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Five populations of interplanetary meteoroids
DOI: 10.1029/93JE01203 Bibcode: 1993JGR....9817029D

Divine, Neil

A description of the interplanetary meteoroid environment is proposed in terms of distinct populations, each of which has separable distributions in particle mass and in orbital inclination, eccentricity, and perihelion distance. This treatment leads to expressions for particle concentration and flux which explicitly incorporate both Keplerian dyn…

1993 Journal of Geophysical Research
Ulysses 184
A survey of low frequency waves at Jupiter: The Ulysses encounter
DOI: 10.1029/93JA02586 Bibcode: 1993JGR....9821203T

Tsurutani, Bruce T.; Smith, Edward J.; Balogh, Andre +1 more

We report the results of a survey of low-frequency (LF) plasma waves detected during the Ulysses Jupiter flyby. In the Jovian foreshock, two predominant wave periods are detected: 102-s and 5-s, as measured in the spacecraft frame. The 102-s waves are highly nonlinear propagate at large angles to B\searrow0 (typica…

1993 Journal of Geophysical Research
Ulysses 71
Detection of the local interstellar cloud from high-resolution spectra of nearby stars: Inferences on the heliospheric interface
DOI: 10.1029/93JA01179 Bibcode: 1993JGR....9815193B

Ferlet, R.; Vidal-Madjar, A.; Lallement, R. +1 more

High-resolution spectroscopic observations of the local interstellar medium between the Sun and nearby stars have been recorded with the Aurelie spectrometer of the Observatoire de Haute Provence (France). They have been used to identify and characterize the local interstellar cloud (LIC) in which the Sun is embedded. The ``Doppler triangulation''…

1993 Journal of Geophysical Research
Ulysses 60
Low-frequency electromagnetic plasma waves at comet P/Grigg-Skjellerup: Overview and spectral characteristics
DOI: 10.1029/93JA02583 Bibcode: 1993JGR....9820921G

Neubauer, Fritz M.; Glassmeier, Karl-Heinz

Large-amplitude electromagnetic plasma waves are one of the dominant features of the solar wind-comet interaction. Wave characteristics strongly depend on parameters such as the solar wind flow and Alfvén velocities and the angle between flow and interplanetary magnetic field as well as the production rate. With respect to the latter the flyby of …

1993 Journal of Geophysical Research
Giotto 58
Mirror modes and fast magnetoacoustic waves near the magnetic pileup boundary of comet P/Halley
DOI: 10.1029/93JA02582 Bibcode: 1993JGR....9820955G

Motschmann, Uwe; Neubauer, Fritz M.; Fuselier, S. A. +4 more

Large-amplitude ultralow-frequency wave structures observed on both sides of the magnetic pileup boundary of comet P/Halley during the flyby of the Giotto spacecraft have been analyzed using suprathermal electron density and magnetic field observations. Upstream of the boundary, electron density and magnetic field magnitude variations are anticorr…

1993 Journal of Geophysical Research
Giotto 58
Velocity space diffusion and nongyrotropy of pickup water group ions at comet Grigg-Skjellerup
DOI: 10.1029/93JA02535 Bibcode: 1993JGR....9820985C

Coates, A. J.; Neubauer, Fritz M.; Wilken, B. +1 more

The diffusion of water group cometary ions in velocity space at comet Grigg-Skjellerup was measured during the Giotto spacecraft encounter. The evolution of the collapsed pitch angle and energy distributions during the inbound and outbound passes shows that the timescale for energy diffusion may be similar to that for pitch angle diffusion. Fully …

1993 Journal of Geophysical Research
Giotto 57
Morphology and time variation of the Jovian far UV aurora: Hubble Space Telescope observations
DOI: 10.1029/93JE01334 Bibcode: 1993JGR....9818793G

Paresce, Francesco; Prange, Renee; Gerard, Jean-Claude +1 more

High spatial resolution images of the north polar region of Jupiter have been obtained with the Faint Object Camera on board the Hubble Space Telescope. The first set of two images collected 87 min apart in February 1992 shows a bright (≃180 kR) emission superimposed on the background in rotation with the planet. Both Ly α images show common regio…

1993 Journal of Geophysical Research
eHST 55
The dusty ballerina skirt of Jupiter
DOI: 10.1029/93JA02588 Bibcode: 1993JGR....9821245H

Horanyi, M.; Gruen, E.; Morfill, G.

We suggest a model to explain the unexpected recurrent dust events that were observed during the Jupiter encounter by the dust detector on board the Ulysses spacecraft. This model is based on dust-magnetosphere interactions. Dust particles inside the Jovian magnetosphere collect electrostatic charges and their interaction with the magnetic and ele…

1993 Journal of Geophysical Research
Ulysses 53
Bernstein waves in the Io plasma torus: A novel kind of electron temperature sensor
DOI: 10.1029/93JA02587 Bibcode: 1993JGR....9821163M

Moncuquet, Michel; Meyer-Vernet, Nicole; Hoang, Sang

During Ulysses passage through the Io plasma torus, along a basically north-to-south trajectory crossing the magnetic equator at R~7.8 RJ from Jupiter, the Unified Radio and Plasma Wave experiment observed weakly banded emissions with well-defined minima at gyroharmonics. These noise bands are interpreted as stable electrostatic fluctua…

1993 Journal of Geophysical Research
Ulysses 52
Correlated variations of UV and radio emissions during an outstanding Jovian auroral event
DOI: 10.1029/93JE01802 Bibcode: 1993JGR....9818779P

Moos, H. W.; Bame, S. J.; Zarka, P. +6 more

An exceptional Jovian aurora was detected in the FUV on December 21, 1990, by means of Vilspa and Goddard Space Flight Center (GFSC) International Ultraviolet Explorer (IUE) observations. This event included intensification by a factor of three between December 20 and 21, leading to the brightest aurora identified in the IUE data analyzed, and, in…

1993 Journal of Geophysical Research
IUE Ulysses 50