Interstellar Dust in the Solar System
Harald Krueger, Markus Landgraf, Nicolas Altobelli, Eberhard Gruen

TL;DR
This paper reviews in-situ measurements of interstellar dust within the solar system, highlighting Ulysses' data showing a shifted impact direction and discussing the effects of solar forces on dust trajectories.
Contribution
It provides the latest Ulysses interstellar dust data and discusses the observed shift in impact direction compared to the interstellar helium flow.
Findings
Ulysses detected a 30-degree shift in dust impact direction.
Interstellar dust flow is influenced by solar radiation and magnetic fields.
Data from multiple spacecraft extend the understanding of dust distribution.
Abstract
The Ulysses spacecraft has been orbiting the Sun on a highly inclined ellipse almost perpendicular to the ecliptic plane (inclination 79 deg, perihelion distance 1.3 AU, aphelion distance 5.4 AU) since it encountered Jupiter in 1992. The in-situ dust detector on board continuously measured interstellar dust grains with masses up to 10^-13 kg, penetrating deep into the solar system. The flow direction is close to the mean apex of the Sun's motion through the solar system and the grains act as tracers of the physical conditions in the local interstellar cloud (LIC). While Ulysses monitored the interstellar dust stream at high ecliptic latitudes between 3 and 5 AU, interstellar impactors were also measured with the in-situ dust detectors on board Cassini, Galileo and Helios, covering a heliocentric distance range between 0.3 and 3 AU in the ecliptic plane. The interstellar dust stream in…
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