| omega |
Omega (the last letter in the Greek alphabet) refers to ratio of the observed density of the Universe (how much mass there is per unit volume) to the critical density of the Universe (the density that would be necessary to stop the expansion of the Universe). If omega is greater than one, then the Universe will eventually stop expanding and begin to contract, and the Universe will end in a "Big Crunch. ...
출처: www.enchantedlearning.com/subjects/astronomy/gloss...
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| omega. |
Omega (the last letter in the Greek alphabet) refers to ratio of the observed density of the Universe (how much mass there is per unit volume) to the critical density of the Universe (the density that would be necessary to stop the expansion of the Universe). If omega is greater than one, then the Universe will eventually stop expanding and begin to contract, and the Universe will end in a "Big Crunch. ...
출처: www.enchantedlearning.com/subjects/astronomy/gloss...
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| omega |
One chip Multimedia EnGine Architecture One of CMG's product family for digital video products
출처: www.st.com/stonline/press/news/glossary/o.htm
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| omega. |
One chip Multimedia EnGine Architecture One of CMG's product family for digital video products
출처: www.st.com/stonline/press/news/glossary/o.htm
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| omega |
A term used to describe vertical motion in the atmosphere. The "omega equation" used in numerical weather models is composed of two terms, the "differential vorticity advection" term and the "thickness advection" term. Put more simply, omega is determined by the amount of spin (or large scale rotation) and warm (or cold) advection present in the atmosphere. On a weather forecast chart, high values of omega (or a strong omega field) relate to upward vertical motion in the atmosphere. ...
출처: www.srh.weather.gov/srh/jetstream/append/glossary_...
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