FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4308117981> ?p ?o ?g. }

• W4308117981 endingPage "5486" @default.
• W4308117981 startingPage "5486" @default.
• W4308117981 abstract "During emergency events, we could significantly depend on the stable operation of radio communication, navigation, and radars. The ionosphere, especially its auroral regions, significantly influences radio systems, which is why scientists and engineers create systems to monitor these regions. Using data from the global GNSS network, we analyzed the 10 strongest magnetic storms of solar cycle 24: five coronal mass ejection-driven (CME-driven) and five high-speed stream-driven (HSS-driven) storms. The analysis was based on the calculation of the standard deviation of the total electron content (TEC) derivative (rate of TEC index, ROTI). Under all the storms, the ROTI featured similar dynamics: the average ROTI reaches the highest values during the main phase, and the higher the intensity is, the more intense and equatorward the average ROTI registered. The highest cross-correlations are observed with a lag of 1 h, between the IMF z-component Bz and the magnetic latitude where the highest ROTI values appear. The auroral electrojet (SME index) shows the highest impact on the ROTI dynamics. An increase in the space weather indices (in absolute value) is accompanied by a decrease in the latitude where the maximal ROTI occurs. We found that the peculiarities of a storm affect the ROTI dynamics: all the CME-driven storms feature a high cross-correlation (>0.75) between the IMF z-component Bz and the magnetic latitude where the highest ROTI appears, while the HSS-driven storms feature a lower cross-correlation (<0.75) between them. The difference in duration of similar (by maximal values of geomagnetic indices) HSS- and CME-driven storms could produce differences in the highest ROTI values. Correlations show that compared to HSS-driven storms, CME-driven ones more directly impact the ROTI values and locations of regions with a high ROTI." @default.
• W4308117981 created "2022-11-08" @default.
• W4308117981 creator A5009700730 @default.
• W4308117981 creator A5090330499 @default.
• W4308117981 date "2022-10-31" @default.
• W4308117981 modified "2023-10-05" @default.
• W4308117981 title "Auroral Oval Boundary Dynamics on the Nature of Geomagnetic Storm" @default.
• W4308117981 cites W1526723381 @default.
• W4308117981 cites W1558740187 @default.
• W4308117981 cites W1616645436 @default.
• W4308117981 cites W1627554331 @default.
• W4308117981 cites W1900342918 @default.
• W4308117981 cites W1925717721 @default.
• W4308117981 cites W1964073316 @default.
• W4308117981 cites W1997574807 @default.
• W4308117981 cites W1998820031 @default.
• W4308117981 cites W2014674958 @default.
• W4308117981 cites W2050311703 @default.
• W4308117981 cites W2059020445 @default.
• W4308117981 cites W2077776032 @default.
• W4308117981 cites W2087594811 @default.
• W4308117981 cites W2094736009 @default.
• W4308117981 cites W2126314625 @default.
• W4308117981 cites W2140050818 @default.
• W4308117981 cites W2160811494 @default.
• W4308117981 cites W2278387834 @default.
• W4308117981 cites W2578611950 @default.
• W4308117981 cites W2800618584 @default.
• W4308117981 cites W2807200728 @default.
• W4308117981 cites W2883530500 @default.
• W4308117981 cites W2886030789 @default.
• W4308117981 cites W2912270737 @default.
• W4308117981 cites W2921998177 @default.
• W4308117981 cites W2946200232 @default.
• W4308117981 cites W2948658949 @default.
• W4308117981 cites W2997016292 @default.
• W4308117981 cites W3016005717 @default.
• W4308117981 cites W3020207185 @default.
• W4308117981 cites W3024425801 @default.
• W4308117981 cites W3027843661 @default.
• W4308117981 cites W3033966919 @default.
• W4308117981 cites W3035721993 @default.
• W4308117981 cites W3036507049 @default.
• W4308117981 cites W3042626425 @default.
• W4308117981 cites W3049675834 @default.
• W4308117981 cites W3089484317 @default.
• W4308117981 cites W3138416038 @default.
• W4308117981 cites W3159614494 @default.
• W4308117981 cites W3186436004 @default.
• W4308117981 cites W3199737163 @default.
• W4308117981 cites W4200334821 @default.
• W4308117981 cites W4200526509 @default.
• W4308117981 cites W4280570456 @default.
• W4308117981 doi "https://doi.org/10.3390/rs14215486" @default.
• W4308117981 hasPublicationYear "2022" @default.
• W4308117981 type Work @default.
• W4308117981 citedByCount "4" @default.
• W4308117981 countsByYear W43081179812023 @default.
• W4308117981 crossrefType "journal-article" @default.
• W4308117981 hasAuthorship W4308117981A5009700730 @default.
• W4308117981 hasAuthorship W4308117981A5090330499 @default.
• W4308117981 hasBestOaLocation W43081179811 @default.
• W4308117981 hasConcept C105306849 @default.
• W4308117981 hasConcept C108411613 @default.
• W4308117981 hasConcept C116403925 @default.
• W4308117981 hasConcept C121332964 @default.
• W4308117981 hasConcept C151325931 @default.
• W4308117981 hasConcept C153294291 @default.
• W4308117981 hasConcept C170641098 @default.
• W4308117981 hasConcept C176379880 @default.
• W4308117981 hasConcept C39432304 @default.
• W4308117981 hasConcept C62520636 @default.
• W4308117981 hasConcept C8058405 @default.
• W4308117981 hasConcept C82706917 @default.
• W4308117981 hasConcept C91586092 @default.
• W4308117981 hasConceptScore W4308117981C105306849 @default.
• W4308117981 hasConceptScore W4308117981C108411613 @default.
• W4308117981 hasConceptScore W4308117981C116403925 @default.
• W4308117981 hasConceptScore W4308117981C121332964 @default.
• W4308117981 hasConceptScore W4308117981C151325931 @default.
• W4308117981 hasConceptScore W4308117981C153294291 @default.
• W4308117981 hasConceptScore W4308117981C170641098 @default.
• W4308117981 hasConceptScore W4308117981C176379880 @default.
• W4308117981 hasConceptScore W4308117981C39432304 @default.
• W4308117981 hasConceptScore W4308117981C62520636 @default.
• W4308117981 hasConceptScore W4308117981C8058405 @default.
• W4308117981 hasConceptScore W4308117981C82706917 @default.
• W4308117981 hasConceptScore W4308117981C91586092 @default.
• W4308117981 hasFunder F4320327494 @default.
• W4308117981 hasIssue "21" @default.
• W4308117981 hasLocation W43081179811 @default.
• W4308117981 hasOpenAccess W4308117981 @default.
• W4308117981 hasPrimaryLocation W43081179811 @default.
• W4308117981 hasRelatedWork W2071423018 @default.
• W4308117981 hasRelatedWork W2107259236 @default.
• W4308117981 hasRelatedWork W2159166122 @default.
• W4308117981 hasRelatedWork W2567440351 @default.
• W4308117981 hasRelatedWork W2968868265 @default.

• next