Search Publications

Ulysses observations from pole-to-pole: An introduction
DOI: 10.1029/95GL03556 Bibcode: 1995GeoRL..22.3297S

Smith, Edward J.; Marsden, Richard G.

Recent results from the Ulysses spacecraft as it observed particles and fields above the Sun's south polar cap, returned rapidly across the equator and traversed the northern solar hemisphere are presented in subsequent articles. This introduction provides a brief description of the spacecraft, the experiments, the unique trajectory and highlights…

1995 Geophysical Research Letters
Ulysses 30
Ulysses observations of opposed tilts of solar wind corotating interaction regions in the northern and southern solar hemispheres
DOI: 10.1029/95GL03312 Bibcode: 1995GeoRL..22.3333G

McComas, D. J.; Forsyth, R. J.; Phillips, J. L. +3 more

Data obtained during Ulysses' rapid northbound traverse across the heliographic equator provide evidence for predicted, opposed north-south tilts of corotating interaction regions formed from streams originating in the northern and southern solar hemispheres respectively. In both hemispheres, reverse waves that were propagating poleward were obser…

1995 Geophysical Research Letters
Ulysses 29
The Ulysses south polar pass: Transient fluxes of energetic ions
DOI: 10.1029/95GL02620 Bibcode: 1995GeoRL..22.3369B

Balogh, A.; Forsyth, R. J.; Goldstein, B. E. +5 more

Using Ulysses low energy telescope (LET) measurements of protons and alpha particles with energies of ∼1-5 MeV/n, we present first observations of transient energetic particle events in the high latitude heliosphere. Three transient particle events with gradual onsets and time durations of several days have been identified in the LET data at helio…

1995 Geophysical Research Letters
Ulysses 28
The low radio frequency limit of solar type III bursts: Ulysses observations in and out of the ecliptic
DOI: 10.1029/95GL01717 Bibcode: 1995GeoRL..22.3429L

Hoang, S.; Leblanc, Y.; Dulk, G. A.

We measure the low frequency limit flo of 1028 type III bursts and compare it with the observed plasma frequency at the spacecraft fp. We consider three periods: when Ulysses was in the ecliptic plane near the Sun, far from the Sun, and out of the ecliptic; the average plasma frequency was 20, 10, and 5 kHz respectively. The …

1995 Geophysical Research Letters
Ulysses 26
Abundances of ammonia and carbon disulfide in the Jovian stratosphere following the impact of comet Shoemaker-Levy 9
DOI: 10.1029/95GL01718 Bibcode: 1995GeoRL..22.1625A

Edgington, S. G.; Atreya, S. K.; Trafton, L. M. +3 more

Radiative transfer-scattering models were used to fit the Hubble Space Telescope UV spectroscopic observations of Jupiter taken 2.5 hours after the impact of fragment G of comet P/Shoemaker-Levy 9. They yield abundances for NH3 and CS2 of (0.25-1.3) × 1016cm-2 and (0.43-1.1) × 1015cm-2

1995 Geophysical Research Letters
eHST 26
An intercomparison of plasma turbulence at three comets: Grigg-Skjellerup, Giacobini-Zinner, and Halley
DOI: 10.1029/95GL00806 Bibcode: 1995GeoRL..22.1149T

Glassmeier, K. -H.; Neubauer, F. M.; Tsurutani, Bruce T.

We examine and intercompare the LF plasma wave turbulence at three comets: Grigg-Skjellerup (GS), Giacobini-Zinner (GZ), and Halley (H). All three have power spectral peaks at the local ion cyclotron frequency (the pump wave) at ∼10-2 Hz, and a power-law fall-off at higher frequencies that suggest the development of turbulent cascades […

1995 Geophysical Research Letters
Giotto 25
Latitudinal structure of a coronal mass ejection inferred from Ulysses and Geotail observations
DOI: 10.1029/95GL01016 Bibcode: 1995GeoRL..22.1169H

Balogh, A.; Phillips, J. L.; Gosling, J. T. +7 more

We present the first observations of a CME by two spacecraft separated substantially in heliographic latitude. Ulysses and Geotail both see similar features in the plasma and magnetic field parameters during an interval in which Geotail is located in the deep magnetosheath (>150 RE) and Ulysses is located in the solar wind at 5 AU, ∼…

1995 Geophysical Research Letters
Ulysses 24
Constraints on Solar Wind Acceleration Mechanisms from ULYSSES Plasma Observations: The First Polar Pass
DOI: 10.1029/95GL03532 Bibcode: 1995GeoRL..22.3309B

Phillips, John L.; Barnes, Aaron; Gazis, Paul R.

The mass flux density and velocity of the solar wind at polar latitudes can provide strong constraints on solar wind acceleration mechanisms. We use plasma observations from the first polar passage of the Ulysses spacecraft to investigate this question. We find that the mass flux density and velocity are too high to reconcile with acceleration of …

1995 Geophysical Research Letters
Ulysses 24
Differences between the 0.35-1.0 MeV/nucleon H/He ratio in solar and Co-rotating events at high heliolatitude
DOI: 10.1029/95GL02780 Bibcode: 1995GeoRL..22.3365S

Simnett, G. M.; Roelof, E. C.; Sayle, K. A.

We discuss measurements from the Ulysses spacecraft of the 0.35-1.0 MeV/nucleon H/He intensity ratio at high heliolatitudes. In early 1994 two transient solar events were detected in the gaps between particle intensity increases associated with the passage at low latitude of a co-rotating interaction region. The H/He ratio was ≳ one order-of-magni…

1995 Geophysical Research Letters
Ulysses 19
Tangential discontinuities at high heliographic latitudes (∼-80°)
DOI: 10.1029/95GL02981 Bibcode: 1995GeoRL..22.3409H

Balogh, A.; Tsurutani, B. T.; Goldstein, B. E. +2 more

In this study, tangential discontinuities (TDs) near -80° heliographic latitude have been studied. Based on our quantitative definitions, we find that the TDs may generally be divided into two clear types. There is a distinct population of TDs small (<40°) directional changes. About 19% of all high-latitude TDs are in this category. These types…

1995 Geophysical Research Letters
Ulysses 18