FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3103274077> ?p ?o ?g. }

• W3103274077 endingPage "15" @default.
• W3103274077 startingPage "15" @default.
• W3103274077 abstract "We present the general properties of the far-ultraviolet (FUV; 1370–1710 Å) continuum background over most of the sky, obtained with the Spectroscopy of Plasma Evolution from Astrophysical Radiation (SPEAR) instrument (also known as FIMS), flown aboard the STSAT-1 satellite mission. We find that the diffuse FUV continuum intensity is well correlated with NH i, 100 μm, and Hα intensities but anti-correlated with soft X-ray intensity. The correlation of the diffuse background with the direct stellar flux is weaker than the correlation with other parameters. The continuum spectra are relatively flat. However, a weak softening of the FUV spectra toward some sight lines, mostly at high Galactic latitudes, is found not only in direct stellar but also in diffuse background spectra. The diffuse background is relatively softer than the direct stellar spectrum. We also find that the diffuse FUV background averaged over the sky has a bit softer spectrum compared to direct stellar radiation. A map of the ratio of 1370–1520 Å to 1560–1710 Å band intensity shows that the sky is divided into roughly two parts. However, this map shows a lot of patchy structures on small scales. The spatial variation of the hardness ratio seems to be largely determined by the longitudinal distribution of OB-type stars in the Galactic plane. A correlation of the hardness ratio with the FUV intensity is found at high intensities but an anti-correlation is found at low intensities. We also find evidence that the FUV intensity distribution is log-normal in nature." @default.
• W3103274077 created "2020-11-23" @default.
• W3103274077 creator A5006673585 @default.
• W3103274077 creator A5022961030 @default.
• W3103274077 creator A5029382046 @default.
• W3103274077 creator A5030371304 @default.
• W3103274077 creator A5034326826 @default.
• W3103274077 creator A5044366449 @default.
• W3103274077 creator A5046443475 @default.
• W3103274077 creator A5056385826 @default.
• W3103274077 creator A5069926210 @default.
• W3103274077 date "2011-09-20" @default.
• W3103274077 modified "2023-09-24" @default.
• W3103274077 title "OBSERVATION OF THE FAR-ULTRAVIOLET CONTINUUM BACKGROUND WITH SPEAR/FIMS" @default.
• W3103274077 cites W114694543 @default.
• W3103274077 cites W1554404447 @default.
• W3103274077 cites W1864437707 @default.
• W3103274077 cites W1868184765 @default.
• W3103274077 cites W1901242835 @default.
• W3103274077 cites W1939846958 @default.
• W3103274077 cites W1967095196 @default.
• W3103274077 cites W1968045620 @default.
• W3103274077 cites W1969573927 @default.
• W3103274077 cites W1971531178 @default.
• W3103274077 cites W1976515596 @default.
• W3103274077 cites W1976579441 @default.
• W3103274077 cites W1979905105 @default.
• W3103274077 cites W1980145009 @default.
• W3103274077 cites W1982480143 @default.
• W3103274077 cites W1982655690 @default.
• W3103274077 cites W1987467220 @default.
• W3103274077 cites W1989292520 @default.
• W3103274077 cites W1992864467 @default.
• W3103274077 cites W1995232986 @default.
• W3103274077 cites W1998949119 @default.
• W3103274077 cites W2002606918 @default.
• W3103274077 cites W2004757408 @default.
• W3103274077 cites W2011878313 @default.
• W3103274077 cites W2012720914 @default.
• W3103274077 cites W2017064550 @default.
• W3103274077 cites W2017139529 @default.
• W3103274077 cites W2019134034 @default.
• W3103274077 cites W2019579421 @default.
• W3103274077 cites W2025423306 @default.
• W3103274077 cites W2026734549 @default.
• W3103274077 cites W2027437172 @default.
• W3103274077 cites W2028220795 @default.
• W3103274077 cites W2028601982 @default.
• W3103274077 cites W2029623000 @default.
• W3103274077 cites W2029858814 @default.
• W3103274077 cites W2031166418 @default.
• W3103274077 cites W2031667343 @default.
• W3103274077 cites W2032066446 @default.
• W3103274077 cites W2033550193 @default.
• W3103274077 cites W2034608771 @default.
• W3103274077 cites W2036668029 @default.
• W3103274077 cites W2037051410 @default.
• W3103274077 cites W2037131602 @default.
• W3103274077 cites W2038283347 @default.
• W3103274077 cites W2040241222 @default.
• W3103274077 cites W2043225419 @default.
• W3103274077 cites W2046558475 @default.
• W3103274077 cites W2051816764 @default.
• W3103274077 cites W2052101749 @default.
• W3103274077 cites W2052926897 @default.
• W3103274077 cites W2056504659 @default.
• W3103274077 cites W2060204629 @default.
• W3103274077 cites W2067884381 @default.
• W3103274077 cites W2069417155 @default.
• W3103274077 cites W2071120135 @default.
• W3103274077 cites W2075222279 @default.
• W3103274077 cites W2079245469 @default.
• W3103274077 cites W2080967593 @default.
• W3103274077 cites W2082179897 @default.
• W3103274077 cites W2084844372 @default.
• W3103274077 cites W2085389248 @default.
• W3103274077 cites W2089798086 @default.
• W3103274077 cites W2090913213 @default.
• W3103274077 cites W2100696415 @default.
• W3103274077 cites W2111817932 @default.
• W3103274077 cites W2133725650 @default.
• W3103274077 cites W2133791001 @default.
• W3103274077 cites W2138942709 @default.
• W3103274077 cites W2157040099 @default.
• W3103274077 cites W2157421053 @default.
• W3103274077 cites W2163946872 @default.
• W3103274077 cites W2164355923 @default.
• W3103274077 cites W2170691558 @default.
• W3103274077 cites W3023717689 @default.
• W3103274077 cites W3098389726 @default.
• W3103274077 cites W3098603160 @default.
• W3103274077 cites W3098662408 @default.
• W3103274077 cites W3098685356 @default.
• W3103274077 cites W3100852565 @default.
• W3103274077 cites W3101451826 @default.
• W3103274077 cites W3104257347 @default.
• W3103274077 cites W3104647164 @default.
• W3103274077 cites W3104752565 @default.

• next