FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2036342225> ?p ?o ?g. }

• W2036342225 endingPage "1031" @default.
• W2036342225 startingPage "1023" @default.
• W2036342225 abstract "Magnetic storms due to corotating interaction regions (CIRs) have been shown to elicit different responses in the magnetosphere than those prompted by other types of solar wind driving conditions such as coronal mass ejections (CMEs). In particular, CIRs provoke a much weaker response in ground magnetometer data (Dst), possibly indicative of a weaker ring current. They also last many days longer than the CME events, yet over these longer events they couple a great deal of energy, sometimes comparable to that involved in typically larger-Dst CME events. It may seem at first that the weaker driving of CIR events must result in proportionally weaker magnetospheric response, but that is not always the case. In this work we show that magnetic storms driven by CIRs deposit more energy in the ionosphere and ring current than would be expected from the electromagnetic energy input from the CIRs. They appear to be more geoefficient, in the sense that the ratio of the measured energy deposited (ring current, Joule heating, and auroral precipitation) to energy input is greater than that for CMEs." @default.
• W2036342225 created "2016-06-24" @default.
• W2036342225 creator A5004034517 @default.
• W2036342225 creator A5012841287 @default.
• W2036342225 creator A5030898415 @default.
• W2036342225 creator A5053168658 @default.
• W2036342225 date "2009-07-01" @default.
• W2036342225 modified "2023-10-16" @default.
• W2036342225 title "Geoefficiency and energy partitioning in CIR-driven and CME-driven storms" @default.
• W2036342225 cites W1574301248 @default.
• W2036342225 cites W1638851641 @default.
• W2036342225 cites W1665152549 @default.
• W2036342225 cites W1679805614 @default.
• W2036342225 cites W1834219724 @default.
• W2036342225 cites W1965057733 @default.
• W2036342225 cites W1970488982 @default.
• W2036342225 cites W1970974534 @default.
• W2036342225 cites W1971834677 @default.
• W2036342225 cites W1974705747 @default.
• W2036342225 cites W1980260426 @default.
• W2036342225 cites W1986396546 @default.
• W2036342225 cites W2002497661 @default.
• W2036342225 cites W2003412877 @default.
• W2036342225 cites W2029116031 @default.
• W2036342225 cites W2030877989 @default.
• W2036342225 cites W2033203174 @default.
• W2036342225 cites W2034105878 @default.
• W2036342225 cites W2038785802 @default.
• W2036342225 cites W2040491062 @default.
• W2036342225 cites W2043677973 @default.
• W2036342225 cites W2046648585 @default.
• W2036342225 cites W2052012982 @default.
• W2036342225 cites W2064746205 @default.
• W2036342225 cites W2072579688 @default.
• W2036342225 cites W2075512560 @default.
• W2036342225 cites W2081614087 @default.
• W2036342225 cites W2083766750 @default.
• W2036342225 cites W2087594811 @default.
• W2036342225 cites W2094117988 @default.
• W2036342225 cites W2109569220 @default.
• W2036342225 cites W2117798875 @default.
• W2036342225 cites W2169384784 @default.
• W2036342225 cites W2169685069 @default.
• W2036342225 doi "https://doi.org/10.1016/j.jastp.2009.02.005" @default.
• W2036342225 hasPublicationYear "2009" @default.
• W2036342225 type Work @default.
• W2036342225 sameAs 2036342225 @default.
• W2036342225 citedByCount "127" @default.
• W2036342225 countsByYear W20363422252012 @default.
• W2036342225 countsByYear W20363422252013 @default.
• W2036342225 countsByYear W20363422252014 @default.
• W2036342225 countsByYear W20363422252015 @default.
• W2036342225 countsByYear W20363422252016 @default.
• W2036342225 countsByYear W20363422252017 @default.
• W2036342225 countsByYear W20363422252018 @default.
• W2036342225 countsByYear W20363422252019 @default.
• W2036342225 countsByYear W20363422252020 @default.
• W2036342225 countsByYear W20363422252021 @default.
• W2036342225 countsByYear W20363422252022 @default.
• W2036342225 countsByYear W20363422252023 @default.
• W2036342225 crossrefType "journal-article" @default.
• W2036342225 hasAuthorship W2036342225A5004034517 @default.
• W2036342225 hasAuthorship W2036342225A5012841287 @default.
• W2036342225 hasAuthorship W2036342225A5030898415 @default.
• W2036342225 hasAuthorship W2036342225A5053168658 @default.
• W2036342225 hasConcept C105306849 @default.
• W2036342225 hasConcept C108411613 @default.
• W2036342225 hasConcept C115260700 @default.
• W2036342225 hasConcept C116403925 @default.
• W2036342225 hasConcept C121332964 @default.
• W2036342225 hasConcept C128277356 @default.
• W2036342225 hasConcept C130443932 @default.
• W2036342225 hasConcept C153294291 @default.
• W2036342225 hasConcept C170641098 @default.
• W2036342225 hasConcept C30475298 @default.
• W2036342225 hasConcept C44870925 @default.
• W2036342225 hasConcept C62520636 @default.
• W2036342225 hasConcept C72886185 @default.
• W2036342225 hasConcept C8058405 @default.
• W2036342225 hasConcept C91586092 @default.
• W2036342225 hasConcept C9844520 @default.
• W2036342225 hasConceptScore W2036342225C105306849 @default.
• W2036342225 hasConceptScore W2036342225C108411613 @default.
• W2036342225 hasConceptScore W2036342225C115260700 @default.
• W2036342225 hasConceptScore W2036342225C116403925 @default.
• W2036342225 hasConceptScore W2036342225C121332964 @default.
• W2036342225 hasConceptScore W2036342225C128277356 @default.
• W2036342225 hasConceptScore W2036342225C130443932 @default.
• W2036342225 hasConceptScore W2036342225C153294291 @default.
• W2036342225 hasConceptScore W2036342225C170641098 @default.
• W2036342225 hasConceptScore W2036342225C30475298 @default.
• W2036342225 hasConceptScore W2036342225C44870925 @default.
• W2036342225 hasConceptScore W2036342225C62520636 @default.
• W2036342225 hasConceptScore W2036342225C72886185 @default.
• W2036342225 hasConceptScore W2036342225C8058405 @default.
• W2036342225 hasConceptScore W2036342225C91586092 @default.
• W2036342225 hasConceptScore W2036342225C9844520 @default.
• W2036342225 hasIssue "10-11" @default.

• next