FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2007706441> ?p ?o ?g. }

• W2007706441 abstract "[1] Simple analytical models have been derived for the first time, describing the 2-D distribution (along and across the Earth's magnetotail) of the central plasma sheet (CPS) ion temperature, density, and pressure, as functions of the incoming solar wind and interplanetary magnetic field (IMF) parameters, at distances between 10 and 50 RE. The models are based on a large set of data of the Low-Energy Particle (LEP) and Magnetic Field (MGF) instruments, taken by Geotail spacecraft between 1994 and 1998, comprising 7234 1-min average values of the CPS temperature and density. Concurrent solar wind and IMF data were provided by the Wind and IMP 8 spacecraft. The accuracy of the models was gauged by the correlation coefficient (c.c.) R between the observed and predicted values of a parameter. The CPS ion density N is controlled mostly by the solar wind proton density and by the northward component of the IMF. Being the least stable characteristic of the CPS, it yielded the lowest c.c. RN = 0.57. The CPS temperature T, controlled mainly by the solar wind speed V and the IMF Bz, gave a higher c.c. RT = 0.71. The CPS ion pressure P was best controlled by the solar wind ram pressure Psw and by an IMF-related parameter F = B⟂, where B⟂ is the perpendicular component of the IMF and θ is its clock angle. In a striking contrast with N and T, the model pressure P revealed a very high c.c. with the data, RP = 0.95, an apparent consequence of the force balance between the CPS and the tail lobe magnetic field. No significant dawn-dusk asymmetry of the CPS was found beyond the distance 10 RE, in line with the observed symmetry of the tail lobe magnetic field. The plasma density N is lowest at midnight and increases toward the tail's flanks. Larger (smaller) solar wind ion densities and northward (southward) IMF Bz result in larger (smaller) N in the CPS. In contrast to the density N, the temperature T peaks at the midnight meridian and falls off toward the dawn/dusk flanks. Faster (slower) solar wind flow and southward (northward) IMF Bz result in a hotter (cooler) CPS. The CPS ion pressure P is essentially a function of only XGSM in the midtail (20–50 RE); at closer distances the isobars gradually bend to approximately follow the contours of constant geomagnetic field strength. For northward IMF conditions combined with a slow solar wind, the isobars remain quasi-circular up to larger distances, reflecting a weaker tail current and, hence, more dipole-like magnetic field." @default.
• W2007706441 created "2016-06-24" @default.
• W2007706441 creator A5017832500 @default.
• W2007706441 date "2003-01-01" @default.
• W2007706441 modified "2023-10-18" @default.
• W2007706441 title "Tail plasma sheet models derived from Geotail particle data" @default.
• W2007706441 cites W1563937939 @default.
• W2007706441 cites W1658876719 @default.
• W2007706441 cites W1965499424 @default.
• W2007706441 cites W1968297928 @default.
• W2007706441 cites W1974700351 @default.
• W2007706441 cites W1980186939 @default.
• W2007706441 cites W1983609891 @default.
• W2007706441 cites W2015205771 @default.
• W2007706441 cites W2038574245 @default.
• W2007706441 cites W2048153225 @default.
• W2007706441 cites W2074805056 @default.
• W2007706441 cites W2081323702 @default.
• W2007706441 cites W2086149029 @default.
• W2007706441 cites W2103442202 @default.
• W2007706441 cites W2110581506 @default.
• W2007706441 cites W2116887196 @default.
• W2007706441 cites W2125997496 @default.
• W2007706441 cites W2136044855 @default.
• W2007706441 cites W2161501266 @default.
• W2007706441 cites W2162546849 @default.
• W2007706441 cites W2167986987 @default.
• W2007706441 cites W4244584727 @default.
• W2007706441 doi "https://doi.org/10.1029/2002ja009707" @default.
• W2007706441 hasPublicationYear "2003" @default.
• W2007706441 type Work @default.
• W2007706441 sameAs 2007706441 @default.
• W2007706441 citedByCount "187" @default.
• W2007706441 countsByYear W20077064412012 @default.
• W2007706441 countsByYear W20077064412013 @default.
• W2007706441 countsByYear W20077064412014 @default.
• W2007706441 countsByYear W20077064412015 @default.
• W2007706441 countsByYear W20077064412016 @default.
• W2007706441 countsByYear W20077064412017 @default.
• W2007706441 countsByYear W20077064412018 @default.
• W2007706441 countsByYear W20077064412019 @default.
• W2007706441 countsByYear W20077064412020 @default.
• W2007706441 countsByYear W20077064412021 @default.
• W2007706441 countsByYear W20077064412022 @default.
• W2007706441 countsByYear W20077064412023 @default.
• W2007706441 crossrefType "journal-article" @default.
• W2007706441 hasAuthorship W2007706441A5017832500 @default.
• W2007706441 hasBestOaLocation W20077064411 @default.
• W2007706441 hasConcept C111368507 @default.
• W2007706441 hasConcept C121332964 @default.
• W2007706441 hasConcept C127313418 @default.
• W2007706441 hasConcept C130443932 @default.
• W2007706441 hasConcept C134581325 @default.
• W2007706441 hasConcept C185544564 @default.
• W2007706441 hasConcept C2778517922 @default.
• W2007706441 hasConcept C30475298 @default.
• W2007706441 hasConcept C57879066 @default.
• W2007706441 hasConcept C8058405 @default.
• W2007706441 hasConcept C82706917 @default.
• W2007706441 hasConceptScore W2007706441C111368507 @default.
• W2007706441 hasConceptScore W2007706441C121332964 @default.
• W2007706441 hasConceptScore W2007706441C127313418 @default.
• W2007706441 hasConceptScore W2007706441C130443932 @default.
• W2007706441 hasConceptScore W2007706441C134581325 @default.
• W2007706441 hasConceptScore W2007706441C185544564 @default.
• W2007706441 hasConceptScore W2007706441C2778517922 @default.
• W2007706441 hasConceptScore W2007706441C30475298 @default.
• W2007706441 hasConceptScore W2007706441C57879066 @default.
• W2007706441 hasConceptScore W2007706441C8058405 @default.
• W2007706441 hasConceptScore W2007706441C82706917 @default.
• W2007706441 hasIssue "A3" @default.
• W2007706441 hasLocation W20077064411 @default.
• W2007706441 hasOpenAccess W2007706441 @default.
• W2007706441 hasPrimaryLocation W20077064411 @default.
• W2007706441 hasRelatedWork W1514285912 @default.
• W2007706441 hasRelatedWork W1537797671 @default.
• W2007706441 hasRelatedWork W1974580357 @default.
• W2007706441 hasRelatedWork W1981896073 @default.
• W2007706441 hasRelatedWork W2023804093 @default.
• W2007706441 hasRelatedWork W2036754350 @default.
• W2007706441 hasRelatedWork W2113209897 @default.
• W2007706441 hasRelatedWork W2372086831 @default.
• W2007706441 hasRelatedWork W337635856 @default.
• W2007706441 hasRelatedWork W39649430 @default.
• W2007706441 hasVolume "108" @default.
• W2007706441 isParatext "false" @default.
• W2007706441 isRetracted "false" @default.
• W2007706441 magId "2007706441" @default.
• W2007706441 workType "article" @default.