FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2156879319> ?p ?o ?g. }

• W2156879319 endingPage "7213" @default.
• W2156879319 startingPage "7199" @default.
• W2156879319 abstract "Abstract A statistical survey of 560 fast flows in midnight central plasma sheet is performed based on Time History of Events and Macroscale Interactions during Substorms (THEMIS) observations during its first two tail phases. From superposed epoch analysis, no significant substorm activities are found to be associated with the occurrence of fast flows beyond X =−15 R e . Considering the associations with substorm activities, the fast flows inside of X =−15 R e can be classified into two obvious classes: short duration (< 2.0 min) and long duration (> 4.0 min). Substorm breakups are shown to be more closely correlated to short‐duration fast flows. Furthermore, the onset of short‐duration fast flows in the dipolarization region ( X =−9 to −11 R e ) is almost simultaneous with the onset of substorm breakups and dipolarizations. On the other hand, time delays of 2–4 min are both found in the near‐Earth region ( X =−7 to −9 R e ) and in the near‐tail region ( X =−11 to −15 R e ). Assuming that short‐duration fast flows are generated by the force imbalance caused by cross‐tail current disruption, these features are consistent with the predictions made by the cowling electrojet current loop and the cross‐tail current disruption substorm models. In comparison, although more magnetic flux is transported toward Earth for long‐duration fast flows, no clear substorm breakup is closely associated with them. The analysis of 2‐D ion velocity distribution further shows some differences. For short‐duration fast flows, multiple crescent‐shaped ion populations are found. However, for long‐duration fast flows, there exists only a single crescent‐shaped ion population. The difference may be an important signature for distinguishing these two classes of fast flows." @default.
• W2156879319 created "2016-06-24" @default.
• W2156879319 creator A5018603529 @default.
• W2156879319 creator A5053237628 @default.
• W2156879319 creator A5075992973 @default.
• W2156879319 date "2014-09-01" @default.
• W2156879319 modified "2023-10-18" @default.
• W2156879319 title "Classification of fast flows in central plasma sheet: Superposed epoch analysis based on THEMIS observations" @default.
• W2156879319 cites W1593617336 @default.
• W2156879319 cites W1612594723 @default.
• W2156879319 cites W1630117700 @default.
• W2156879319 cites W1677621284 @default.
• W2156879319 cites W1887474673 @default.
• W2156879319 cites W1941028439 @default.
• W2156879319 cites W1965122059 @default.
• W2156879319 cites W1967959558 @default.
• W2156879319 cites W1977544241 @default.
• W2156879319 cites W1978866544 @default.
• W2156879319 cites W1980494593 @default.
• W2156879319 cites W1982366233 @default.
• W2156879319 cites W1983609891 @default.
• W2156879319 cites W1984645000 @default.
• W2156879319 cites W1994588075 @default.
• W2156879319 cites W1997526559 @default.
• W2156879319 cites W1999972909 @default.
• W2156879319 cites W2002270082 @default.
• W2156879319 cites W2002345125 @default.
• W2156879319 cites W2002457915 @default.
• W2156879319 cites W2005450585 @default.
• W2156879319 cites W2014267492 @default.
• W2156879319 cites W2016383558 @default.
• W2156879319 cites W2020631520 @default.
• W2156879319 cites W2023878915 @default.
• W2156879319 cites W2030775917 @default.
• W2156879319 cites W2032010034 @default.
• W2156879319 cites W2034819846 @default.
• W2156879319 cites W2050112897 @default.
• W2156879319 cites W2051063522 @default.
• W2156879319 cites W2055935861 @default.
• W2156879319 cites W2060337859 @default.
• W2156879319 cites W2062277859 @default.
• W2156879319 cites W2072404929 @default.
• W2156879319 cites W2075011376 @default.
• W2156879319 cites W2083263420 @default.
• W2156879319 cites W2084225263 @default.
• W2156879319 cites W2087487952 @default.
• W2156879319 cites W2088791205 @default.
• W2156879319 cites W2088940580 @default.
• W2156879319 cites W2092321620 @default.
• W2156879319 cites W2093198221 @default.
• W2156879319 cites W2099237689 @default.
• W2156879319 cites W2101947270 @default.
• W2156879319 cites W2103484130 @default.
• W2156879319 cites W2128880675 @default.
• W2156879319 cites W2129455499 @default.
• W2156879319 cites W2138761700 @default.
• W2156879319 cites W2170395381 @default.
• W2156879319 cites W2171175633 @default.
• W2156879319 doi "https://doi.org/10.1002/2014ja020105" @default.
• W2156879319 hasPublicationYear "2014" @default.
• W2156879319 type Work @default.
• W2156879319 sameAs 2156879319 @default.
• W2156879319 citedByCount "2" @default.
• W2156879319 countsByYear W21568793192016 @default.
• W2156879319 countsByYear W21568793192018 @default.
• W2156879319 crossrefType "journal-article" @default.
• W2156879319 hasAuthorship W2156879319A5018603529 @default.
• W2156879319 hasAuthorship W2156879319A5053237628 @default.
• W2156879319 hasAuthorship W2156879319A5075992973 @default.
• W2156879319 hasBestOaLocation W21568793191 @default.
• W2156879319 hasConcept C115260700 @default.
• W2156879319 hasConcept C121332964 @default.
• W2156879319 hasConcept C130443932 @default.
• W2156879319 hasConcept C134581325 @default.
• W2156879319 hasConcept C148043351 @default.
• W2156879319 hasConcept C150846664 @default.
• W2156879319 hasConcept C157899998 @default.
• W2156879319 hasConcept C199635899 @default.
• W2156879319 hasConcept C2777871205 @default.
• W2156879319 hasConcept C2780317896 @default.
• W2156879319 hasConcept C35666279 @default.
• W2156879319 hasConcept C44870925 @default.
• W2156879319 hasConcept C57879066 @default.
• W2156879319 hasConcept C62520636 @default.
• W2156879319 hasConcept C8058405 @default.
• W2156879319 hasConcept C82706917 @default.
• W2156879319 hasConcept C97355855 @default.
• W2156879319 hasConceptScore W2156879319C115260700 @default.
• W2156879319 hasConceptScore W2156879319C121332964 @default.
• W2156879319 hasConceptScore W2156879319C130443932 @default.
• W2156879319 hasConceptScore W2156879319C134581325 @default.
• W2156879319 hasConceptScore W2156879319C148043351 @default.
• W2156879319 hasConceptScore W2156879319C150846664 @default.
• W2156879319 hasConceptScore W2156879319C157899998 @default.
• W2156879319 hasConceptScore W2156879319C199635899 @default.
• W2156879319 hasConceptScore W2156879319C2777871205 @default.
• W2156879319 hasConceptScore W2156879319C2780317896 @default.
• W2156879319 hasConceptScore W2156879319C35666279 @default.

• next