FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1992606918> ?p ?o ?g. }

• W1992606918 endingPage "20759" @default.
• W1992606918 startingPage "20759" @default.
• W1992606918 abstract "IMP 8 (IMP J) magnetic field observations are used to determine the properties of the high-latitude tail boundary, which separates the tail lobe and the magnetosheath. Boundary crossings are marked by transitions from quiet lobe to disturbed magnetosheath fields. From five years (1978–1982) of IMP 8 observations, a data set of 244 boundary crossings has been identified in the XGSM range of −15 to −40 RE and |Z′GSM| >15 RE, where Z′GSM is the distance from the neutral sheet. The results suggest the following: (1) the tail cross section is slightly flattened in the north–south direction, (2) the high-latitude magnetotail field and boundary continue to flare antisunward out to 40 RE downstream of the Earth, and (3) interplanetary magnetic field (IMF) BZ and the solar wind dynamic pressure (but not, evidently, the solar wind magnetic pressure) control the boundary location. The dependence on IMF BZ is consistent with the buildup of magnetic fluxes in the magnetotail during periods of southward IMF BZ. Examination of the magnetic fields on each side of the boundary indicates the following: (1) The solar wind dynamic pressure determines the lobe-side field strength. (2) The flaring angle is estimated on the basis of the classical model of the Chapman-Ferraro problem. The result is consistent with the X dependence of the tail size and with the orientation of the lobe-side field (all have flaring angles of 7°–8°). (3) The IMF strength controls the sheath-side field strength, with a lesser contribution from the solar wind dynamic pressure. (4) The current flowing at the boundary primarily depends on the solar wind dynamic pressure. In summary, the present results indicate that the solar wind dynamic pressure is the most important factor determining the nature of the near-Earth magnetotail magnetopause. We also present evidence that the IMF BZ plays an important role in these processes." @default.
• W1992606918 created "2016-06-24" @default.
• W1992606918 creator A5043490114 @default.
• W1992606918 creator A5083926853 @default.
• W1992606918 date "1990-01-01" @default.
• W1992606918 modified "2023-09-25" @default.
• W1992606918 title "IMP 8 magnetic observations of the high-latitude tail boundary: Locations and force balance" @default.
• W1992606918 cites W1488810278 @default.
• W1992606918 cites W1631675178 @default.
• W1992606918 cites W1966271754 @default.
• W1992606918 cites W1971311710 @default.
• W1992606918 cites W1977276451 @default.
• W1992606918 cites W1982142361 @default.
• W1992606918 cites W1993559049 @default.
• W1992606918 cites W1995333698 @default.
• W1992606918 cites W1997730214 @default.
• W1992606918 cites W1999239776 @default.
• W1992606918 cites W2016103444 @default.
• W1992606918 cites W2016955499 @default.
• W1992606918 cites W2020168936 @default.
• W1992606918 cites W2033686255 @default.
• W1992606918 cites W2038420843 @default.
• W1992606918 cites W2042929170 @default.
• W1992606918 cites W2043522612 @default.
• W1992606918 cites W2058346098 @default.
• W1992606918 cites W2060206130 @default.
• W1992606918 cites W2065077801 @default.
• W1992606918 cites W2067127557 @default.
• W1992606918 cites W2075467910 @default.
• W1992606918 cites W2077189156 @default.
• W1992606918 cites W2086563217 @default.
• W1992606918 cites W2103041946 @default.
• W1992606918 cites W2103350226 @default.
• W1992606918 cites W2106030370 @default.
• W1992606918 cites W2107878644 @default.
• W1992606918 cites W2109640488 @default.
• W1992606918 cites W2113336467 @default.
• W1992606918 cites W2123787169 @default.
• W1992606918 cites W2150070598 @default.
• W1992606918 cites W2166429692 @default.
• W1992606918 cites W2171411205 @default.
• W1992606918 cites W2466402948 @default.
• W1992606918 cites W4255260736 @default.
• W1992606918 doi "https://doi.org/10.1029/ja095ia12p20759" @default.
• W1992606918 hasPublicationYear "1990" @default.
• W1992606918 type Work @default.
• W1992606918 sameAs 1992606918 @default.
• W1992606918 citedByCount "15" @default.
• W1992606918 countsByYear W19926069182019 @default.
• W1992606918 crossrefType "journal-article" @default.
• W1992606918 hasAuthorship W1992606918A5043490114 @default.
• W1992606918 hasAuthorship W1992606918A5083926853 @default.
• W1992606918 hasConcept C121332964 @default.
• W1992606918 hasConcept C122523270 @default.
• W1992606918 hasConcept C127313418 @default.
• W1992606918 hasConcept C130443932 @default.
• W1992606918 hasConcept C13280743 @default.
• W1992606918 hasConcept C134306372 @default.
• W1992606918 hasConcept C185544564 @default.
• W1992606918 hasConcept C3017817131 @default.
• W1992606918 hasConcept C33923547 @default.
• W1992606918 hasConcept C57879066 @default.
• W1992606918 hasConcept C62354387 @default.
• W1992606918 hasConcept C8058405 @default.
• W1992606918 hasConcept C82706917 @default.
• W1992606918 hasConcept C91586092 @default.
• W1992606918 hasConceptScore W1992606918C121332964 @default.
• W1992606918 hasConceptScore W1992606918C122523270 @default.
• W1992606918 hasConceptScore W1992606918C127313418 @default.
• W1992606918 hasConceptScore W1992606918C130443932 @default.
• W1992606918 hasConceptScore W1992606918C13280743 @default.
• W1992606918 hasConceptScore W1992606918C134306372 @default.
• W1992606918 hasConceptScore W1992606918C185544564 @default.
• W1992606918 hasConceptScore W1992606918C3017817131 @default.
• W1992606918 hasConceptScore W1992606918C33923547 @default.
• W1992606918 hasConceptScore W1992606918C57879066 @default.
• W1992606918 hasConceptScore W1992606918C62354387 @default.
• W1992606918 hasConceptScore W1992606918C8058405 @default.
• W1992606918 hasConceptScore W1992606918C82706917 @default.
• W1992606918 hasConceptScore W1992606918C91586092 @default.
• W1992606918 hasIssue "A12" @default.
• W1992606918 hasLocation W19926069181 @default.
• W1992606918 hasOpenAccess W1992606918 @default.
• W1992606918 hasPrimaryLocation W19926069181 @default.
• W1992606918 hasRelatedWork W1603623444 @default.
• W1992606918 hasRelatedWork W1646954443 @default.
• W1992606918 hasRelatedWork W1657594004 @default.
• W1992606918 hasRelatedWork W1677136756 @default.
• W1992606918 hasRelatedWork W2047872663 @default.
• W1992606918 hasRelatedWork W2061674797 @default.
• W1992606918 hasRelatedWork W2131426691 @default.
• W1992606918 hasRelatedWork W3014145384 @default.
• W1992606918 hasRelatedWork W643280293 @default.
• W1992606918 hasRelatedWork W2126106680 @default.
• W1992606918 hasVolume "95" @default.
• W1992606918 isParatext "false" @default.
• W1992606918 isRetracted "false" @default.
• W1992606918 magId "1992606918" @default.

• next