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Found 4 result(s)

Data Buoy Cooperation Panel

DBCP

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The DBCP is an international program coordinating the use of autonomous data buoys to observe atmospheric and oceanographic conditions, over ocean areas where few other measurements are taken.

RAVE database

Radial Velocity Experiment Database

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RAVE (RAdial Velocity Experiment) is a multi-fiber spectroscopic astronomical survey of stars in the Milky Way using the 1.2-m UK Schmidt Telescope of the Anglo-Australian Observatory (AAO). The RAVE collaboration consists of researchers from over 20 institutions around the world and is coordinated by the Leibniz-Institut für Astrophysik Potsdam. As a southern hemisphere survey covering 20,000 square degrees of the sky, RAVE's primary aim is to derive the radial velocity of stars from the observed spectra. Additional information is also derived such as effective temperature, surface gravity, metallicity, photometric parallax and elemental abundance data for the stars. The survey represents a giant leap forward in our understanding of our own Milky Way galaxy; with RAVE's vast stellar kinematic database the structure, formation and evolution of our Galaxy can be studied.

Upper Ocean Processes Group

UOP

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The primary focus of the Upper Ocean Processes Group is the study of physical processes in the upper ocean and at the air-sea interface using moored surface buoys equipped with meteorological and oceanographic sensors. UOP Project Map The Upper Ocean Processes Group provides technical support to upper ocean and air-sea interface science programs. Deep-ocean and shallow-water moored surface buoy arrays are designed, fabricated, instrumented, tested, and deployed at sea for periods of up to one year

MARGINS Data Portal

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<<<!!!<<< Margin is now Geoprism see: https://www.re3data.org/repository/r3d100010639 >>>!!!>>>