FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W2021896128> ?p ?o ?g. }

• W2021896128 endingPage "283" @default.
• W2021896128 startingPage "276" @default.
• W2021896128 abstract "In principle, the temperatures of solar upper atmosphere plasmas can be derived from the degree of ionization of the ions in the plasma and also from intensity ratios of properly selected lines within particular ions. When such comparisons are made, more often than not discrepancies between the two methods appear. The reason for the discrepancies may be due to wrong assumptions regarding the atomic processes that occur in the emitting plasma or to inaccuracies in the atomic cross-sections used in deriving the temperature sensitive line intensity ratios. This paper presents several types of spectral lines for which their intensity ratios are expected to be sensitive to the temperature of solar plasmas. However, before the diagnostic capabilities of these lines can be explored, the dependency of intensity ratios on temperature needs to be established from a well-understood laboratory measurement. It is proposed that attempts be made to measure some of the listed intensity ratios as a function of electron beam energy in an Electron Beam Ion Trap (EBIT) machine." @default.
• W2021896128 created "2016-06-24" @default.
• W2021896128 creator A5064460256 @default.
• W2021896128 date "2001-04-01" @default.
• W2021896128 modified "2023-10-18" @default.
• W2021896128 title "EBIT Measurements that Can Help Establish the Excitation Conditions in Hot Solar Upper Atmosphere Plasmas" @default.
• W2021896128 cites W1564793458 @default.
• W2021896128 cites W1968625479 @default.
• W2021896128 cites W1969141487 @default.
• W2021896128 cites W1969848295 @default.
• W2021896128 cites W1970020198 @default.
• W2021896128 cites W1974007549 @default.
• W2021896128 cites W1980276189 @default.
• W2021896128 cites W1981695348 @default.
• W2021896128 cites W1982223556 @default.
• W2021896128 cites W1984837465 @default.
• W2021896128 cites W1989432205 @default.
• W2021896128 cites W1996460874 @default.
• W2021896128 cites W1997839360 @default.
• W2021896128 cites W1998842152 @default.
• W2021896128 cites W1999942313 @default.
• W2021896128 cites W2000431444 @default.
• W2021896128 cites W2003666105 @default.
• W2021896128 cites W2005613973 @default.
• W2021896128 cites W2014908324 @default.
• W2021896128 cites W2027400180 @default.
• W2021896128 cites W2030505820 @default.
• W2021896128 cites W2032617549 @default.
• W2021896128 cites W2039107394 @default.
• W2021896128 cites W2059618400 @default.
• W2021896128 cites W2065926768 @default.
• W2021896128 cites W2089024771 @default.
• W2021896128 cites W2092740267 @default.
• W2021896128 cites W2095338645 @default.
• W2021896128 cites W2124368422 @default.
• W2021896128 cites W2125109271 @default.
• W2021896128 cites W2313648145 @default.
• W2021896128 cites W3003952908 @default.
• W2021896128 cites W3034593516 @default.
• W2021896128 cites W4231305900 @default.
• W2021896128 cites W4233590929 @default.
• W2021896128 cites W4248600500 @default.
• W2021896128 cites W4253285497 @default.
• W2021896128 doi "https://doi.org/10.1238/physica.regular.063a00276" @default.
• W2021896128 hasPublicationYear "2001" @default.
• W2021896128 type Work @default.
• W2021896128 sameAs 2021896128 @default.
• W2021896128 citedByCount "4" @default.
• W2021896128 countsByYear W20218961282019 @default.
• W2021896128 crossrefType "journal-article" @default.
• W2021896128 hasAuthorship W2021896128A5064460256 @default.
• W2021896128 hasConcept C120665830 @default.
• W2021896128 hasConcept C121332964 @default.
• W2021896128 hasConcept C1276947 @default.
• W2021896128 hasConcept C145148216 @default.
• W2021896128 hasConcept C147120987 @default.
• W2021896128 hasConcept C153294291 @default.
• W2021896128 hasConcept C168834538 @default.
• W2021896128 hasConcept C184779094 @default.
• W2021896128 hasConcept C185544564 @default.
• W2021896128 hasConcept C192562407 @default.
• W2021896128 hasConcept C198291218 @default.
• W2021896128 hasConcept C198352243 @default.
• W2021896128 hasConcept C22175881 @default.
• W2021896128 hasConcept C2524010 @default.
• W2021896128 hasConcept C2781126634 @default.
• W2021896128 hasConcept C30475298 @default.
• W2021896128 hasConcept C33923547 @default.
• W2021896128 hasConcept C4839761 @default.
• W2021896128 hasConcept C62520636 @default.
• W2021896128 hasConcept C65440619 @default.
• W2021896128 hasConcept C82706917 @default.
• W2021896128 hasConcept C83581075 @default.
• W2021896128 hasConcept C93038891 @default.
• W2021896128 hasConcept C95312477 @default.
• W2021896128 hasConceptScore W2021896128C120665830 @default.
• W2021896128 hasConceptScore W2021896128C121332964 @default.
• W2021896128 hasConceptScore W2021896128C1276947 @default.
• W2021896128 hasConceptScore W2021896128C145148216 @default.
• W2021896128 hasConceptScore W2021896128C147120987 @default.
• W2021896128 hasConceptScore W2021896128C153294291 @default.
• W2021896128 hasConceptScore W2021896128C168834538 @default.
• W2021896128 hasConceptScore W2021896128C184779094 @default.
• W2021896128 hasConceptScore W2021896128C185544564 @default.
• W2021896128 hasConceptScore W2021896128C192562407 @default.
• W2021896128 hasConceptScore W2021896128C198291218 @default.
• W2021896128 hasConceptScore W2021896128C198352243 @default.
• W2021896128 hasConceptScore W2021896128C22175881 @default.
• W2021896128 hasConceptScore W2021896128C2524010 @default.
• W2021896128 hasConceptScore W2021896128C2781126634 @default.
• W2021896128 hasConceptScore W2021896128C30475298 @default.
• W2021896128 hasConceptScore W2021896128C33923547 @default.
• W2021896128 hasConceptScore W2021896128C4839761 @default.
• W2021896128 hasConceptScore W2021896128C62520636 @default.
• W2021896128 hasConceptScore W2021896128C65440619 @default.
• W2021896128 hasConceptScore W2021896128C82706917 @default.
• W2021896128 hasConceptScore W2021896128C83581075 @default.
• W2021896128 hasConceptScore W2021896128C93038891 @default.

• next