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Found 11 dataset(s) matching "3-axis".
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CARICOOS Caribbean Buoy VI1. CARICOOS real-time buoy observations near Puerto Rico and the U.S. Virgin Islands at VI1 - CarICOOS Data Buoy C, located at 18d 14.952m N, 64d 45.792m Wl, South of St...
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CARICOOS real-time buoy observations near Puerto Rico and the U.S. Virgin Islands at PR3 - CARICOOS Data Buoy E, located at 18d 15.660m N, 65d 27.846m Wl, North of Vieques. Buoy PR312 was...
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CARICOOS real-time buoy observations near Puerto Rico and the U.S. Virgin Islands at PR1 - CarICOOS Data Buoy A, located at 17d 52.200m N, 66d 32.220m Wl, South of Caja de Muertos Island. Buoy...
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CARICOOS real-time buoy observations near Puerto Rico and the U.S. Virgin Islands at PR2 - CarICOOS Data Buoy B, located at 18d 28.548m N, 66d 5.970m Wl, North side of Puerto Rico near San Juan. ...
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TWINS, Two Wide-angle Imaging Neutral-atom Spectrometers, is a Mission of Opportunity under NASA's Small Explorer, SMEX, Program. TWINS-1 and TWINS-2 are the Designations for NASA-Sponsored...
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TWINS, Two Wide-angle Imaging Neutral-atom Spectrometers, is a Mission of Opportunity under NASA's Small Explorer, SMEX, Program. TWINS-1 and TWINS-2 are the Designations for NASA-Sponsored...
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Repeat Stations are temporary magnetic installations, where the Earth’s magnetic field, or geomagnetic field, is measured for several days, with the goal of producing mean values of the vector...
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A total of 119 passive seismic soundings were collected with Tromino (MoHo s.r.l.) 3-axis seismometers in the Fountain Creek area to partially refine alluvial aquifer thickness (depth to bedrock)...
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TWINS, Two Wide-angle Imaging Neutral-atom Spectrometers, is a Mission of Opportunity under NASA's Small Explorer, SMEX, Program. TWINS-1 and TWINS-2 are the Designations for NASA-Sponsored...
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TWINS, Two Wide-angle Imaging Neutral-atom Spectrometers, is a Mission of Opportunity under NASA's Small Explorer, SMEX, Program. TWINS-1 and TWINS-2 are the Designations for NASA-Sponsored...
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This MESSENGER Magnetic field data set contains cruise-phase magnetic field vectors in RTN coordinates at time resolutions typically of 0.5 s or 1.0 s and sometimes as fine as 0.05 s. The Mercury...
