FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W4221017648> ?p ?o ?g. }

• W4221017648 endingPage "18" @default.
• W4221017648 startingPage "18" @default.
• W4221017648 abstract "We input solar wind parameters responsible for the main phases of 15 great geomagnetic storms (GGSs: $Delta$SYM-H$le-$200 nT) into the empirical formulae created by cite{Burton1975}(hereafter Burton equation), and by cite{OBrien2000}(hereafter OM equation) to evaluate whether textbf{two equations} can correctly estimate the intensities of GGSs. The results show that the intensities of most GGSs estimated by OM equation are much smaller than the observed intensities. The RMS error between the intensities estimated by OM equation and the observed intensities is textbf{203} nT, implying that the estimated storm intensity deviates significantly from the observed one. The RMS error between the intensities estimated by Burton equation and the observed intensities is 130.8 nT. The relative error caused by Burton equation for the storms with intensities $Delta$SYM-H$<$-400 nT is larger than 27%, implying that the absolute error will be large for the storms with $Delta$SYM-H$<$-400 nT. The results indicate that the two equations cannot work effectively in the estimation of GGSs. On the contrary, the intensity of a GGS estimated by the empirical formula created by cite{WangCB2003} can always be very close to the observed one if we select the right weight for solar wind dynamic pressure, proving that solar wind dynamic pressure is an important factor for GGS intensity, but it is overlooked in the ring current injection terms of Burton equation or OM equation. This is the reason why the two equations cannot work effectively in the estimation of GGSs." @default.
• W4221017648 created "2022-04-03" @default.
• W4221017648 creator A5022899104 @default.
• W4221017648 creator A5034358836 @default.
• W4221017648 creator A5066375848 @default.
• W4221017648 date "2022-03-01" @default.
• W4221017648 modified "2023-09-28" @default.
• W4221017648 title "Can We Estimate the Intensities of Great Geomagnetic Storms (ΔSYM-H ≤ −200 nT) with the Burton Equation or the O’Brien and McPherron Equation?" @default.
• W4221017648 cites W1545771930 @default.
• W4221017648 cites W1548928142 @default.
• W4221017648 cites W1928092027 @default.
• W4221017648 cites W1965057733 @default.
• W4221017648 cites W1965919891 @default.
• W4221017648 cites W1970488982 @default.
• W4221017648 cites W1974798730 @default.
• W4221017648 cites W1977658572 @default.
• W4221017648 cites W1986396546 @default.
• W4221017648 cites W1987495055 @default.
• W4221017648 cites W1988167844 @default.
• W4221017648 cites W1991191639 @default.
• W4221017648 cites W1997912130 @default.
• W4221017648 cites W2006488078 @default.
• W4221017648 cites W2023831893 @default.
• W4221017648 cites W2025451149 @default.
• W4221017648 cites W2032650292 @default.
• W4221017648 cites W2039714137 @default.
• W4221017648 cites W2040798260 @default.
• W4221017648 cites W2047385385 @default.
• W4221017648 cites W2072579688 @default.
• W4221017648 cites W2076172640 @default.
• W4221017648 cites W2087594811 @default.
• W4221017648 cites W2089356175 @default.
• W4221017648 cites W2091177078 @default.
• W4221017648 cites W2093298685 @default.
• W4221017648 cites W2093661103 @default.
• W4221017648 cites W2116215979 @default.
• W4221017648 cites W2135234482 @default.
• W4221017648 cites W2142025025 @default.
• W4221017648 cites W2154635195 @default.
• W4221017648 cites W2161975006 @default.
• W4221017648 cites W2417317418 @default.
• W4221017648 cites W2562647817 @default.
• W4221017648 cites W2591123938 @default.
• W4221017648 cites W2596430013 @default.
• W4221017648 cites W2734595147 @default.
• W4221017648 cites W2755381497 @default.
• W4221017648 cites W2944673805 @default.
• W4221017648 cites W2960804062 @default.
• W4221017648 cites W2964281925 @default.
• W4221017648 cites W2992545530 @default.
• W4221017648 cites W3008924826 @default.
• W4221017648 cites W3048142023 @default.
• W4221017648 cites W3104093601 @default.
• W4221017648 cites W3113679799 @default.
• W4221017648 cites W3120273548 @default.
• W4221017648 cites W3120547459 @default.
• W4221017648 cites W3123838461 @default.
• W4221017648 cites W3124032888 @default.
• W4221017648 cites W3139051242 @default.
• W4221017648 cites W3154229837 @default.
• W4221017648 cites W3163290109 @default.
• W4221017648 cites W3206287090 @default.
• W4221017648 cites W4200174252 @default.
• W4221017648 cites W4248814915 @default.
• W4221017648 doi "https://doi.org/10.3847/1538-4357/ac50a8" @default.
• W4221017648 hasPublicationYear "2022" @default.
• W4221017648 type Work @default.
• W4221017648 citedByCount "5" @default.
• W4221017648 countsByYear W42210176482022 @default.
• W4221017648 countsByYear W42210176482023 @default.
• W4221017648 crossrefType "journal-article" @default.
• W4221017648 hasAuthorship W4221017648A5022899104 @default.
• W4221017648 hasAuthorship W4221017648A5034358836 @default.
• W4221017648 hasAuthorship W4221017648A5066375848 @default.
• W4221017648 hasBestOaLocation W42210176481 @default.
• W4221017648 hasConcept C108411613 @default.
• W4221017648 hasConcept C115260700 @default.
• W4221017648 hasConcept C121332964 @default.
• W4221017648 hasConcept C170641098 @default.
• W4221017648 hasConcept C199635899 @default.
• W4221017648 hasConcept C37914503 @default.
• W4221017648 hasConcept C62520636 @default.
• W4221017648 hasConcept C93038891 @default.
• W4221017648 hasConcept C9844520 @default.
• W4221017648 hasConceptScore W4221017648C108411613 @default.
• W4221017648 hasConceptScore W4221017648C115260700 @default.
• W4221017648 hasConceptScore W4221017648C121332964 @default.
• W4221017648 hasConceptScore W4221017648C170641098 @default.
• W4221017648 hasConceptScore W4221017648C199635899 @default.
• W4221017648 hasConceptScore W4221017648C37914503 @default.
• W4221017648 hasConceptScore W4221017648C62520636 @default.
• W4221017648 hasConceptScore W4221017648C93038891 @default.
• W4221017648 hasConceptScore W4221017648C9844520 @default.
• W4221017648 hasFunder F4320338178 @default.
• W4221017648 hasIssue "1" @default.
• W4221017648 hasLocation W42210176481 @default.
• W4221017648 hasLocation W42210176482 @default.
• W4221017648 hasOpenAccess W4221017648 @default.

• next