Browse terms - alphabetical

alphabetical | high score | recent | volatile | stable | filter:
Term Definition Contributor Modified
deformed No definition provided Ryan McGranaghan 2023.04.16
Deformed ice A general term for sea ice that has been broken and reoriented. It includes ridged, hummocked, and rafted ice. Deformed ice is distinguished by its high surface roughness. GCW Glossary 2023.03.27
Deformed ice A general term for ice that has been squeezed together and, in places, forced upwards (and downwards). Subdivisions are rafted ice, ridged ice, and hummocked ice. GCW Glossary 2023.03.27
Deformed ice A general term for ice which has been squeezed together and forced upwards and downwards in places. Subdivisions are rated ice, ridge ice, hummocked ice, and other similar deformations. GCW Glossary 2023.03.27
Deformed ice Sea ice terminology. It is a general term for ice which has been squeezed together, and in places, forced upwards and downwards. The subdivisions of deformed ice are known as rafted ice, ridged ice, a nd hummocked ice. GCW Glossary 2023.03.27
Deformed ice A general term for ice which has been squeezed together and broken up with formation of surface and underwater conglomerations. Subdivisions are rafted ice, rough ice, ridged ice, jammed brash barrier and hillocky multiyear ice. GCW Glossary 2023.03.27
Deformities No definition provided Christopher Rauch 2023.12.01
Deformities, Artificial No definition provided Christopher Rauch 2023.12.01
Deformities, Cure of No definition provided Christopher Rauch 2023.12.01
degas No definition provided Ryan McGranaghan 2023.04.16
Degenerate matter Highly compressed matter in which the normal atomic structure has broken down and which, because of quantum-mechanical effects, exerts a pressure that is independent of temperature. Bodies with masses less than Chandrasekhar's limit (1.4 solar masses) are supported by electron degeneracy pressure and have densities of about 10^6 kg/m^3. In collapsed stars of mass above 1.4 solar masses, gravity will overwhelm electron degeneracy and further collapse ensues. Electrons combine with protons to form neutrons, so producing a neutron star. Because neutrons, like electrons, are fermions and therefore subject to the Pauli exclusion principle, at high enough densities, about 10^14 kg/m^3, neutron degeneracy pressure prevents further collapse of the star. For masses larger than 2-3 solar masses, even neutron degeneracy cannot prevent further collapse, and a black hole is formed. Ryan McGranaghan 2023.04.16
Degeneration No definition provided Christopher Rauch 2023.12.01
Degeneration, Fatty No definition provided Christopher Rauch 2023.12.01
Degeneration (Pathology) No definition provided Christopher Rauch 2023.12.01
Deglaciation The removal of land ice from an area; the opposite of glacierization. GCW Glossary 2023.03.27
Deglaciation/glacial termination Transitions from full glacial conditions (ice age) to warm interglacials characterized by global warming and sea level rise due to change in continental ice volume. GCW Glossary 2023.03.27
Deglutition No definition provided Christopher Rauch 2023.12.01
degree No definition provided Ryan McGranaghan 2023.04.16
degree c No definition provided Ryan McGranaghan 2023.04.16
Degree-day A unit of measurement to express the departure of the mean temperature for a day from a given References (or base) temperature. The Freezing Index and the Thawing Index are expressed in degree-days wi th respect to a References temperature of 0C (32F); units: degree-day Celsius or degree-day Fahrenheit. GCW Glossary 2023.03.27
1 2 ... 560 561 562 563 564 565 566 ... 2677 2678