@prefix qx8: <http://data.loterre.fr/ark:/67375/QX8> .
@prefix skos: <http://www.w3.org/2004/02/skos/core#> .

qx8: a skos:ConceptScheme .
qx8:-RNZQ9DK5-N
  skos:exactMatch <http://data.loterre.fr/ark:/67375/26L-B976QT79-4>, <https://en.wikipedia.org/wiki/Scoria>, <https://fr.wikipedia.org/wiki/Scorie> ;
  skos:prefLabel "scorie"@fr, "scoria"@en ;
  skos:definition "Le terme scories désigne également des éjectas (des fragments de roches magmatiques éjectés par une éruption volcanique) légers et poreux, comme la pouzzolane. Leur densité est supérieure à celle de l'eau, ce qui les différencie des ponces. Les cônes de scories sont des édifices volcaniques essentiellement constitués de scories et de cendres (les cendres volcaniques se distinguent des scories par leur plus grand état de division). (Adapté de : <a href=\"https://fr.wikipedia.org/wiki/Scorie\">https://fr.wikipedia.org/wiki/Scorie</a>)"@fr, "Scoria is a pyroclastic, highly vesicular, dark-colored volcanic rock formed by ejection from a volcano as a molten blob and cooled in the air to form discrete grains called clasts. It is typically dark in color (brown, black or purplish-red), and basaltic or andesitic in composition. Scoria has relatively low density, as it is riddled with macroscopic ellipsoidal vesicles (gas bubbles), but in contrast to pumice, scoria always has a specific gravity greater than 1 and sinks in water. Scoria may form as part of a lava flow, typically near its surface, or as fragmental ejecta (lapilli, blocks, and bombs), for instance in Strombolian eruptions that form steep-sided scoria cones, also called cinder cones. Scoria's holes or vesicles form when gases dissolved in the original magma come out of solution as it erupts, creating bubbles in the molten rock, some of which are frozen in place as the rock cools and solidifies. Most scoria is composed of glassy fragments and may contain phenocrysts. Scoria differs from pumice, another vesicular volcanic rock, in having larger vesicles and thicker vesicle walls, and hence is denser. The difference is probably the result of lower magma viscosity, allowing rapid volatile diffusion, bubble growth, coalescence, and bursting. As rising magma encounters lower pressures, dissolved gases are able to exsolve and form vesicles. Some of the vesicles are trapped when the magma chills and solidifies. Vesicles are usually small, spheroidal and do not impinge upon one another; instead, they open into one another with little distortion. Volcanic cones of scoria can be left behind after eruptions, usually forming mountains with a crater at the summit. (Adapted from: <a href=\"https://en.wikipedia.org/wiki/Scoria\">https://en.wikipedia.org/wiki/Scoria</a>)"@en ;
  a skos:Concept ;
  skos:broader qx8:-HG875W53-R ;
  skos:inScheme qx8: .

qx8:-HG875W53-R
  skos:prefLabel "study material"@en, "matériau d'étude"@fr ;
  a skos:Concept ;
  skos:narrower qx8:-RNZQ9DK5-N .