FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2130896593> ?p ?o ?g. }

• W2130896593 endingPage "14771" @default.
• W2130896593 startingPage "14763" @default.
• W2130896593 abstract "The intensity of >70 MeV cosmic ray protons observed during solar cycle 22 by Voyager 2 (V2) in the distant heliosphere reached a minimum in 1990, corresponding to the maximum of solar activity in mid‐1989 (allowing for the propagation time of the solar wind from the sun to Voyager 2 near 32 AU). A step decrease in the cosmic ray intensity observed within the first ≈ 125 days of 1990 was caused by a global merged interaction region (GMIR), consisting of a cluster of large‐amplitude magnetic field strength fluctuations, in which the field was predominantly stronger than average. The step decrease consists of four events in each of which the decrease in cosmic ray intensity is relatively large, and the recovery is either brief or absent. The relation between the cosmic ray intensity and the magnetic field strength observed near 32 AU during this period at the maximum of solar activity in 1989/1990 is similar to that which Voyager 2 observed near 11 AU in 1982/1983 following the maximum of solar activity in the previous solar cycle in 1980. The local changes in the cosmic ray intensity profile are related to the magnetic field strength. Near solar maximum the emission rate of ejecta, which contain magnetic fields that deviate significantly from the spiral direction, is a maximum. Nevertheless, the distribution of elevation angles of the magnetic field observed by Voyager 2 during 1990 is essentially the same as that observed during earlier parts of the solar cycle from 1986 through 1989, including solar minimum in 1986 and 1987. During 1990, the width of the distribution of elevation angles at ≈ 2 AU was the same as that observed at 1 AU. Sectors were observed, but no sector structure was present during 1990, just as in 1988, 1989, and 1991. The distribution of daily averages of the magnetic field strength is lognormal for 0.05 nT < B < 0.25 nT. However, there are more strong magnetic fields than the lognormal distribution predicts for 0.25 nT < B < 0.4 nT, owing to the large MIRs. The large‐scale fluctuations of the magnetic field strength have a multifractal structure in the low‐frequency range from 2.7 days to at least 21.3 days that influences the cosmic ray intensity profile." @default.
• W2130896593 created "2016-06-24" @default.
• W2130896593 creator A5015143017 @default.
• W2130896593 creator A5025300641 @default.
• W2130896593 creator A5087596659 @default.
• W2130896593 date "1995-08-01" @default.
• W2130896593 modified "2023-09-27" @default.
• W2130896593 title "Magnetic fields and cosmic rays in the distant heliosphere at solar maximum: Voyager 2 observations near 32 AU during 1990" @default.
• W2130896593 cites W1868863050 @default.
• W2130896593 cites W1977113547 @default.
• W2130896593 cites W1978949564 @default.
• W2130896593 cites W1981652677 @default.
• W2130896593 cites W1993790280 @default.
• W2130896593 cites W1996789889 @default.
• W2130896593 cites W2011096119 @default.
• W2130896593 cites W2011206836 @default.
• W2130896593 cites W2011977081 @default.
• W2130896593 cites W2014491215 @default.
• W2130896593 cites W2024598580 @default.
• W2130896593 cites W2033750748 @default.
• W2130896593 cites W2038509838 @default.
• W2130896593 cites W2045722349 @default.
• W2130896593 cites W2046837323 @default.
• W2130896593 cites W2062425987 @default.
• W2130896593 cites W2062440986 @default.
• W2130896593 cites W2067878364 @default.
• W2130896593 cites W2086314783 @default.
• W2130896593 cites W2091612307 @default.
• W2130896593 cites W2099680843 @default.
• W2130896593 cites W2105567047 @default.
• W2130896593 cites W2116162090 @default.
• W2130896593 cites W2131843659 @default.
• W2130896593 cites W2139364442 @default.
• W2130896593 cites W2140637432 @default.
• W2130896593 cites W2983717917 @default.
• W2130896593 cites W4294183471 @default.
• W2130896593 doi "https://doi.org/10.1029/95ja01557" @default.
• W2130896593 hasPublicationYear "1995" @default.
• W2130896593 type Work @default.
• W2130896593 sameAs 2130896593 @default.
• W2130896593 citedByCount "10" @default.
• W2130896593 countsByYear W21308965932015 @default.
• W2130896593 countsByYear W21308965932017 @default.
• W2130896593 countsByYear W21308965932021 @default.
• W2130896593 countsByYear W21308965932023 @default.
• W2130896593 crossrefType "journal-article" @default.
• W2130896593 hasAuthorship W2130896593A5015143017 @default.
• W2130896593 hasAuthorship W2130896593A5025300641 @default.
• W2130896593 hasAuthorship W2130896593A5087596659 @default.
• W2130896593 hasConcept C102988692 @default.
• W2130896593 hasConcept C108411613 @default.
• W2130896593 hasConcept C110619738 @default.
• W2130896593 hasConcept C111309251 @default.
• W2130896593 hasConcept C115260700 @default.
• W2130896593 hasConcept C120665830 @default.
• W2130896593 hasConcept C121332964 @default.
• W2130896593 hasConcept C127592171 @default.
• W2130896593 hasConcept C1276947 @default.
• W2130896593 hasConcept C144391981 @default.
• W2130896593 hasConcept C144992956 @default.
• W2130896593 hasConcept C164495641 @default.
• W2130896593 hasConcept C171428510 @default.
• W2130896593 hasConcept C180205008 @default.
• W2130896593 hasConcept C197370839 @default.
• W2130896593 hasConcept C43867161 @default.
• W2130896593 hasConcept C44870925 @default.
• W2130896593 hasConcept C52083857 @default.
• W2130896593 hasConcept C54834619 @default.
• W2130896593 hasConcept C62520636 @default.
• W2130896593 hasConcept C92150305 @default.
• W2130896593 hasConcept C93038891 @default.
• W2130896593 hasConceptScore W2130896593C102988692 @default.
• W2130896593 hasConceptScore W2130896593C108411613 @default.
• W2130896593 hasConceptScore W2130896593C110619738 @default.
• W2130896593 hasConceptScore W2130896593C111309251 @default.
• W2130896593 hasConceptScore W2130896593C115260700 @default.
• W2130896593 hasConceptScore W2130896593C120665830 @default.
• W2130896593 hasConceptScore W2130896593C121332964 @default.
• W2130896593 hasConceptScore W2130896593C127592171 @default.
• W2130896593 hasConceptScore W2130896593C1276947 @default.
• W2130896593 hasConceptScore W2130896593C144391981 @default.
• W2130896593 hasConceptScore W2130896593C144992956 @default.
• W2130896593 hasConceptScore W2130896593C164495641 @default.
• W2130896593 hasConceptScore W2130896593C171428510 @default.
• W2130896593 hasConceptScore W2130896593C180205008 @default.
• W2130896593 hasConceptScore W2130896593C197370839 @default.
• W2130896593 hasConceptScore W2130896593C43867161 @default.
• W2130896593 hasConceptScore W2130896593C44870925 @default.
• W2130896593 hasConceptScore W2130896593C52083857 @default.
• W2130896593 hasConceptScore W2130896593C54834619 @default.
• W2130896593 hasConceptScore W2130896593C62520636 @default.
• W2130896593 hasConceptScore W2130896593C92150305 @default.
• W2130896593 hasConceptScore W2130896593C93038891 @default.
• W2130896593 hasIssue "A8" @default.
• W2130896593 hasLocation W21308965931 @default.
• W2130896593 hasOpenAccess W2130896593 @default.
• W2130896593 hasPrimaryLocation W21308965931 @default.
• W2130896593 hasRelatedWork W2000594240 @default.

• next