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Density


GCMD >> EARTH SCIENCE >> Oceans >> Salinity/Density >> Density
Movie ID Title
This animation first depicts thermohaline surface flows over surface density, and illustrates the sinking of water in the dense ocean near Iceland and Greenland. The surface of the ocean then fades away and the animation pulls back to show the global thermohaline circulation. 3658 The Thermohaline Circulation - The Great Ocean Conveyor Belt
An animation of average Sea Surface Temperature on a globe. 3652 Sea Surface Temperature, Salinity and Density

SVS >> Density
Movie ID Title
This animation first depicts thermohaline surface flows over surface density, and illustrates the sinking of water in the dense ocean near Iceland and Greenland. The surface of the ocean then fades away and the animation pulls back to show the global thermohaline circulation. 3658 The Thermohaline Circulation - The Great Ocean Conveyor Belt
An animation of average Sea Surface Temperature on a globe. 3652 Sea Surface Temperature, Salinity and Density
Evolution of the electron fraction during the first 20 milliseconds in the life of a neutron star formed from a Type II supernova 1383 Instabilities in Very Young Neutron Stars: Electron Fraction
Evolution of the temperature during the first 20 milliseconds in the life of a neutron star formed from a Type II supernova 1382 Instabilities in Very Young Neutron Stars: Temperature
Evolution of the density during the first 20 milliseconds in the life of a neutron star formed from a Type II supernova 1381 Instabilities in Very Young Neutron Stars: Density
Evolution of the electron fraction during the first 20 milliseconds in the life of a neutron star formed from a Type II supernova 48 Instabilities in Very Young Neutron Stars: Electron Fraction
Evolution of the temperature during the first 20 milliseconds in the life of a neutron star formed from a Type II supernova 47 Instabilities in Very Young Neutron Stars: Temperature
Evolution of the density during the first 20 milliseconds in the life of a neutron star formed from a Type II supernova 46 Instabilities in Very Young Neutron Stars: Density

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