FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2126269410> ?p ?o ?g. }

• W2126269410 endingPage "673" @default.
• W2126269410 startingPage "657" @default.
• W2126269410 abstract "Remanent and induced magnetization occurs in crustal materials when they are below their Curie temperature, and we consider the problem of determining the magnetic field originating in the earth's core in the presence of such magnetization. Simple physical models of induced magnetization which have been proposed and which lead to deterministic effects account for only a small proportion of the high-degree internal field found using Magsat data, and thus a stochastic description appears more useful. We investigate the effect of remanent magnetization in the crust on satellite measurements of the core magnetic field by posing the question: if the crustal magnetization is correlated only on the shortest possible length-scale, and different components are uncorrelated everywhere, what is the correlation lengthscale at a radius above the earth's surface? Using an idea due to Parker (1988), we model the crust as a zero-mean, stationary, Gaussian random process. We show that the matrix of second-order statistics is proportional to the Gram matrix, which depends only on the inner-products of the appropriate Green's functions, and that at a typical satellite altitude of 400 km the data are correlated out to an angular separation of approximately 15°. Accurate and efficient means of calculating the matrix elements are given. This theory leads to a more conservative form for the correlation in the data than that previously given by Langel, Estes & Sabaka (1989), whilst not being incommensurate with the imprecisely known high-degree power spectrum. Previous studies examining the core field have treated satellite data as independent, and have given different orthogonal components equal weight. Both these assumptions are incorrect, and we show that the variance of measurements of the radial component of magnetic field due to the crust is expected to be approximately twice that in horizontal components. However, the size of the crustal effect is small compared to the random noise in the data, and may not lead to radically different results from those already published." @default.
• W2126269410 created "2016-06-24" @default.
• W2126269410 creator A5041297653 @default.
• W2126269410 date "1990-12-01" @default.
• W2126269410 modified "2023-09-24" @default.
• W2126269410 title "Accounting for crustal magnetization in models of the core magnetic field" @default.
• W2126269410 cites W1908995290 @default.
• W2126269410 cites W1965491113 @default.
• W2126269410 cites W1980101736 @default.
• W2126269410 cites W2001380498 @default.
• W2126269410 cites W2009888279 @default.
• W2126269410 cites W2010332501 @default.
• W2126269410 cites W2013495059 @default.
• W2126269410 cites W2036547934 @default.
• W2126269410 cites W2040336487 @default.
• W2126269410 cites W2041361095 @default.
• W2126269410 cites W2057811158 @default.
• W2126269410 cites W2060861684 @default.
• W2126269410 cites W2063965548 @default.
• W2126269410 cites W2064673686 @default.
• W2126269410 cites W2068029398 @default.
• W2126269410 cites W2073621729 @default.
• W2126269410 cites W2074452692 @default.
• W2126269410 cites W2077715148 @default.
• W2126269410 cites W2082140545 @default.
• W2126269410 cites W2088455220 @default.
• W2126269410 cites W2096448541 @default.
• W2126269410 cites W2099432206 @default.
• W2126269410 cites W2101048818 @default.
• W2126269410 cites W2105332262 @default.
• W2126269410 cites W2107278393 @default.
• W2126269410 cites W2111847404 @default.
• W2126269410 cites W2111967849 @default.
• W2126269410 cites W2113908912 @default.
• W2126269410 cites W2114164194 @default.
• W2126269410 cites W2114285591 @default.
• W2126269410 cites W2135219576 @default.
• W2126269410 cites W2145630053 @default.
• W2126269410 cites W2151510585 @default.
• W2126269410 cites W2152562544 @default.
• W2126269410 cites W2155011601 @default.
• W2126269410 cites W2169789325 @default.
• W2126269410 cites W4214812258 @default.
• W2126269410 doi "https://doi.org/10.1111/j.1365-246x.1990.tb05678.x" @default.
• W2126269410 hasPublicationYear "1990" @default.
• W2126269410 type Work @default.
• W2126269410 sameAs 2126269410 @default.
• W2126269410 citedByCount "46" @default.
• W2126269410 countsByYear W21262694102012 @default.
• W2126269410 countsByYear W21262694102013 @default.
• W2126269410 countsByYear W21262694102015 @default.
• W2126269410 countsByYear W21262694102018 @default.
• W2126269410 countsByYear W21262694102021 @default.
• W2126269410 countsByYear W21262694102022 @default.
• W2126269410 crossrefType "journal-article" @default.
• W2126269410 hasAuthorship W2126269410A5041297653 @default.
• W2126269410 hasBestOaLocation W21262694101 @default.
• W2126269410 hasConcept C115260700 @default.
• W2126269410 hasConcept C121332964 @default.
• W2126269410 hasConcept C127313418 @default.
• W2126269410 hasConcept C155058782 @default.
• W2126269410 hasConcept C194482375 @default.
• W2126269410 hasConcept C199635899 @default.
• W2126269410 hasConcept C202444582 @default.
• W2126269410 hasConcept C2776698055 @default.
• W2126269410 hasConcept C32546565 @default.
• W2126269410 hasConcept C33923547 @default.
• W2126269410 hasConcept C62520636 @default.
• W2126269410 hasConcept C66944017 @default.
• W2126269410 hasConcept C8058405 @default.
• W2126269410 hasConcept C9652623 @default.
• W2126269410 hasConceptScore W2126269410C115260700 @default.
• W2126269410 hasConceptScore W2126269410C121332964 @default.
• W2126269410 hasConceptScore W2126269410C127313418 @default.
• W2126269410 hasConceptScore W2126269410C155058782 @default.
• W2126269410 hasConceptScore W2126269410C194482375 @default.
• W2126269410 hasConceptScore W2126269410C199635899 @default.
• W2126269410 hasConceptScore W2126269410C202444582 @default.
• W2126269410 hasConceptScore W2126269410C2776698055 @default.
• W2126269410 hasConceptScore W2126269410C32546565 @default.
• W2126269410 hasConceptScore W2126269410C33923547 @default.
• W2126269410 hasConceptScore W2126269410C62520636 @default.
• W2126269410 hasConceptScore W2126269410C66944017 @default.
• W2126269410 hasConceptScore W2126269410C8058405 @default.
• W2126269410 hasConceptScore W2126269410C9652623 @default.
• W2126269410 hasIssue "3" @default.
• W2126269410 hasLocation W21262694101 @default.
• W2126269410 hasOpenAccess W2126269410 @default.
• W2126269410 hasPrimaryLocation W21262694101 @default.
• W2126269410 hasRelatedWork W1977308170 @default.
• W2126269410 hasRelatedWork W1997003100 @default.
• W2126269410 hasRelatedWork W2018376393 @default.
• W2126269410 hasRelatedWork W2039820186 @default.
• W2126269410 hasRelatedWork W2047344370 @default.
• W2126269410 hasRelatedWork W2157366305 @default.
• W2126269410 hasRelatedWork W2162157156 @default.
• W2126269410 hasRelatedWork W2322591626 @default.
• W2126269410 hasRelatedWork W2381323493 @default.

• next