Then, without warning, these structures can erupt and blow large amounts of gas and plasma out into space. How to use filament in a sentence. (See fall.) These areas are pulled by magnetic fields that are generated by sunspots. CallUrl('www>robgendlerastropics>comhtml',0), Lerner gives the example of ~TildeLink()s or sheets 150 million light years apart in Figure 1.1, and then asserts that material would have to travel 270 million light years to make the structure. CallUrl('www>astromart>comasp?news_id=864',1), Galactic ~TildeLink()sA distribution of galaxies simulated using the Swinburne supercomputer. They are suspended above the surface of the sun by loops of magnetic fields. Their causes are uncertain but probably involve magnetic forces. Filamentary definition, pertaining to or of the nature of a filament. allgemein eine einzelne Faser beliebiger Länge; Filament (Textilfaser), die internationale Bezeichnung für Fasern mit praktisch unbegrenzter Länge Chemiefaser; Glasfaser; ein Glühfaden zur Emission von Elektronen, siehe Glühkathode; Astronomie: eine Protuberanz – ein fadenförmiges Gasgebilde in der Astronomie … It is possible for a projection to be both a filament and a prominence. What is the definition of filament? ~TildeLink()s are generally cool. Filaments are most easily seen in photos of the Sun taken with a filter that only transmits a specific wavelength of red light. This formation is instead called a solar filament. n. 1. Learn more. In physical cosmology, galaxy filaments (subtypes: supercluster complexes, galaxy walls, and galaxy sheets)[1][2] are the largest known structures in the universe. They provide important clues about how giant black holes affect their surrounding environment. Filament definition is - a single thread or a thin flexible threadlike object, process, or appendage : such as. A ~TildeLink() is a prominence projected on the solar disk. CallUrl('naasbeginners>co>ukhtm',0), ~TildeLink()a strand of cool gas suspended over the photosphere by magnetic fields, which appears dark as seen against the disk of the Sun.Findera small, wide-field telescope attached to a larger telescope. Instead (see section S-4), it is concentrated in narrow ranges of color ("spectral lines") which depend on the atoms from which they came. CallUrl('solar-center>stanford>eduhtml',0), ~TildeLink() cavities are zones which look dark in the X-rays and are above the regions where Hα ~TildeLink()s are observed in the chromosphere. CallUrl('www>universetoday>comspace>com<58-the-sun-formation-facts-and-characteristics>html',1), Thin, wispy, ~TildeLink()ous, or curlyMostly composed of ice crystalsAbove 18,000 feet(High-altitude clouds)Cirro-cumulus Cc ... CallUrl('www>allaboutspace>comphysicsoftheuniverse>comhtml',1), A fresh video from the Herschel space observatory discloses a group of bright spots, thin ~TildeLink()s and bubbling nebulae alongside the diffuse background of the interstellar material. CallUrl('curious>astro>cornell>eduorgspacetoday>orghtml',0), ~TildeLink()A strand of cool gas suspended over the photosphere by magnetic fields, which appears dark as seen against the disk of the Sun.Finder ... CallUrl('www>stargayzers>orghtml',0), ~TildeLink()s and prominences can remain stable for weeks or even months. CallUrl('jtg>sjrdesign>nethtml',0), ~TildeLink()s of gas and dust form a web-like cocoon known as the Crab Nebula in the constellation Taurus in this image from Hubble Space Telescope. It is emitted by hydrogen atoms, the main constituent of the Sun. CallUrl('solarviews>comhtm',0), Huge ~TildeLink()s of dark matter have been detected in a survey of thousands of distant galaxies. filaments 1. These are dense, somewhat cooler, clouds of material that are suspended above the solar surface by loops of magnetic field. [3] Filaments consist of gravitationally bound galaxies. They were formerly sometimes called dark flocculi . CallUrl('www>aanda>orghtml',1), ~TildeLink()s and Plage~TildeLink()s are dark, thread-like features seen in the red light of hydrogen (H-alpha). These structures form giant ~TildeLink()s and ... CallUrl('mcdonaldobservatory>orgastronomy>ohio-state>edu<~poggehtml',0), Commenting on its latest Horsehead Nebula images, Prof Matt Griffin explained: "You can see all the things we look for in Herschel images; the ~TildeLink()s, the bubbles; the wispy material, the reddish material that hasn't yet actually started to form stars. The. As the shock wave slows down, it loses energy by emitting visible light.Personal View ... 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