FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2040897713> ?p ?o ?g. }

• W2040897713 endingPage "1309" @default.
• W2040897713 startingPage "1291" @default.
• W2040897713 abstract "Abstract. The solar maximum solar wind is highly structured in latitude, longitude and in time. Coronal measurements show a very high degree of variability, with large variations that are less apparent within in situ spacecraft measurements. Interplanetary scintillation (IPS) observations from EISCAT, covering distances from 20 to 100 solar radii (RS), are an ideal source of information on the inner solar wind and can be used, therefore, to cast light on its evolution with distance from the Sun. Earlier comparisons of in situ and IPS measurements under solar minimum conditions showed good large-scale agreement, particularly in the fast wind. In this study we attempt a quantitative comparison of measurements made over solar maximum by EISCAT (20–100 RS) and the Wind and Ulysses spacecraft (at 215 RS and 300–1000 RS, respectively). The intervals studied were August–September 1999, May 2000, September 2000 and May 2001, the last-named being the period of the second Ulysses fast latitude scan. Both ballistic and – when possible – MHD/ballistic hybrid models were used to relate the data sets, and we compare the results obtained from these two mapping methods. The results of this study suggest that solar wind velocities measured in situ were less variable than those estimated from IPS measurements closer to the Sun, with the greatest divergence between IPS velocities and in situ measurements occurring in regions where steep longitudinal velocity gradients were seen in situ. We suggest that the interaction between streams of solar wind with different velocities leads to smoothing of solar wind velocities between 30–60 RS and 1 AU, and that this process continues at greater distances from the Sun.Key words. Interplanetary physics (solar wind plasma; sources of the solar wind; instruments and techniques)" @default.
• W2040897713 created "2016-06-24" @default.
• W2040897713 creator A5004034288 @default.
• W2040897713 creator A5008151437 @default.
• W2040897713 creator A5010179711 @default.
• W2040897713 creator A5032645974 @default.
• W2040897713 creator A5055876984 @default.
• W2040897713 creator A5069295962 @default.
• W2040897713 creator A5081184984 @default.
• W2040897713 date "2002-09-30" @default.
• W2040897713 modified "2023-10-16" @default.
• W2040897713 title "The solar wind at solar maximum: comparisons of EISCAT IPS and in situ observations" @default.
• W2040897713 cites W112721901 @default.
• W2040897713 cites W127261416 @default.
• W2040897713 cites W1593154964 @default.
• W2040897713 cites W1636807752 @default.
• W2040897713 cites W1647949622 @default.
• W2040897713 cites W1666731139 @default.
• W2040897713 cites W1680471353 @default.
• W2040897713 cites W1965580956 @default.
• W2040897713 cites W1966911713 @default.
• W2040897713 cites W1976456772 @default.
• W2040897713 cites W1977123853 @default.
• W2040897713 cites W1979960294 @default.
• W2040897713 cites W1994618577 @default.
• W2040897713 cites W1995897024 @default.
• W2040897713 cites W2004375920 @default.
• W2040897713 cites W2007947547 @default.
• W2040897713 cites W2012379073 @default.
• W2040897713 cites W2016474388 @default.
• W2040897713 cites W2021584072 @default.
• W2040897713 cites W2023457622 @default.
• W2040897713 cites W2024709580 @default.
• W2040897713 cites W2028052840 @default.
• W2040897713 cites W2034655745 @default.
• W2040897713 cites W2035498687 @default.
• W2040897713 cites W2048209859 @default.
• W2040897713 cites W2049440614 @default.
• W2040897713 cites W2053438967 @default.
• W2040897713 cites W2062711931 @default.
• W2040897713 cites W2070508695 @default.
• W2040897713 cites W2072371580 @default.
• W2040897713 cites W2074266200 @default.
• W2040897713 cites W2076385432 @default.
• W2040897713 cites W2078080620 @default.
• W2040897713 cites W2078098365 @default.
• W2040897713 cites W2081080574 @default.
• W2040897713 cites W2081337432 @default.
• W2040897713 cites W2083500162 @default.
• W2040897713 cites W2085349139 @default.
• W2040897713 cites W2088553657 @default.
• W2040897713 cites W2092992870 @default.
• W2040897713 cites W2093816626 @default.
• W2040897713 cites W2093899314 @default.
• W2040897713 cites W2097208940 @default.
• W2040897713 cites W2106908151 @default.
• W2040897713 cites W2127112787 @default.
• W2040897713 cites W2130117854 @default.
• W2040897713 cites W2149448058 @default.
• W2040897713 cites W2167078411 @default.
• W2040897713 cites W2172191241 @default.
• W2040897713 cites W2172287724 @default.
• W2040897713 cites W2990339606 @default.
• W2040897713 cites W3021332574 @default.
• W2040897713 cites W3123943931 @default.
• W2040897713 cites W2033856236 @default.
• W2040897713 doi "https://doi.org/10.5194/angeo-20-1291-2002" @default.
• W2040897713 hasPublicationYear "2002" @default.
• W2040897713 type Work @default.
• W2040897713 sameAs 2040897713 @default.
• W2040897713 citedByCount "12" @default.
• W2040897713 countsByYear W20408977132012 @default.
• W2040897713 countsByYear W20408977132019 @default.
• W2040897713 countsByYear W20408977132021 @default.
• W2040897713 crossrefType "journal-article" @default.
• W2040897713 hasAuthorship W2040897713A5004034288 @default.
• W2040897713 hasAuthorship W2040897713A5008151437 @default.
• W2040897713 hasAuthorship W2040897713A5010179711 @default.
• W2040897713 hasAuthorship W2040897713A5032645974 @default.
• W2040897713 hasAuthorship W2040897713A5055876984 @default.
• W2040897713 hasAuthorship W2040897713A5069295962 @default.
• W2040897713 hasAuthorship W2040897713A5081184984 @default.
• W2040897713 hasBestOaLocation W20408977131 @default.
• W2040897713 hasConcept C108411613 @default.
• W2040897713 hasConcept C10880902 @default.
• W2040897713 hasConcept C121332964 @default.
• W2040897713 hasConcept C171428510 @default.
• W2040897713 hasConcept C43867161 @default.
• W2040897713 hasConcept C52083857 @default.
• W2040897713 hasConcept C54834619 @default.
• W2040897713 hasConcept C62520636 @default.
• W2040897713 hasConcept C72886185 @default.
• W2040897713 hasConcept C82706917 @default.
• W2040897713 hasConcept C91586092 @default.
• W2040897713 hasConcept C95448815 @default.
• W2040897713 hasConceptScore W2040897713C108411613 @default.
• W2040897713 hasConceptScore W2040897713C10880902 @default.
• W2040897713 hasConceptScore W2040897713C121332964 @default.

• next