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Corona Borealis, the Northern Crown, is a lovely semi circle of stars centered in the picture and opening to the left. Alphecca, or Gemma, is the bright star at the Crown's center directly in the middle of the picture.
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Coronal loops are the basic structures of the magnetic solar corona. These loops are the closed-magnetic flux cousins of the open-magnetic flux that can be found in coronal hole (polar) regions and the solar wind.
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Corona Borealis, also known as the Corona septentrionalis, and the Northern Crown or Garland, is a constellation of the Northern hemisphere, mentioned by Eudoxus (4th cent. B.C.) and Aratus (3rd cent. B.C.).
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CoronaThe corona is the collection of immediate gases around the Sun. It is extremely hot, much hotter than the surface of the Sun.
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Corona Extra, their most popular brand, is reputedly the number-one selling beer in Mexico, as well as the number one imported beer in the US.
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Corona Austrina Abbreviation: CrA Genitive: Coronae Austrini Translation: The Southern Crown Peoria Astronomical Society Corona Austrina Page Interactive star chart (Java applet) ...
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Corona BorealisTransit Date of principal star: 16 May Corona Borealis, or the Northern Crown, is the crown Ariadne wore at her wedding. It was made by the supreme goldsmith, Hephaestus, at his underwater smithy.
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coronagraphHome ... Science and Technology Astronomy and Space Exploration Astronomy: General ... Essential reading Compare side-by-side A Dictionary of Astronomy The Columbia Encyclopedia, Sixth Edition ...
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Coronary thrombosis is a form of thrombosis affecting the coronary circulation. It is associated with stenosis subsequent to clotting. The condition is considered as a type of ischaemic heart disease....
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Coronal loops have become very important when trying to understand the current coronal heating problem.
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Coronagraphs allow us to see only the outer parts of the corona, because the instrument blocks our view of the inner corona. X-ray images can show us the parts closer to the Sun, because there's no need to block out the solar disk. More info: ...
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Corona. Another important set of unknown lines revealed during an eclipse came from the corona, and so its source element was called coronium.
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Selu CoronaLocated in Terra, Corona measures 350 km (210 mi) in diameter. are circular to elliptical features marked by a ring of concentric ridges, and are thought to result from the flow of heat in the planet's interior.
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Coronal mass ejections are giant magnetic bubbles that expand to nearly the size of the Sun itself as they leave the low corona. The CMEs move outward at speeds from 200 to 1,000 km/s (100 to 600 mi/s).
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Coronal loops, immense coils of hot gas on the surface of the Sun, vibrate wildly after the blast wave from a solar flare hits them. However, their dance is quickly squelched by resistance from the Sun's outer atmosphere ( corona).
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Coronal Holes The best-known early observations of the Sun from space were the ones made in 1973 from the space station Skylab.
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Corona BorealisAbbreviation: CrB Genitive: Coronae Borealis Translation: The Northern Crown Interactive star chart (Java applet) ...
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Corona BorealisMap created in Guide 7.0 with the figure outline based on Johannes Hevelius' Uranographia (1690). Click on the object's name to access its image or click on the name of adjacent constellation to see its map.
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CORONAThe very hot outermost layer of a star's atmosphere. Our Sun's corona can only be seen during a total solar eclipse. COSMONAUT An astronaut from the former Soviet Union or the current republic of Russia.
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CoronaePancake volcanoes Magellan's images show a wide variety of interesting and unique features including pancake volcanoes (left) which seem to be eruptions of very thick lava and coronae (right) which seem to be collapsed domes over large magma ...
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Corona: The atmosphere of the Sun composed of hot, very thin gas, extending out away from the Sun for a substantial distance. This gas emits light but normally that light can't be seen against the direct glare of the Sun.
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CoronaOutermost atmosphere of the Sun immediately above the chromosphere, consisting of hot (1-2 × 106 K), low- density (about 10-16 g cm-3) gas that extends for millions of miles from the Suns's surface.
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The corona is known to be very hot because it has ions with many electrons removed from the atoms. At high enough temperatures the atoms collide with each other with such energy to eject electrons. This process is called ionization.
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The corona is the top layer of the atmosphere; it extends for millions of miles beyond the Sun's surface. The corona has very high temperatures (over a million ;K) and a very low density.
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Solar corona studies conducted by a PI at JPL using DSN's radio link with various interplanetary spacecraft as they pass behind the Sun.
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[10.5] CORONA IN ORBIT / GRAB [10.6] FOUNDATION OF THE NRO / SAMOS & MIDAS [10.7] THE FISHBOWL SPACE NUCLEAR TESTS / THE TEST-BAN TREATY ...
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The solar corona is the outermost part of the Sun's atmosphere. Coronal holes occur where a region is more tenuous than the surrounding corona and are thought to be the primary source of high-speed streams of charged particles from the Sun.
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In 2375, the corona of an O-type star in the Delta Quadrant served to contain the explosion of a Malon export vessel, that otherwise would have destroyed everything within three light years.
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See also: Sun, Solar, Light, Earth, Star
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