Rettig, J. Hahn, S. C. Tegler, M. Mumma, and M. DiSanti 1994a,Periodic Comet Shoemaker-Levy 9(1993e), IAU Circular 6028; H. A. Weaver plus 20 oth…

1996 Icarus
eHST 6
HST Observation of Mg +in Outburst from Comet D/Shoemaker-Levy 9
DOI: 10.1006/icar.1996.0099 Bibcode: 1996Icar..121..442F

Stern, S. A.; Feldman, P. D.; Weaver, H. A. +1 more

Ultraviolet spectra of fragment G1 of Comet D/Shoemaker-Levy 9 taken 4 days before impact (on 14 July 1994) by the Faint Object Spectrograph of the Hubble Space Telescope show a brief outburst of magnesium ions. The Mg+emission decays back to its quiescent (undetectable) level with a time constant of ∼1 min, consistent with the ions bei…

1996 Icarus
eHST 6
Compositional Mapping of Jupiter's Satellite Io Utilizing High Speed Multifilter Photometry during Mutual Satellite Occultations, 1990-1991
DOI: 10.1006/icar.1996.0179 Bibcode: 1996Icar..123..568N

Lane, Arthur L.; Nelson, Robert M.; Hapke, Bruce W. +4 more

We observed selected mutual occultations of Jupiter's satellites in 1990-1991 at four wavelengths and we used the occultation profiles to constrain the areal distribution of selected spectrally active compounds on Io's surface. We performed high speed photometry of Io at four wavelengths while it was being occulted by another Galilean satellite. T…

1996 Icarus
IUE 0