Search Publications

The nature of comet Shoemaker-Levy 9 subnuclei from analysis of preimpact Hubble Space Telescope images
DOI: 10.1029/96JE00520 Bibcode: 1996JGR...101.9271R

Mumma, Michael J.; Hahn, Joseph M.; Rettig, Terrence W. +2 more

We obtained Hubble Space Telescope (HST) Wide Field Planetary Camera images of comet Shoemaker-Levy 9 (S-L 9) prior to impact with Jupiter in 1994 to observe the effects of the Jovian gravitational field on the approaching fragments. The HST images were used to monitor the absolute brightness in the central regions of the comae, changes in the sur…

1996 Journal of Geophysical Research
eHST 8
Upstream and downstream propagating waves generated by pickup ions near comet Halley
DOI: 10.1029/96JA01561 Bibcode: 1996JGR...10121627J

Glassmeier, K. -H.; Neubauer, F. M.; Krauklis, I. +3 more

It is well known that most of the Alfvén waves generated in the solar wind by cometary ion pickup are propagating upstream in the solar wind reference frame. However, the magnitude of the small proportion propagating downstream is extremely important because it controls the amount of ion acceleration driven by the second order Fermi process. The v…

1996 Journal of Geophysical Research
Giotto 6
Solar cycle dependence of the solar wind dynamics: Pioneer, Voyager, and Ulysses from 1 to 5 AU
Bibcode: 1996JGR...10124359A

Smith, Edward J.; Américo González-Esparza, J.

1996 Journal of Geophysical Research
Ulysses 6
Magnetic field structure in the comet Grigg-Skjellerup pileup region
DOI: 10.1029/95JA03864 Bibcode: 1996JGR...10111125I

Coates, A. J.; Neubauer, F. M.; Israelevich, P. L. +1 more

The position of the Giotto spacecraft relative to comet Grigg-Skjellerup is found from the draping geometry based on the vector magnetic field data. It is shown that Giotto passed the cometary nucleus on the nightside. The behavior of the magnetic field vectors exhibits two different types in the pileup region. In the outer pileup region, the magn…

1996 Journal of Geophysical Research
Giotto 5
Low-energy particle oscillations and correlations with hydromagnetic waves in the Jovian magnetosphere: Ulysses measurements
DOI: 10.1029/96JA01296 Bibcode: 1996JGR...10117305K

Krupp, N.; Tsurutani, B. T.; Lanzerotti, L. J. +1 more

We report on measurements of energetic particle modulations (ions and electrons with energies E>50 keV) observed by the heliosphere instrument for spectra, composition, and anisotropy at low energies (HI-SCALE) aboard the Ulysses spacecraft that were associated with the only hydromagnetic (HM) wave event measured inside the Jovian magnetosphere…

1996 Journal of Geophysical Research
Ulysses 4
Ulysses observations of corotation lags in the dayside Jovian magnetosphere: An evaluation of the hinged magnetodisc and magnetic anomaly models
DOI: 10.1029/96JA02042 Bibcode: 1996JGR...10121439H

Dougherty, Michele K.; Phillips, John L.; Hoogeveen, Gary W.

Ulysses observations during the inbound leg of the February 1992 encounter with Jupiter offer the opportunity to evaluate both the hinged magnetodisc and the magnetic anomaly models currently used to describe the Jovian magnetospheric corotation lag. Particle and field detectors on board Ulysses measure signatures of the current and plasma sheets.…

1996 Journal of Geophysical Research
Ulysses 1
D/H and O-18/O-16 ratio in the hydronium ion and in neutral water from in situ ion measurements in comet Halley
DOI: 10.1029/94JA02936 Bibcode: 1995JGR...100.5827B

Altwegg, K.; Balsiger, H.; Geiss, J.

The D/H ratio and the O-18/O-16 ratio in hydronium ions in the gas coma of comet Halley have been determined from ion data obtained by the high intensity sensor (HIS) of the ion spectometer (IMS) on board the spacecraft Giotto in 1986. The HIS instrument measured the reliable data for the water group ions over a large distance range from the nucle…

1995 Journal of Geophysical Research
Giotto 155
Ulysses observations of microstreams in the solar wind from coronal holes
DOI: 10.1029/95JA02723 Bibcode: 1995JGR...10023389N

Balogh, A.; McComas, D. J.; Goldstein, B. E. +2 more

During its south polar passage in 1994, the Ulysses spacecraft continuously sampled the properties of the solar wind emanating from the south polar coronal hole. At latitudes poleward of ~-60°, the solar wind speed had an average value of 764 km/s and a range of 700-833 km/s. The principal variations in the vector velocity were associated with eit…

1995 Journal of Geophysical Research
Ulysses 99
Ulysses observation of a noncoronal mass ejection flux rope: Evidence of interplanetary magnetic reconnection
DOI: 10.1029/95JA01123 Bibcode: 1995JGR...10019903M

Balogh, A.; McComas, D. J.; Forsyth, R. J. +5 more

A well-defined, small-scale (~0.05 AU) magnetic flux rope was observed by Ulysses at about 5 AU in close proximity to a heat flux dropout (HFD) at the heliospheric current sheet (HCS). This magnetic flux rope is characterized by a rotation of the field in the plane approximately perpendicular to the ecliptic (and containing the Sun and the spacecr…

1995 Journal of Geophysical Research
Ulysses 96
C+ pickup ions in the heliosphere and their origin
DOI: 10.1029/95JA03051 Bibcode: 1995JGR...10023373G

Geiss, J.; Gloeckler, G.; Fisk, L. A. +1 more

C+ pickup ions were discovered with the solar wind ion composition spectrometer flying on Ulysses. Whereas the other nonlocally occurring pickup ions are produced from the interstellar gas penetrating deep into the heliosphere, C+ comes from an ``inner source'' which is located at a solar distance of a few AU and extends over…

1995 Journal of Geophysical Research
Ulysses 96