FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2149787105> ?p ?o ?g. }

• W2149787105 endingPage "619" @default.
• W2149787105 startingPage "583" @default.
• W2149787105 abstract "Short period geomagnetic pulsations called IPDP (intervals of pulsations of diminishing periods) are investigated, using ground data obtained at 35 campaign stations in the northern polar region. Comparison of the frequency-time (f-t) spectrograms of data from the stations shows that the internal structures of f-t pattern of IPDP pulsations vary with a small separation between stations. The variability of the internal structures suggests that “an IPDP event” consists of many discrete wave packets each of which comes from individual sources. Spatial-temporal developments of IPDP wave power are also examined. The two-dimensional distribution of IPDP power is both highly structured in space, suggesting presence of discrete source regions, and also highly variable with time, indicating characteristic dynamic features of the source regions. The source regions are located in the dusk half of the magnetosphere in a range of L value from 4 to 10. Three types of dynamics of the source regions are found; 1) fast westward motion consistent with magnetic-drift velocity of 60-70keV protons in the magnetosphere, 2) quasi-stationary sources, which are almost stationary in the magnetospheric frame for periods longer than 10 minutes, 3) evolution of the IPDP region toward the night and earthward with increase in center frequency. When the westward moving sources arrive at the location of the stationary sources, they merge with them and do not go further westward beyond the stationary sources. These time developments of the IPDP source regions comprehensively explain most of the IPDP characteristics so far obtained from observations in a limited area. Not only well-defined IPDP's but also IPDP-like events with small and slower frequency rise were observed in high latitudes associated with concurrent magnetic field depressions at synchronous orbit and with positive magnetic bays. For both, the magnetic field depression is probably due to hot plasma injection into the evening sector, although clear substorm onsets were only identified for well-defined IPDP's. The occurrence rate of IPDP events monitored within the semi-global coverage of the network was once every six days or 20 percent in hourly occurrence in the dusk sector, more than twice the previously reported rate. The occurrence rate of IPDP is still much smaller than that of substorms. The small occurrence shows that IPDP events are not caused by every “plasma injection” associated with substorms." @default.
• W2149787105 created "2016-06-24" @default.
• W2149787105 creator A5016373585 @default.
• W2149787105 creator A5026008897 @default.
• W2149787105 creator A5033483342 @default.
• W2149787105 creator A5038127872 @default.
• W2149787105 creator A5043490114 @default.
• W2149787105 creator A5045499242 @default.
• W2149787105 creator A5050590135 @default.
• W2149787105 creator A5058005678 @default.
• W2149787105 creator A5060258990 @default.
• W2149787105 creator A5063484993 @default.
• W2149787105 creator A5071529415 @default.
• W2149787105 creator A5079117664 @default.
• W2149787105 creator A5083504095 @default.
• W2149787105 creator A5084217762 @default.
• W2149787105 creator A5086551478 @default.
• W2149787105 creator A5088208616 @default.
• W2149787105 date "1988-01-01" @default.
• W2149787105 modified "2023-10-16" @default.
• W2149787105 title "Multi-station observation of IPDP micropulsations - Two-dimensional distribution and evolution of the source regions." @default.
• W2149787105 cites W1973186224 @default.
• W2149787105 cites W1973350308 @default.
• W2149787105 cites W1988933184 @default.
• W2149787105 cites W1989618512 @default.
• W2149787105 cites W1995641386 @default.
• W2149787105 cites W2011782996 @default.
• W2149787105 cites W2012985101 @default.
• W2149787105 cites W2023807402 @default.
• W2149787105 cites W2025524804 @default.
• W2149787105 cites W2034700568 @default.
• W2149787105 cites W2042202625 @default.
• W2149787105 cites W2043910085 @default.
• W2149787105 cites W2047148383 @default.
• W2149787105 cites W2048123755 @default.
• W2149787105 cites W2056523231 @default.
