FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2015236469> ?p ?o ?g. }

• W2015236469 endingPage "918" @default.
• W2015236469 startingPage "912" @default.
• W2015236469 abstract "We investigate the relative intensities of the two moderately bright Be-like 2s2 1S0-2s2p 3P1 and 2s2p 1P1-2p2 1D2 lines as a function of electron temperature. We show that the intensity ratios of the lines in the beryllium isoelectronic sequence from C III to Ni XXV ions can serve as sensitive temperature indicators for a large variety of solar plasmas. While the C III-Ne VII lines can be used to diagnose unresolved fine structures in relatively cold solar atmosphere plasmas [(1-5) × 105 K], the Na VIII-Ar XV ions can be used to diagnose coronal plasmas [(0.8-3) × 106 K], and Ca XVII-Ni XXV lines are useful to measure the temperature in flaring plasmas [(5-16) × 107 K]. We investigate the effects on the temperature determination caused by varying the number of energy levels that are included in the atomic model for the considered ions. It is found that a model that includes the 2l2l' and 2l3l' configurations is sufficient for adequately describing the relevant level populations of the Be-like ions in coronal conditions. We compare theoretical ratios obtained using collisional cross section and transition probability values derived by different theoretical methods. The atomic data are obtained from the CHIANTI database, the Hebrew University Lawrence Livermore Atomic Code (HULLAC) suite of programs, and other available sources in the literature. Finally, we use spectra of an apparently isothermal coronal plasma observed by the Solar Ultraviolet Measurement of Emitted Radiation instrument on the Solar and Heliospheric Observatory to determine the electron temperature of streamer plasma using the HULLAC and CHIANTI atomic data sets. The result is compared with the temperature derived in an earlier study using different methods." @default.
• W2015236469 created "2016-06-24" @default.
• W2015236469 creator A5000926259 @default.
• W2015236469 creator A5064460256 @default.
• W2015236469 creator A5067705520 @default.
• W2015236469 creator A5075035609 @default.
• W2015236469 date "2001-08-01" @default.
• W2015236469 modified "2023-09-25" @default.
• W2015236469 title "Intensity Ratios between the 2<i>s</i>²¹<i>S</i>₀–2<i>s</i>2<i>p</i>³<i>P</i>₁and 2<i>s</i>²<i>p</i>¹<i>P</i>₁–2<i>p</i>²¹<i>D</i>₂Transitions in Be‐like Ions as Electron Temperature Indicators for Solar Upper Atmosphere Plasmas" @default.
• W2015236469 cites W1559719081 @default.
• W2015236469 cites W1564793458 @default.
• W2015236469 cites W1615973393 @default.
• W2015236469 cites W1627579912 @default.
• W2015236469 cites W1970020198 @default.
• W2015236469 cites W1973606979 @default.
• W2015236469 cites W1974752306 @default.
• W2015236469 cites W1981328574 @default.
• W2015236469 cites W1985665347 @default.
• W2015236469 cites W1989432205 @default.
• W2015236469 cites W1990971976 @default.
• W2015236469 cites W1995002037 @default.
• W2015236469 cites W2008823219 @default.
• W2015236469 cites W2014011549 @default.
• W2015236469 cites W2024174781 @default.
• W2015236469 cites W2027290069 @default.
• W2015236469 cites W2033729312 @default.
• W2015236469 cites W2045601761 @default.
• W2015236469 cites W2050979105 @default.
• W2015236469 cites W2051175354 @default.
• W2015236469 cites W2067834034 @default.
• W2015236469 cites W2072557708 @default.
• W2015236469 cites W2087294137 @default.
• W2015236469 cites W2090505269 @default.
• W2015236469 cites W2094453818 @default.
• W2015236469 cites W2095453886 @default.
• W2015236469 cites W2102663545 @default.
• W2015236469 cites W2125109271 @default.
• W2015236469 cites W2479235689 @default.
• W2015236469 cites W3003952908 @default.
• W2015236469 cites W3106398819 @default.
• W2015236469 cites W836244844 @default.
• W2015236469 doi "https://doi.org/10.1086/321599" @default.
• W2015236469 hasPublicationYear "2001" @default.
• W2015236469 type Work @default.
• W2015236469 sameAs 2015236469 @default.
• W2015236469 citedByCount "22" @default.
• W2015236469 countsByYear W20152364692013 @default.
• W2015236469 countsByYear W20152364692014 @default.
• W2015236469 countsByYear W20152364692015 @default.
• W2015236469 countsByYear W20152364692017 @default.
• W2015236469 countsByYear W20152364692018 @default.
• W2015236469 countsByYear W20152364692021 @default.
• W2015236469 crossrefType "journal-article" @default.
• W2015236469 hasAuthorship W2015236469A5000926259 @default.
• W2015236469 hasAuthorship W2015236469A5064460256 @default.
• W2015236469 hasAuthorship W2015236469A5067705520 @default.
• W2015236469 hasAuthorship W2015236469A5075035609 @default.
• W2015236469 hasBestOaLocation W20152364691 @default.
• W2015236469 hasConcept C121332964 @default.
• W2015236469 hasConcept C185544564 @default.
• W2015236469 hasConceptScore W2015236469C121332964 @default.
• W2015236469 hasConceptScore W2015236469C185544564 @default.
• W2015236469 hasIssue "2" @default.
• W2015236469 hasLocation W20152364691 @default.
• W2015236469 hasOpenAccess W2015236469 @default.
• W2015236469 hasPrimaryLocation W20152364691 @default.
• W2015236469 hasRelatedWork W1965779136 @default.
• W2015236469 hasRelatedWork W1972975647 @default.
• W2015236469 hasRelatedWork W1983332724 @default.
• W2015236469 hasRelatedWork W2011020689 @default.
• W2015236469 hasRelatedWork W2016104246 @default.
• W2015236469 hasRelatedWork W2016441982 @default.
• W2015236469 hasRelatedWork W2024051034 @default.
• W2015236469 hasRelatedWork W2127130427 @default.
• W2015236469 hasRelatedWork W2132086913 @default.
• W2015236469 hasRelatedWork W50473424 @default.
• W2015236469 hasVolume "556" @default.
• W2015236469 isParatext "false" @default.
• W2015236469 isRetracted "false" @default.
• W2015236469 magId "2015236469" @default.
• W2015236469 workType "article" @default.