How to use fadings in a sentence? Find typical usage patterns (collocations)/phrases/context for "fadings" and check conjugation/comparative form for "fadings". Mastering all the usages of "fadings" from sentence examples published by news publications.
The 'Virginia Reel' and 'fadings', 'The Fading' or 'With a fading' - ("A Winter's Tale" Act IV) mentioned by William Shakespeare in A Winter's Tale have been associated with rince fada.
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The constant features are prominent carbon lines, strong atmospheric hydrogen deficiencies, and obviously the intermittent fadings. The DY Persei variables have been considered a sub-class of R CrB variable, although they are less luminous carbon-rich AGB stars and may be unrelated.
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Not a single note of the original's text is being altered, nothing is added, nothing is omitted, nothing is being changed in any way. The electronics on the other hand solely consist of amplification. No additional sound whatsoever is being produced. The possibilities of interference span a large variety of movements, from almost inaudibly slow fadings to extremely fast and brutal chopping.
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It is this which is often referred to as the Appleton Layer as is responsible for enabling most long range short wave telecommunication. The magneto-ionic theory also allowed Appleton to explain the origin of the mysterious fadings heard on the radio around sunset. During the day, the light from the sun causes the molecules in the air to become ionised even at fairly low altitudes.
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This means absorption rates diminish and waves can be reflected with sufficient strengths to be noticed, leading to the interference phenomena we have mentioned. For these interference patterns to occur though, there must not simply be the presence of a reflected wave but a change in the reflected wave. Otherwise the interference is constant and fadings would not be heard. The received signal would simply be louder or softer than during the day.
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FG Sagittae is the central star of the planetary nebula Henize 1-5. Since 1992 the star has exhibited fadings and recoveries similar to that of a R Coronae Borealis variable star; this behavior is emphasized by a hydrogen deficiency typical for this class of stars. It has been proposed that this star has undergone a "late thermal pulse" (LTP) of helium fusion after having left the asymptotic giant branch (AGB) to move towards the hottest end of the "white dwarf cooling track". This thermal pulse is believed to have revived this aged star to once again, for a short time, behave as an AGB star.
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Of this diverse class of stars, some Orion variables may exhibit a small amplitude (up to 1 magnitude) periodic variation, some are characterized by abrupt fadings, and some show spectral characteristics indicating mass downfall upon the star (YY Orionis stars). Many of these characteristics may occur in any one Orion variable. The term 'Orion Variable' was a handy catch-all term but is now tending to drop out of disuse among the astronomical community, though for historical reasons the GCVS still uses it. Astronomers use more specialised terms which refer to actual physical differences among the 'zoo' of young variable stars, such as 'Classical T Tauri' or 'UX Orionis' stars.
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Visual light curve for RY Sagittarii, 1988–2015, showing classic behaviour for this type of variable An R Coronae Borealis variable (abbreviated RCB, R CrB) is an eruptive variable star that varies in luminosity in two modes, one low amplitude pulsation (a few tenths of a magnitude), and one irregular, unpredictably-sudden fading by 1 to 9 magnitudes. The prototype star R Coronae Borealis was discovered by the English amateur astronomer Edward Pigott in 1795, who first observed the enigmatic fadings of the star. Only about 150 RCB stars are currently known in our Galaxy while up to 1000 were expected, making this class a very rare kind of star. It is increasingly suspected that R Coronae Borealis (RCB) stars – rare hydrogen-deficient and carbon-rich supergiant stars – are the product of mergers of white-dwarfs in the intermediary mass regime (total mass between 0.6 and 1.2 ).
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