• W2149787105 cites W2064537735 @default.
• W2149787105 cites W2067157677 @default.
• W2149787105 cites W2079242722 @default.
• W2149787105 cites W2090130446 @default.
• W2149787105 cites W2094113171 @default.
• W2149787105 cites W2124287763 @default.
• W2149787105 cites W2124910177 @default.
• W2149787105 doi "https://doi.org/10.5636/jgg.40.583" @default.
• W2149787105 hasPublicationYear "1988" @default.
• W2149787105 type Work @default.
• W2149787105 sameAs 2149787105 @default.
• W2149787105 citedByCount "12" @default.
• W2149787105 countsByYear W21497871052021 @default.
• W2149787105 crossrefType "journal-article" @default.
• W2149787105 hasAuthorship W2149787105A5016373585 @default.
• W2149787105 hasAuthorship W2149787105A5026008897 @default.
• W2149787105 hasAuthorship W2149787105A5033483342 @default.
• W2149787105 hasAuthorship W2149787105A5038127872 @default.
• W2149787105 hasAuthorship W2149787105A5043490114 @default.
• W2149787105 hasAuthorship W2149787105A5045499242 @default.
• W2149787105 hasAuthorship W2149787105A5050590135 @default.
• W2149787105 hasAuthorship W2149787105A5058005678 @default.
• W2149787105 hasAuthorship W2149787105A5060258990 @default.
• W2149787105 hasAuthorship W2149787105A5063484993 @default.
• W2149787105 hasAuthorship W2149787105A5071529415 @default.
• W2149787105 hasAuthorship W2149787105A5079117664 @default.
• W2149787105 hasAuthorship W2149787105A5083504095 @default.
• W2149787105 hasAuthorship W2149787105A5084217762 @default.
• W2149787105 hasAuthorship W2149787105A5086551478 @default.
• W2149787105 hasAuthorship W2149787105A5088208616 @default.
• W2149787105 hasBestOaLocation W21497871051 @default.
• W2149787105 hasConcept C115260700 @default.
• W2149787105 hasConcept C121332964 @default.
• W2149787105 hasConcept C127313418 @default.
• W2149787105 hasConcept C130443932 @default.
• W2149787105 hasConcept C13280743 @default.
• W2149787105 hasConcept C197129107 @default.
• W2149787105 hasConcept C199635899 @default.
• W2149787105 hasConcept C23123220 @default.
• W2149787105 hasConcept C2777016058 @default.
• W2149787105 hasConcept C41008148 @default.
• W2149787105 hasConcept C62520636 @default.
• W2149787105 hasConcept C62649853 @default.
• W2149787105 hasConcept C8058405 @default.
• W2149787105 hasConceptScore W2149787105C115260700 @default.
• W2149787105 hasConceptScore W2149787105C121332964 @default.
• W2149787105 hasConceptScore W2149787105C127313418 @default.
• W2149787105 hasConceptScore W2149787105C130443932 @default.
• W2149787105 hasConceptScore W2149787105C13280743 @default.
• W2149787105 hasConceptScore W2149787105C197129107 @default.
• W2149787105 hasConceptScore W2149787105C199635899 @default.
• W2149787105 hasConceptScore W2149787105C23123220 @default.
• W2149787105 hasConceptScore W2149787105C2777016058 @default.
• W2149787105 hasConceptScore W2149787105C41008148 @default.
• W2149787105 hasConceptScore W2149787105C62520636 @default.
• W2149787105 hasConceptScore W2149787105C62649853 @default.
• W2149787105 hasConceptScore W2149787105C8058405 @default.
• W2149787105 hasIssue "5" @default.
• W2149787105 hasLocation W21497871051 @default.
• W2149787105 hasOpenAccess W2149787105 @default.
• W2149787105 hasPrimaryLocation W21497871051 @default.
• W2149787105 hasRelatedWork W142717093 @default.

• next