FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2059637165> ?p ?o ?g. }

• W2059637165 endingPage "618" @default.
• W2059637165 startingPage "613" @default.
• W2059637165 abstract "Neutron monitor and interplanetary magnetic field data have been used to study features of the role of drift effect in the temporal changes of the diurnal anisotropy and of the energy spectrum of the 11-year variation of galactic cosmic rays. In order to strictly separate the sectors of the interplanetary magnetic field and its influence on the anisotropy of galactic cosmic rays four solar minima periods (1965, 1976, 1987 and 1997) have been considered. An attempt to separate drift effects in the diurnal anisotropy of galactic cosmic rays, first, due to the gradient and curvature of the regular interplanetary magnetic field, and second, due to the heliospheric neutral sheet has been made. The global survey methods has been used to calculate the components of the three dimensional diurnal anisotropy of galactic cosmic rays based on neutron monitors data. It is shown that there are significant differences between the diurnal anisotropy of galactic cosmic rays found in the reliably established various sectors (duration of each sectors is ≥ 4 days) of the interplanetary magnetic field. The interplanetary magnetic field sector structure effect in the diurnal anisotropy of galactic cosmic rays is assumed to be connected to the heliospheric neutral sheet drift, while 22-year variation of the diurnal anisotropy of galactic cosmic rays is assumed to be connected to drift due to the gradient and curvature of the regular interplanetary magnetic field for different qa > 0 and qA<0 solar magnetic cycles. It is shown that the role of drift in the temporal changes of the energy spectrum of the 11-year variation of GCR is insignificant in both of the qA > 0 and the qA<0 solar magnetic cycles. The temporal changes of the exponent index of the 11-year variation of GCR generally is connected with the various character of the diffusion in interplanetary space for minima and maxima epochs of solar activity." @default.
• W2059637165 created "2016-06-24" @default.
• W2059637165 creator A5000755241 @default.
• W2059637165 creator A5030653893 @default.
• W2059637165 creator A5032374859 @default.
• W2059637165 creator A5052334137 @default.
• W2059637165 creator A5091436362 @default.
• W2059637165 date "2001-01-01" @default.
• W2059637165 modified "2023-10-14" @default.
• W2059637165 title "The role of drift on the diurnal anisotropy and on temporal changes in the energy spectra of the 11-year variation for galactic cosmic rays" @default.
• W2059637165 cites W1964443169 @default.
• W2059637165 cites W1981474614 @default.
• W2059637165 cites W2003833064 @default.
• W2059637165 cites W2005268774 @default.
• W2059637165 cites W2018327652 @default.
• W2059637165 cites W2025810544 @default.
• W2059637165 cites W2075407888 @default.
• W2059637165 cites W2082221208 @default.
• W2059637165 cites W2082563749 @default.
• W2059637165 cites W2098429612 @default.
• W2059637165 cites W2109758598 @default.
• W2059637165 cites W2161229253 @default.
• W2059637165 cites W4239290506 @default.
• W2059637165 doi "https://doi.org/10.1016/s0273-1177(01)00092-8" @default.
• W2059637165 hasPublicationYear "2001" @default.
• W2059637165 type Work @default.
• W2059637165 sameAs 2059637165 @default.
• W2059637165 citedByCount "11" @default.
• W2059637165 countsByYear W20596371652015 @default.
• W2059637165 countsByYear W20596371652019 @default.
• W2059637165 countsByYear W20596371652020 @default.
• W2059637165 countsByYear W20596371652023 @default.
• W2059637165 crossrefType "journal-article" @default.
• W2059637165 hasAuthorship W2059637165A5000755241 @default.
• W2059637165 hasAuthorship W2059637165A5030653893 @default.
• W2059637165 hasAuthorship W2059637165A5032374859 @default.
• W2059637165 hasAuthorship W2059637165A5052334137 @default.
• W2059637165 hasAuthorship W2059637165A5091436362 @default.
• W2059637165 hasConcept C102988692 @default.
• W2059637165 hasConcept C108411613 @default.
• W2059637165 hasConcept C111309251 @default.
• W2059637165 hasConcept C115260700 @default.
• W2059637165 hasConcept C120665830 @default.
• W2059637165 hasConcept C121332964 @default.
• W2059637165 hasConcept C1276947 @default.
• W2059637165 hasConcept C194462397 @default.
• W2059637165 hasConcept C2780510704 @default.
• W2059637165 hasConcept C44870925 @default.
• W2059637165 hasConcept C54834619 @default.
• W2059637165 hasConcept C59496990 @default.
• W2059637165 hasConcept C62520636 @default.
• W2059637165 hasConcept C72886185 @default.
• W2059637165 hasConcept C85725439 @default.
• W2059637165 hasConceptScore W2059637165C102988692 @default.
• W2059637165 hasConceptScore W2059637165C108411613 @default.
• W2059637165 hasConceptScore W2059637165C111309251 @default.
• W2059637165 hasConceptScore W2059637165C115260700 @default.
• W2059637165 hasConceptScore W2059637165C120665830 @default.
• W2059637165 hasConceptScore W2059637165C121332964 @default.
• W2059637165 hasConceptScore W2059637165C1276947 @default.
• W2059637165 hasConceptScore W2059637165C194462397 @default.
• W2059637165 hasConceptScore W2059637165C2780510704 @default.
• W2059637165 hasConceptScore W2059637165C44870925 @default.
• W2059637165 hasConceptScore W2059637165C54834619 @default.
• W2059637165 hasConceptScore W2059637165C59496990 @default.
• W2059637165 hasConceptScore W2059637165C62520636 @default.
• W2059637165 hasConceptScore W2059637165C72886185 @default.
• W2059637165 hasConceptScore W2059637165C85725439 @default.
• W2059637165 hasIssue "3" @default.
• W2059637165 hasLocation W20596371651 @default.
• W2059637165 hasOpenAccess W2059637165 @default.
• W2059637165 hasPrimaryLocation W20596371651 @default.
• W2059637165 hasRelatedWork W1649426372 @default.
• W2059637165 hasRelatedWork W1666256647 @default.
• W2059637165 hasRelatedWork W1852578845 @default.
• W2059637165 hasRelatedWork W1996004707 @default.
• W2059637165 hasRelatedWork W2018311414 @default.
• W2059637165 hasRelatedWork W2025248174 @default.
• W2059637165 hasRelatedWork W2050894083 @default.
• W2059637165 hasRelatedWork W2594621812 @default.
• W2059637165 hasRelatedWork W2607370968 @default.
• W2059637165 hasRelatedWork W3034995903 @default.
• W2059637165 hasVolume "27" @default.
• W2059637165 isParatext "false" @default.
• W2059637165 isRetracted "false" @default.
• W2059637165 magId "2059637165" @default.
• W2059637165 workType "article" @default.