FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2023474018> ?p ?o ?g. }

• W2023474018 endingPage "356" @default.
• W2023474018 startingPage "347" @default.
• W2023474018 abstract "In the early 1990s, after its Jupiter flyby, the Ulysses spacecraft identified interstellar dust in the solar system. Since then the in-situ dust detector on board Ulysses continuously monitored interstellar grains with masses up to 10−13 kg, penetrating deep into the solar system. While Ulysses measured 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 the inner solar system is altered by the solar radiation pressure force, gravitational focussing and interaction of charged grains with the time varying interplanetary magnetic field. The grains act as tracers of the physical conditions in the local interstellar cloud (LIC). Our in-situ measurements imply the existence of a population of ‘big’ interstellar grains (up to 10−13 kg) and a gas-to-dust-mass ratio in the LIC which is a factor of 1.5–2 larger than the one derived from astronomical observations, indicating a concentration of interstellar dust in the very local interstellar medium. Until 2004, the interstellar dust flow direction measured by Ulysses was close to the mean apex of the Sun’s motion through the LIC, while in 2005, the data showed a 30° shift, the reason of which is presently unknown. We review the results from spacecraft-based in-situ interstellar dust measurements in the solar system and their implications for the physical and chemical state of the LIC." @default.
• W2023474018 created "2016-06-24" @default.
• W2023474018 creator A5069923642 @default.
• W2023474018 creator A5076519013 @default.
• W2023474018 date "2008-09-26" @default.
• W2023474018 modified "2023-10-12" @default.
• W2023474018 title "Interstellar Dust Inside and Outside the Heliosphere" @default.
• W2023474018 cites W1567986462 @default.
• W2023474018 cites W1594079022 @default.
• W2023474018 cites W1623532745 @default.
• W2023474018 cites W1967403974 @default.
• W2023474018 cites W1978662015 @default.
• W2023474018 cites W1982331924 @default.
• W2023474018 cites W1992639143 @default.
• W2023474018 cites W1997423946 @default.
• W2023474018 cites W2000629565 @default.
• W2023474018 cites W2001205957 @default.
• W2023474018 cites W2003160727 @default.
• W2023474018 cites W2004118030 @default.
• W2023474018 cites W2008837559 @default.
• W2023474018 cites W2010328731 @default.
• W2023474018 cites W2010578069 @default.
• W2023474018 cites W2010848361 @default.
• W2023474018 cites W2012850863 @default.
• W2023474018 cites W2014144733 @default.
• W2023474018 cites W2019579421 @default.
• W2023474018 cites W2025948394 @default.
• W2023474018 cites W2027806272 @default.
• W2023474018 cites W2030624538 @default.
• W2023474018 cites W2035033462 @default.
• W2023474018 cites W2039983228 @default.
• W2023474018 cites W2043777136 @default.
• W2023474018 cites W2048516349 @default.
• W2023474018 cites W2049975802 @default.
• W2023474018 cites W2050632133 @default.
• W2023474018 cites W2053186614 @default.
• W2023474018 cites W2053226282 @default.
• W2023474018 cites W2053813584 @default.
• W2023474018 cites W2055112665 @default.
• W2023474018 cites W2062727889 @default.
• W2023474018 cites W2064468972 @default.
• W2023474018 cites W2067729711 @default.
• W2023474018 cites W2073618867 @default.
• W2023474018 cites W2084386777 @default.
• W2023474018 cites W2086040970 @default.
• W2023474018 cites W2100489979 @default.
• W2023474018 cites W2147274499 @default.
• W2023474018 cites W2168795016 @default.
• W2023474018 cites W2171175695 @default.
• W2023474018 cites W3098992670 @default.
• W2023474018 cites W3100169872 @default.
• W2023474018 cites W3102000940 @default.
• W2023474018 cites W3104079063 @default.
• W2023474018 cites W3106253105 @default.
• W2023474018 cites W4238983876 @default.
• W2023474018 cites W64807908 @default.
• W2023474018 doi "https://doi.org/10.1007/s11214-008-9431-3" @default.
• W2023474018 hasPublicationYear "2008" @default.
• W2023474018 type Work @default.
• W2023474018 sameAs 2023474018 @default.
• W2023474018 citedByCount "56" @default.
• W2023474018 countsByYear W20234740182012 @default.
• W2023474018 countsByYear W20234740182014 @default.
• W2023474018 countsByYear W20234740182015 @default.
• W2023474018 countsByYear W20234740182017 @default.
• W2023474018 countsByYear W20234740182018 @default.
• W2023474018 countsByYear W20234740182019 @default.
• W2023474018 countsByYear W20234740182023 @default.
• W2023474018 crossrefType "journal-article" @default.
• W2023474018 hasAuthorship W2023474018A5069923642 @default.
• W2023474018 hasAuthorship W2023474018A5076519013 @default.
• W2023474018 hasBestOaLocation W20234740181 @default.
• W2023474018 hasConcept C108411613 @default.
• W2023474018 hasConcept C115260700 @default.
• W2023474018 hasConcept C121332964 @default.
• W2023474018 hasConcept C1276947 @default.
• W2023474018 hasConcept C151465644 @default.
• W2023474018 hasConcept C190841160 @default.
• W2023474018 hasConcept C193587279 @default.
• W2023474018 hasConcept C194462397 @default.
• W2023474018 hasConcept C196939603 @default.
• W2023474018 hasConcept C32449521 @default.
• W2023474018 hasConcept C44870925 @default.
• W2023474018 hasConcept C539450922 @default.
• W2023474018 hasConcept C54834619 @default.
• W2023474018 hasConcept C62520636 @default.
• W2023474018 hasConcept C87355193 @default.
• W2023474018 hasConcept C96819898 @default.
• W2023474018 hasConcept C98444146 @default.
• W2023474018 hasConceptScore W2023474018C108411613 @default.
• W2023474018 hasConceptScore W2023474018C115260700 @default.
• W2023474018 hasConceptScore W2023474018C121332964 @default.
• W2023474018 hasConceptScore W2023474018C1276947 @default.
• W2023474018 hasConceptScore W2023474018C151465644 @default.
• W2023474018 hasConceptScore W2023474018C190841160 @default.
• W2023474018 hasConceptScore W2023474018C193587279 @default.
• W2023474018 hasConceptScore W2023474018C194462397 @default.
• W2023474018 hasConceptScore W2023474018C196939603 @default.

• next