FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2484613426> ?p ?o ?g. }

• W2484613426 abstract "Abstract In the conventional pole figure, an accurate representation can be attained by correcting the observed X-ray diffraction intensity for any change in diffraction geometry and by comparing this with the correctly established standard intensity. For the intensity corrections, ASTM has prescribed the method of Decker et al . In practice, however, the validity of the correction formula is uncertain, since the prerequisite is difficult to attain for parallelism of an incident beam of sufficient intensity. For the standard intensity, it is desirable to take the intensity obtained with the randomly oriented material of the same composition. However, in most cases an arbitrary unit has been taken because of the difficulty in getting a truly random and uniform sample. Under these circumstances, it is first necessary for an accurate representation of pole figures to make a random sample of uniform thickness for the standard. The authors have obtained satisfactory standard samples by sintering the randomly oriented iron powder made from iron chloride and made use of them to check the method of intensity correction. Satisfactory results are obtained in the randomness tests, such as the comparison of the relative intensity diffracted from the crystal planes parallel to the sample surface and the fluctuation of diffraction intensity during α rotation. In the reflection case by the Schulz method, the (110) reflection intensity of a random sample, by Co K α radiation, is independent of the tilting angle up to 50°. The other reflections do not give a constant intensity for the wide range of the tilting angles because of dispersion of the diffracted beam due to the wider separation of K α doublet in the higher reflection angle and the wider irradiated area at the lower angles. In the transmission case Schulz's correction formula is in good agreement with the observed values for the various diffraction lines and the samples of various µ t, while the Decker-Harker formula does not give the absorption change with α -rotation even by an incident beam of ⅙° divergence. In both cases, an accurate determination of pole densities is made by comparing the diffraction intensity of the standard sample substituted in place of the test specimen and by correcting the absorption change due to the difference of µ t between the standard and test sample, which affords good coincidence in the overlapped region. The pole figure obtained by the above method furnishes an accurate prediction of plastic and elastic anisotropy in sheet metals." @default.
• W2484613426 created "2016-08-23" @default.
• W2484613426 creator A5001250802 @default.
• W2484613426 creator A5016837296 @default.
• W2484613426 creator A5085012855 @default.
• W2484613426 date "1966-01-01" @default.
• W2484613426 modified "2023-09-26" @default.
• W2484613426 title "Improvement of Accuracy in Representation of Conventional Pole Figures" @default.
• W2484613426 cites W1973350594 @default.
• W2484613426 cites W1979667457 @default.
• W2484613426 cites W1982920331 @default.
• W2484613426 cites W2004704850 @default.
• W2484613426 cites W2047199540 @default.
• W2484613426 cites W2089032275 @default.
• W2484613426 cites W2564500963 @default.
• W2484613426 cites W2605379478 @default.
• W2484613426 doi "https://doi.org/10.1154/s0376030800004511" @default.
• W2484613426 hasPublicationYear "1966" @default.
• W2484613426 type Work @default.
• W2484613426 sameAs 2484613426 @default.
• W2484613426 citedByCount "2" @default.
• W2484613426 crossrefType "journal-article" @default.
• W2484613426 hasAuthorship W2484613426A5001250802 @default.
• W2484613426 hasAuthorship W2484613426A5016837296 @default.
• W2484613426 hasAuthorship W2484613426A5085012855 @default.
• W2484613426 hasConcept C105795698 @default.
• W2484613426 hasConcept C120665830 @default.
• W2484613426 hasConcept C121332964 @default.
• W2484613426 hasConcept C125112378 @default.
• W2484613426 hasConcept C198531522 @default.
• W2484613426 hasConcept C199360897 @default.
• W2484613426 hasConcept C207114421 @default.
• W2484613426 hasConcept C2524010 @default.
• W2484613426 hasConcept C33923547 @default.
• W2484613426 hasConcept C41008148 @default.
• W2484613426 hasConcept C65682993 @default.
• W2484613426 hasConcept C74050887 @default.
• W2484613426 hasConcept C93038891 @default.
• W2484613426 hasConcept C97355855 @default.
• W2484613426 hasConceptScore W2484613426C105795698 @default.
• W2484613426 hasConceptScore W2484613426C120665830 @default.
• W2484613426 hasConceptScore W2484613426C121332964 @default.
• W2484613426 hasConceptScore W2484613426C125112378 @default.
• W2484613426 hasConceptScore W2484613426C198531522 @default.
• W2484613426 hasConceptScore W2484613426C199360897 @default.
• W2484613426 hasConceptScore W2484613426C207114421 @default.
• W2484613426 hasConceptScore W2484613426C2524010 @default.
• W2484613426 hasConceptScore W2484613426C33923547 @default.
• W2484613426 hasConceptScore W2484613426C41008148 @default.
• W2484613426 hasConceptScore W2484613426C65682993 @default.
• W2484613426 hasConceptScore W2484613426C74050887 @default.
• W2484613426 hasConceptScore W2484613426C93038891 @default.
• W2484613426 hasConceptScore W2484613426C97355855 @default.
• W2484613426 hasLocation W24846134261 @default.
• W2484613426 hasOpenAccess W2484613426 @default.
• W2484613426 hasPrimaryLocation W24846134261 @default.
• W2484613426 hasRelatedWork W164515664 @default.
• W2484613426 hasRelatedWork W1971382505 @default.
• W2484613426 hasRelatedWork W1993343568 @default.
• W2484613426 hasRelatedWork W2013276457 @default.
• W2484613426 hasRelatedWork W2021705581 @default.
• W2484613426 hasRelatedWork W2024912802 @default.
• W2484613426 hasRelatedWork W2033791606 @default.
• W2484613426 hasRelatedWork W2036111268 @default.
• W2484613426 hasRelatedWork W2041273792 @default.
• W2484613426 hasRelatedWork W2068500495 @default.
• W2484613426 hasRelatedWork W2072288630 @default.
• W2484613426 hasRelatedWork W2079730329 @default.
• W2484613426 hasRelatedWork W2112854926 @default.
• W2484613426 hasRelatedWork W2137121637 @default.
• W2484613426 hasRelatedWork W2325645639 @default.
• W2484613426 hasRelatedWork W2327357066 @default.
• W2484613426 hasRelatedWork W2330188595 @default.
• W2484613426 hasRelatedWork W2479181238 @default.
• W2484613426 hasRelatedWork W2396811011 @default.
• W2484613426 hasRelatedWork W2879539272 @default.
• W2484613426 isParatext "false" @default.
• W2484613426 isRetracted "false" @default.
• W2484613426 magId "2484613426" @default.
• W2484613426 workType "article" @default.