 |
at Global Oneness Community.
Share your dreams and let others help you with the interpretation!
Dream Sharing Forum
|
 |
grain size | A Wisdom Archive on grain size |  | grain size A selection of articles related to grain size |  |
| We recommend this article: grain size - 1, and also this: grain size - 2. |
 | |
grain size
|  | | Page 1 » Page 2 « Page 3 More » |  |
 | |
| ARTICLES RELATED TO grain size | | | |  |  |  | grain size: Encyclopedia II - Sedimentary rock - Classification
Sedimentary rock - Clastic sedimentary rocks.
Clastic sedimentary rocks are composed of discrete fragments or clasts of materials derived from other rocks. They are composed largely of quartz with other common minerals including feldspars, amphiboles, clay minerals, and sometimes more exotic igneous and metamorphic minerals.
Clastic sedimentary rocks may be regarded as falling along a scale of grain size, with shale being the finest with particles less than 0.004 mm, siltstone being intermediate with parti ...
See also:Sedimentary rock, Sedimentary rock - Formation, Sedimentary rock - Classification, Sedimentary rock - Clastic sedimentary rocks, Sedimentary rock - Biogenic sedimentary rocks, Sedimentary rock - Precipitate sedimentary rocks, Sedimentary rock - Other information Read more here: » Sedimentary rock: Encyclopedia II - Sedimentary rock - Classification |
|  |
| |  |  |  | grain size: Encyclopedia II - Casting - Cooling rateThe rate at which a casting cools affects its microstructure, quality, and properties.
The products of sand casting and slurry-mold processes, often large with thick walls, generally cool slowly. This increases the metal's grain size, creating a coarse microstructure that lowers the strength of the casting. Coarse grains can allow elements of an alloy to separate, which also weakens the casting. But slower cooling keeps the casting metal liquid longer, which allows more gases and waste metal to escape, reducing the voids a ...
See also:Casting, Casting - Lost wax casting process, Casting - Other casting processes used in creating artworks, Casting - Casting in manufacturing, Casting - Expendable mold casting, Casting - Nonexpendable mold casting, Casting - Cooling rate, Casting - Shrinkage Read more here: » Casting: Encyclopedia II - Casting - Cooling rate |
|  |
|  |  |  | grain size: Encyclopedia II - Cosmic dust - Dust grain destructionHow are the interstellar grains destroyed? There are some ultraviolet processes which lead to grain "explosions" (d'Hendecourt et al., 1985; Greenberg, 1976). Evans (1994) also describes evaporation, sputtering (when an atom or ion strikes the surface of a solid with enough momentum to eject atoms from it), and grain-grain collisions, which have a major influence on the grain size distribution, as well.
These destructive processes happen in a variety of places. Some grains are destroyed in the supernovae/novae explosion (and then some ...
See also:Cosmic dust, Cosmic dust - Introductory Material, Cosmic dust - Some bulk properties of cosmic dust, Cosmic dust - Radiative properties of cosmic dust, Cosmic dust - Dust grain formation, Cosmic dust - Dust grain destruction, Cosmic dust - Some dusty clouds in the universe Read more here: » Cosmic dust: Encyclopedia II - Cosmic dust - Dust grain destruction |
|  |
|  |  |  | grain size: Encyclopedia II - Cosmic dust - Some bulk properties of cosmic dustCosmic dust is dust grains and agreggates of dust grains. These particles are irregularly-shaped with porosity ranging from fluffy to compact. The composition, size, and other properties depends on where the dust is found. General diffuse interstellar medium dust should be distinguished from dust grains in dense clouds, which should be distinguished from planetary rings dust, which should be distinguished from circumstellar dust, and so on. For example, grains in dense clouds have acquired a mantle of ice and the average dimens ...
