FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2067181472> ?p ?o ?g. }

• W2067181472 endingPage "L66" @default.
• W2067181472 startingPage "L62" @default.
• W2067181472 abstract "The X-ray line intensity ratio 3C/3D in Fe xvii is potentially one of the most useful plasma diagnostic line ratios for X-ray astronomy. Based on our recent converged and highly accurate atomic calculations for electron impact excitation of Fe xvii using the fully relativistic close-coupling method, we demonstrate that 3C/3D in Fe xvii is not a constant with respect to electron temperature/energy. The cascade effects (including the excitation and recombination population pumping) on 3C/3D as a function of temperature (for Maxwellian plasmas) or electron beam energy (for some laboratory plasmas) are studied and elaborated. For Maxwellian plasmas prevailing in astrophysical sources under the condition of collisional ionization equilibrium, a new and highly accurate 3C/3D line ratio is reported. The values of 3C/3D reported in this work are 2.66, 2.76, 2.81, 2.88 and 2.94 for electron temperatures of 2, 3, 4, 6 and 10 MK, respectively. The uncertainty in our new line ratio is estimated to be about 5 per cent. These new 3C/3D values are expected to have immediate applications for a wide range of X-ray spectra observed from both point sources as well as extended sources." @default.
• W2067181472 created "2016-06-24" @default.
• W2067181472 creator A5046372093 @default.
• W2067181472 date "2008-05-01" @default.
• W2067181472 modified "2023-09-23" @default.
• W2067181472 title "X-ray line ratio 3C/3D in Fe xvii" @default.
• W2067181472 cites W129583845 @default.
• W2067181472 cites W1558601041 @default.
• W2067181472 cites W1595731585 @default.
• W2067181472 cites W1616015223 @default.
• W2067181472 cites W1964677281 @default.
• W2067181472 cites W1965324153 @default.
• W2067181472 cites W1984422607 @default.
• W2067181472 cites W1985049707 @default.
• W2067181472 cites W1993244900 @default.
• W2067181472 cites W1995386948 @default.
• W2067181472 cites W1996674820 @default.
• W2067181472 cites W2003732201 @default.
• W2067181472 cites W2006568542 @default.
• W2067181472 cites W2008973800 @default.
• W2067181472 cites W2020287955 @default.
• W2067181472 cites W2028369244 @default.
• W2067181472 cites W2032776783 @default.
• W2067181472 cites W2046374612 @default.
• W2067181472 cites W2048386486 @default.
• W2067181472 cites W2059940261 @default.
• W2067181472 cites W2075080106 @default.
• W2067181472 cites W2075490961 @default.
• W2067181472 cites W2076581452 @default.
• W2067181472 cites W2084265947 @default.
• W2067181472 cites W2094352205 @default.
• W2067181472 cites W2096990639 @default.
• W2067181472 cites W2121537375 @default.
• W2067181472 cites W2138114434 @default.
• W2067181472 cites W2165301651 @default.
• W2067181472 cites W2403195588 @default.
• W2067181472 cites W2443936260 @default.
• W2067181472 cites W3100225361 @default.
• W2067181472 cites W3103079452 @default.
• W2067181472 cites W3104523264 @default.
• W2067181472 cites W3104524692 @default.
• W2067181472 cites W3105311925 @default.
• W2067181472 cites W4300008952 @default.
• W2067181472 cites W4300592266 @default.
• W2067181472 doi "https://doi.org/10.1111/j.1745-3933.2008.00461.x" @default.
• W2067181472 hasPublicationYear "2008" @default.
• W2067181472 type Work @default.
• W2067181472 sameAs 2067181472 @default.
• W2067181472 citedByCount "14" @default.
• W2067181472 countsByYear W20671814722012 @default.
• W2067181472 countsByYear W20671814722013 @default.
• W2067181472 countsByYear W20671814722014 @default.
• W2067181472 countsByYear W20671814722015 @default.
• W2067181472 countsByYear W20671814722019 @default.
• W2067181472 countsByYear W20671814722021 @default.
• W2067181472 crossrefType "journal-article" @default.
• W2067181472 hasAuthorship W2067181472A5046372093 @default.
• W2067181472 hasBestOaLocation W20671814721 @default.
• W2067181472 hasConcept C120665830 @default.
• W2067181472 hasConcept C121332964 @default.
• W2067181472 hasConcept C1276947 @default.
• W2067181472 hasConcept C144024400 @default.
• W2067181472 hasConcept C145148216 @default.
• W2067181472 hasConcept C147120987 @default.
• W2067181472 hasConcept C149923435 @default.
• W2067181472 hasConcept C159985019 @default.
• W2067181472 hasConcept C184779094 @default.
• W2067181472 hasConcept C185544564 @default.
• W2067181472 hasConcept C192562407 @default.
• W2067181472 hasConcept C198291218 @default.
• W2067181472 hasConcept C198352243 @default.
• W2067181472 hasConcept C204323151 @default.
• W2067181472 hasConcept C22175881 @default.
• W2067181472 hasConcept C2524010 @default.
• W2067181472 hasConcept C2779328170 @default.
• W2067181472 hasConcept C2781219984 @default.
• W2067181472 hasConcept C2908647359 @default.
• W2067181472 hasConcept C33923547 @default.
• W2067181472 hasConcept C4839761 @default.
• W2067181472 hasConcept C62520636 @default.
• W2067181472 hasConcept C82706917 @default.
• W2067181472 hasConcept C83581075 @default.
• W2067181472 hasConcept C96141758 @default.
• W2067181472 hasConceptScore W2067181472C120665830 @default.
• W2067181472 hasConceptScore W2067181472C121332964 @default.
• W2067181472 hasConceptScore W2067181472C1276947 @default.
• W2067181472 hasConceptScore W2067181472C144024400 @default.
• W2067181472 hasConceptScore W2067181472C145148216 @default.
• W2067181472 hasConceptScore W2067181472C147120987 @default.
• W2067181472 hasConceptScore W2067181472C149923435 @default.
• W2067181472 hasConceptScore W2067181472C159985019 @default.
• W2067181472 hasConceptScore W2067181472C184779094 @default.
• W2067181472 hasConceptScore W2067181472C185544564 @default.
• W2067181472 hasConceptScore W2067181472C192562407 @default.
• W2067181472 hasConceptScore W2067181472C198291218 @default.
• W2067181472 hasConceptScore W2067181472C198352243 @default.
• W2067181472 hasConceptScore W2067181472C204323151 @default.
• W2067181472 hasConceptScore W2067181472C22175881 @default.

• next