FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2000882316> ?p ?o ?g. }

• W2000882316 endingPage "598" @default.
• W2000882316 startingPage "575" @default.
• W2000882316 abstract "Auroral nighttime infrared emission observed by the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument onboard the Thermosphere–Ionosphere–Mesosphere Energetics and Dynamics (TIMED) satellite is used to develop an empirical model of geomagnetic storm enhancements to E-region electron densities. The empirical model is called STORM-E and will be incorporated into the 2012 release of the International Reference Ionosphere (IRI). The proxy for characterizing the E-region response to geomagnetic forcing is NO+(v) Volume Emission Rates (VER) derived from the TIMED/SABER 4.3 μm channel limb radiance measurements. The storm-time response of the NO+(v) 4.3 μm VER is most sensitive to auroral particle precipitation. A statistical database of storm-time to climatological quiet-time ratios of SABER-observed NO+(v) 4.3 μm VER are fit to widely available geomagnetic indices using the theoretical framework of linear impulse-response theory. The STORM-E model provides a dynamic storm-time correction factor to adjust a known nighttime quiescent E-region electron density peak concentration for geomagnetic enhancements due to auroral particle precipitation. Part I of this series gives a detailed description of the algorithms and methodologies used to derive NO+(v) VER from SABER 4.3 μm limb emission measurements. In this paper, Part II of the series, the development of the E-region electron density storm-time correction factor is described. The STORM-E storm-time correction factor is fit to a single geomagnetic index. There are four versions of the STORM-E model, which are currently independent of magnetic local time. Each version is fit to one of the following indices: HP, AE, Ap, or Dst. High-latitude Incoherent Scatter Radar (ISR) E-region electron density measurements are compared to STORM-E predictions for various geomagnetic storm periods during solar cycle 23. These comparisons show that STORM-E significantly improves the prediction of E-region electron density enhancements due to auroral particle precipitation, in comparison to the nominal IRI model or to the quiet-time baseline electron density concentrations measured by ISR. The STORM-E/ISR comparisons indicate that the STORM-E fits to the Ap-, AE-, and HP-indices are comparable in both absolute accuracy and relative dynamical response. Contrarily, the Dst-index does not appear to be a suitable input driver to parameterize the E-region electron density response to geomagnetic activity." @default.
• W2000882316 created "2016-06-24" @default.
• W2000882316 creator A5004951061 @default.
• W2000882316 creator A5026205519 @default.
• W2000882316 creator A5035062621 @default.
• W2000882316 creator A5043866951 @default.
• W2000882316 creator A5090642422 @default.
• W2000882316 date "2013-02-01" @default.
• W2000882316 modified "2023-10-16" @default.
• W2000882316 title "Empirical STORM-E model: II. Geomagnetic corrections to nighttime ionospheric E-region electron densities" @default.
• W2000882316 cites W1576600094 @default.
• W2000882316 cites W1976375279 @default.
• W2000882316 cites W1986964719 @default.
• W2000882316 cites W1991410149 @default.
• W2000882316 cites W1991440943 @default.
• W2000882316 cites W1991523891 @default.
• W2000882316 cites W2007750023 @default.
• W2000882316 cites W2024784262 @default.
• W2000882316 cites W2034198774 @default.
• W2000882316 cites W2034877505 @default.
• W2000882316 cites W2047670190 @default.
• W2000882316 cites W2048631225 @default.
• W2000882316 cites W2057980539 @default.
• W2000882316 cites W2059069638 @default.
• W2000882316 cites W2066826612 @default.
• W2000882316 cites W2069954011 @default.
• W2000882316 cites W2076305882 @default.
• W2000882316 cites W2077507552 @default.
• W2000882316 cites W2088070691 @default.
• W2000882316 cites W2103550040 @default.
• W2000882316 cites W2118065507 @default.
• W2000882316 cites W2136436157 @default.
• W2000882316 cites W2150126807 @default.
