FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2018127991> ?p ?o ?g. }

• W2018127991 endingPage "1846" @default.
• W2018127991 startingPage "1837" @default.
• W2018127991 abstract "Dayside reconnection, which is particularly effective for a southward interplanetary magnetic field (IMF), allows magnetosheath particles to enter the magnetosphere where they form the plasma mantle. The motions of the reconnected flux tubes produce convective flows in the ionosphere. It is known that the convection patterns in the polar cap are skewed to the dawnside for a positive IMF B y (or duskside for a negative IMF B y ) in the northern polar cap. Correspondingly, one would expect to find asymmetric distributions of mantle particle precipitation, but previous results have been unclear. In this paper the correlation between B y and the distribution of mantle particle precipitation is studied for steady IMF conditions with southward IMF. Ion and electron data from the DMSP F6 and F7 satellites are used to identify the mantle region and IMP 8 is used as a solar wind monitor to characterize the IMF. We study the local time extension of mantle precipitation in the prenoon and postnoon regions. We find that, in accordance with theoretical expectations for a positive (negative) IMF B y , mantle particle precipitation mainly appears in the prenoon region of the northern (southern) hemisphere. The mantle particle precipitation can extend to as early as 0600 magnetic local time (MLT) in the prenoon region but extends over a smaller local time region in the postnoon sector (we did not find mantle plasma beyond 1600 MLT in our data set although coverage is scant in this area). Magnetometer data from F7 are used to determine whether part of the region 1 current flows on open field lines. We find that at times part of the region 1 sense current extends into the region of mantle particle precipitation, and is therefore on open field lines. In other cases, region 1 currents are absent on open field lines. Most of the observed features can be readily interpreted in terms of the open magnetosphere model." @default.
• W2018127991 created "2016-06-24" @default.
• W2018127991 creator A5017051923 @default.
• W2018127991 creator A5045867667 @default.
• W2018127991 creator A5066399283 @default.
• W2018127991 creator A5071392286 @default.
• W2018127991 creator A5089192067 @default.
• W2018127991 date "1995-02-01" @default.
• W2018127991 modified "2023-10-13" @default.
• W2018127991 title "Interplanetary magnetic field control of mantle precipitation and associated field‐aligned currents" @default.
• W2018127991 cites W1565779905 @default.
• W2018127991 cites W1584781897 @default.
• W2018127991 cites W1626037342 @default.
• W2018127991 cites W1670350366 @default.
• W2018127991 cites W1964344434 @default.
• W2018127991 cites W1977276451 @default.
• W2018127991 cites W1983679859 @default.
• W2018127991 cites W1986048969 @default.
• W2018127991 cites W1992023004 @default.
• W2018127991 cites W1997878204 @default.
• W2018127991 cites W2002861593 @default.
• W2018127991 cites W2006579639 @default.
• W2018127991 cites W2007024794 @default.
• W2018127991 cites W2010031777 @default.
• W2018127991 cites W2017921450 @default.
• W2018127991 cites W2022242462 @default.
• W2018127991 cites W2024183712 @default.
• W2018127991 cites W2024308221 @default.
• W2018127991 cites W2030795570 @default.
• W2018127991 cites W2038936445 @default.
• W2018127991 cites W2039684162 @default.
• W2018127991 cites W2049284007 @default.
• W2018127991 cites W2066608977 @default.
• W2018127991 cites W2068456598 @default.
• W2018127991 cites W2078752943 @default.
• W2018127991 cites W2087217114 @default.
• W2018127991 cites W2093615122 @default.
• W2018127991 cites W2094285495 @default.
• W2018127991 cites W2094839310 @default.
• W2018127991 cites W2107391508 @default.
• W2018127991 cites W2127610356 @default.
• W2018127991 cites W2131996381 @default.
• W2018127991 cites W2142159801 @default.
• W2018127991 cites W2146553970 @default.
• W2018127991 cites W2149641874 @default.
• W2018127991 cites W2171492829 @default.
• W2018127991 doi "https://doi.org/10.1029/94ja02037" @default.
• W2018127991 hasPublicationYear "1995" @default.
• W2018127991 type Work @default.
• W2018127991 sameAs 2018127991 @default.
• W2018127991 citedByCount "14" @default.
• W2018127991 countsByYear W20181279912012 @default.
• W2018127991 countsByYear W20181279912013 @default.
• W2018127991 countsByYear W20181279912023 @default.
• W2018127991 crossrefType "journal-article" @default.
• W2018127991 hasAuthorship W2018127991A5017051923 @default.
• W2018127991 hasAuthorship W2018127991A5045867667 @default.
• W2018127991 hasAuthorship W2018127991A5066399283 @default.
• W2018127991 hasAuthorship W2018127991A5071392286 @default.
• W2018127991 hasAuthorship W2018127991A5089192067 @default.
• W2018127991 hasConcept C102988692 @default.
• W2018127991 hasConcept C108411613 @default.
• W2018127991 hasConcept C10899652 @default.
• W2018127991 hasConcept C115260700 @default.
• W2018127991 hasConcept C121332964 @default.
• W2018127991 hasConcept C127313418 @default.
• W2018127991 hasConcept C130443932 @default.
• W2018127991 hasConcept C140161248 @default.
• W2018127991 hasConcept C153294291 @default.
• W2018127991 hasConcept C61922881 @default.
• W2018127991 hasConcept C62520636 @default.
• W2018127991 hasConcept C67236022 @default.
• W2018127991 hasConcept C8058405 @default.
• W2018127991 hasConceptScore W2018127991C102988692 @default.
• W2018127991 hasConceptScore W2018127991C108411613 @default.
• W2018127991 hasConceptScore W2018127991C10899652 @default.
• W2018127991 hasConceptScore W2018127991C115260700 @default.
• W2018127991 hasConceptScore W2018127991C121332964 @default.
• W2018127991 hasConceptScore W2018127991C127313418 @default.
• W2018127991 hasConceptScore W2018127991C130443932 @default.
• W2018127991 hasConceptScore W2018127991C140161248 @default.
• W2018127991 hasConceptScore W2018127991C153294291 @default.
• W2018127991 hasConceptScore W2018127991C61922881 @default.
• W2018127991 hasConceptScore W2018127991C62520636 @default.
• W2018127991 hasConceptScore W2018127991C67236022 @default.
• W2018127991 hasConceptScore W2018127991C8058405 @default.
• W2018127991 hasIssue "A2" @default.
• W2018127991 hasLocation W20181279911 @default.
• W2018127991 hasOpenAccess W2018127991 @default.
• W2018127991 hasPrimaryLocation W20181279911 @default.
• W2018127991 hasRelatedWork W1887198777 @default.
• W2018127991 hasRelatedWork W1973105758 @default.
• W2018127991 hasRelatedWork W1987051663 @default.
• W2018127991 hasRelatedWork W2011779211 @default.
• W2018127991 hasRelatedWork W2017051871 @default.
• W2018127991 hasRelatedWork W2041326892 @default.
• W2018127991 hasRelatedWork W2047470230 @default.
• W2018127991 hasRelatedWork W2071525369 @default.

• next