1997
DOI: 10.1006/icar.1997.5789
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South–North and Radial Traverses through the Interplanetary Dust Cloud

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Cited by 117 publications
(106 citation statements)
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References 28 publications
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“…Staubach (Staubach et al 1996;Grün et al 1997) upgraded Divine's model using new data from GALILEO and ULYSSES dust detectors. Solar radiation pressure was added as a second perturbation force and an additional population, Inter Stellar Dust (ISD), was implemented.…”
Section: Model Descriptionmentioning
confidence: 99%
“…Staubach (Staubach et al 1996;Grün et al 1997) upgraded Divine's model using new data from GALILEO and ULYSSES dust detectors. Solar radiation pressure was added as a second perturbation force and an additional population, Inter Stellar Dust (ISD), was implemented.…”
Section: Model Descriptionmentioning
confidence: 99%
“…About 30 years ago, analysis of the data obtained with the dust instruments flown on a couple of spacecraft suggested that ISD grains can cross the heliospheric boundary and penetrate deeply into the heliosphere (Bertaux and Blamont 1976;Wolf et al 1976). In the 1990s, this was undoubtedly demonstrated with the dust instrument carried by the Ulysses spacecraft: the Ulysses dust detector, which measured mass, speed and approach direction of the impacting grains, identified ISD grains with radius above 0.1 µm sweeping through the heliosphere (Grün et al 1993(Grün et al , 1994.…”
Section: Introductionmentioning
confidence: 99%
“…The motion of the interstellar grains through the solar system was parallel to the flow of neutral interstellar hydrogen and helium gas, both traveling at a speed of 26 km s −1 (Baguhl et al 1995). The interstellar dust flow persisted at higher latitudes above the ecliptic plane, even over the poles of the Sun, whereas interplanetary dust is strongly depleted away from the ecliptic plane (Grün et al 1997).…”
Section: Large Interstellar Dust Grains In the Heliospherementioning
confidence: 98%
“…The Ulysses spacecraft detected impacts predominantly from a direction that was opposite to the expected impact direction of interplanetary dust grains. It was found that, on average, the impact velocities exceeded the local solar system escape velocity (Grün et al 1994). The motion of the interstellar grains through the solar system was parallel to the flow of neutral interstellar hydrogen and helium gas, both traveling at a speed of 26 km s −1 (Baguhl et al 1995).…”
Section: Large Interstellar Dust Grains In the Heliospherementioning
confidence: 99%