See also:Cosmic dust, Cosmic dust - Introductory Material, Cosmic dust - Some bulk properties of cosmic dust, Cosmic dust - Radiative properties of cosmic dust, Cosmic dust - Dust grain formation, Cosmic dust - Dust grain destruction, Cosmic dust - Some dusty clouds in the universe Read more here: » Cosmic dust: Encyclopedia II - Cosmic dust - Some bulk properties of cosmic dust |
|  |
| | |  |  |  | grain size: Encyclopedia II - Cosmic dust - Radiative properties of cosmic dustA dust particle interacts with electromagnetic radiation in a way that depends on its cross section, the wavelength of the electromagnetic radiation, and on the nature of the grain: its refractive index, size, etc. The radiation process for an individual grain is called its emissivity, dependent on the grain's efficiency factor. Furthermore, we have to specify whether the emissivity process is extinction, scattering, or absorption. In the radiation emission curves, several important signatures id ...
See also:Cosmic dust, Cosmic dust - Introductory Material, Cosmic dust - Some bulk properties of cosmic dust, Cosmic dust - Radiative properties of cosmic dust, Cosmic dust - Dust grain formation, Cosmic dust - Dust grain destruction, Cosmic dust - Some dusty clouds in the universe Read more here: » Cosmic dust: Encyclopedia II - Cosmic dust - Radiative properties of cosmic dust |
|  |
| |  |  |  | grain size: Encyclopedia II - Zircon - PropertiesZircon is a remarkable mineral, if only for its almost ubiquitous presence in the crust of Earth. It is found in igneous rocks (as primary crystallization products), in metamorphic rocks (as recrystallized grains) and in sedimentary rocks (as detrital grains). Large zircon crystals are seldom abundant. Their average size, e.g. in granite rocks, is about 100-300 µm, but they can also grow to sizes of several centimeters, especially in pegmatites.
Owing to their uranium and thorium content, some zircons may undergo metamictization. This partially disrupts the crystal structure and explains the ...
See also:Zircon, Zircon - Properties, Zircon - Uses, Zircon - Zircons and the age of Earth Read more here: » Zircon: Encyclopedia II - Zircon - Properties |
|  |
| |  |  |  | grain size: Encyclopedia II - Cosmic dust - Introductory MaterialCosmic Dust refers to particles in space which are assemblages of a few molecules to tenth-millimeter-sized grains. Cosmic dust can be further distinguished by its astronomical location; for example: interplanetary dust, interstellar dust, comet dust, circumplanetary dust. This article covers bulk and radiative properties of cosmic dust, the dust particles' origins, end-fates, and specific locations in space.
Historically, cosmic dust used to be an annoyance to astronomers because of the way that the dust obscures the object th ...
See also:Cosmic dust, Cosmic dust - Introductory Material, Cosmic dust - Some bulk properties of cosmic dust, Cosmic dust - Radiative properties of cosmic dust, Cosmic dust - Dust grain formation, Cosmic dust - Dust grain destruction, Cosmic dust - Some dusty clouds in the universe Read more here: » Cosmic dust: Encyclopedia II - Cosmic dust - Introductory Material |
|  |
| | | | | |  |  |  | grain size: Encyclopedia II - Facies - Facies types
Facies - Sedimentary facies.
Generally, facies are distinguished by what aspect of the rock or sediment is being studied. Thus, facies based on petrological characters such as grain size and mineralogy are called lithofacies, whereas facies based on fossil content are called biofacies.
These facies types are usually further subdivided, for example, you might refer to a "tan, cross-bedded oolitic limestone facies" or a "blueschist facies". The characteristics of the rock unit come from the deposition ...
See also:Facies, Facies - Definition, Facies - Facies types, Facies - Sedimentary facies, Facies - Metamorphic facies, Facies - Walther's Law of Facies Read more here: » Facies: Encyclopedia II - Facies - Facies types |
|  |
|  | | Page 1 » Page 2 « Page 3 More » |  |
 | |
|
|
Search the Global Oneness web site |
|
|
|