Twinkling
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Twinkling, also called scintillation, is a generic term for variations in apparent brightness, colour, or position of a distant luminous object viewed through a medium.<ref name="intech">Wang, Ting-I; Williams, Donn; "Scintillation technology bests NIST". Template:Webarchive, InTech, May 1, 2005.</ref> If the object lies outside the Earth's atmosphere, as in the case of stars and planets, the phenomenon is termed astronomical scintillation; for objects within the atmosphere, the phenomenon is termed terrestrial scintillation.<ref>"NASA Aerospace Science and Technology Dictionary", NASA.gov.</ref> As one of the three principal factors governing astronomical seeing (the others being light pollution and cloud cover), atmospheric scintillation is defined as variations in illuminance only.
In simple terms, twinkling of stars is caused by the passing of light through different layers of a turbulent atmosphere. Most scintillation effects are caused by anomalous atmospheric refraction caused by small-scale fluctuations in air density usually related to temperature gradients.<ref name="Sofieva Dalaudier Vernin 2013 p. 20120174">Template:Cite journal</ref><ref>VanCleave, Janice; "Stellar Scintillation: Twinkling Stars". JVC's Science Fair Projects, May 2, 2010.</ref> Scintillation effects are always much more pronounced near the horizon than near the zenith (directly overhead),<ref>"Scintillation or Atmospheric Boil", noaa.gov.</ref> since light rays near the horizon must have longer paths through the atmosphere before reaching the observer. Atmospheric twinkling is measured quantitatively using a scintillometer.<ref>Chun, M.; Avila, R; "Turbulence profiling using a scanning scintillometer", Astronomical Site Evaluation in the Visible and Radio Range, Astronomical Society of the Pacific 266:72–78.</ref>
The effects of twinkling are reduced by using a larger receiver aperture; this effect is known as aperture averaging.<ref>Perlot, N.; Fritzsche, D. "Aperture-Averaging – Theory and Measurements", elib – Electronic Library.</ref><ref>Template:Cite journal</ref> Many modern large telescopes also use adaptive optical systems which precisely deform the figure of a mirror in order to compensate for scintillation.<ref>Template:Cite journal</ref>
While light from stars and other astronomical objects is likely to twinkle,<ref>Template:Cite book</ref> twinkling usually does not cause images of planets to flicker appreciably.<ref>Kenyon, S. L.; Lawrence, M. et al; "Atmospheric Scintillation at Dome C, Antarctica", Astronomical Society of the Pacific 118, 924–932.</ref><ref>Template:Cite journal</ref> Stars twinkle because they are so far from Earth that they appear as point sources of light easily disturbed by Earth's atmospheric turbulence, which acts like lenses and prisms diverting the light's path. Large astronomical objects closer to Earth, like the Moon and other planets, can be resolved as objects with observable diameters. With multiple observed points of light traversing the atmosphere, their light's deviations average out and the viewer perceives less variation in light coming from them.<ref>Graham, John A. "Why do stars twinkle?" Scientific American, October 2005.</ref><ref>Byrd, Deborah; "Why don’t planets twinkle as stars do?", Earthsky, October 24, 2005.</ref>
See alsoEdit
- Adaptive optics
- Interplanetary scintillation
- Observational astronomy
- Twinkle, Twinkle, Little Star
- Twelve Variations on "Ah vous dirai-je, Maman"