• W2000882316 doi "https://doi.org/10.1016/j.asr.2012.09.014" @default.
• W2000882316 hasPublicationYear "2013" @default.
• W2000882316 type Work @default.
• W2000882316 sameAs 2000882316 @default.
• W2000882316 citedByCount "10" @default.
• W2000882316 countsByYear W20008823162014 @default.
• W2000882316 countsByYear W20008823162015 @default.
• W2000882316 countsByYear W20008823162018 @default.
• W2000882316 countsByYear W20008823162019 @default.
• W2000882316 countsByYear W20008823162021 @default.
• W2000882316 countsByYear W20008823162022 @default.
• W2000882316 crossrefType "journal-article" @default.
• W2000882316 hasAuthorship W2000882316A5004951061 @default.
• W2000882316 hasAuthorship W2000882316A5026205519 @default.
• W2000882316 hasAuthorship W2000882316A5035062621 @default.
• W2000882316 hasAuthorship W2000882316A5043866951 @default.
• W2000882316 hasAuthorship W2000882316A5090642422 @default.
• W2000882316 hasConcept C105306849 @default.
• W2000882316 hasConcept C115260700 @default.
• W2000882316 hasConcept C116403925 @default.
• W2000882316 hasConcept C121332964 @default.
• W2000882316 hasConcept C131980223 @default.
• W2000882316 hasConcept C153294291 @default.
• W2000882316 hasConcept C163861444 @default.
• W2000882316 hasConcept C170641098 @default.
• W2000882316 hasConcept C199635899 @default.
• W2000882316 hasConcept C39432304 @default.
• W2000882316 hasConcept C62520636 @default.
• W2000882316 hasConcept C69976271 @default.
• W2000882316 hasConcept C8058405 @default.
• W2000882316 hasConcept C91586092 @default.
• W2000882316 hasConcept C9844520 @default.
• W2000882316 hasConceptScore W2000882316C105306849 @default.
• W2000882316 hasConceptScore W2000882316C115260700 @default.
• W2000882316 hasConceptScore W2000882316C116403925 @default.
• W2000882316 hasConceptScore W2000882316C121332964 @default.
• W2000882316 hasConceptScore W2000882316C131980223 @default.
• W2000882316 hasConceptScore W2000882316C153294291 @default.
• W2000882316 hasConceptScore W2000882316C163861444 @default.
• W2000882316 hasConceptScore W2000882316C170641098 @default.
• W2000882316 hasConceptScore W2000882316C199635899 @default.
• W2000882316 hasConceptScore W2000882316C39432304 @default.
• W2000882316 hasConceptScore W2000882316C62520636 @default.
• W2000882316 hasConceptScore W2000882316C69976271 @default.
• W2000882316 hasConceptScore W2000882316C8058405 @default.
• W2000882316 hasConceptScore W2000882316C91586092 @default.
• W2000882316 hasConceptScore W2000882316C9844520 @default.
• W2000882316 hasIssue "4" @default.
• W2000882316 hasLocation W20008823161 @default.
• W2000882316 hasOpenAccess W2000882316 @default.
• W2000882316 hasPrimaryLocation W20008823161 @default.
• W2000882316 hasRelatedWork W1501023722 @default.
• W2000882316 hasRelatedWork W2049879057 @default.
• W2000882316 hasRelatedWork W2074433695 @default.
• W2000882316 hasRelatedWork W2092046792 @default.
• W2000882316 hasRelatedWork W258512305 @default.
• W2000882316 hasRelatedWork W3008861751 @default.
• W2000882316 hasRelatedWork W3159221365 @default.
• W2000882316 hasRelatedWork W3160652652 @default.
• W2000882316 hasRelatedWork W4200338384 @default.
• W2000882316 hasRelatedWork W4229745065 @default.
• W2000882316 hasVolume "51" @default.
• W2000882316 isParatext "false" @default.
• W2000882316 isRetracted "false" @default.
• W2000882316 magId "2000882316" @default.

• next