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Telescope observations, star catalogs, exoplanet surveys, galaxy morphology, gravitational waves, spectroscopy
2,977 datasets
Annual surveys from 2001 to 2010 sampled bottom sediments at six stations near the Waianae Ocean Outfall in Oahu, Hawaii. Data includes species abundance and richness for multiple faunal groups and geochemical measurements like oxidation-reduction-potential. The dataset was compiled by NOAA's National Centers for Environmental Information.
Macquarie Island peat bog cores provide a high-temporal resolution record of cosmic dust influx variability during the Holocene. The dataset, created by the Australian Antarctic Data Centre (AU_AADC), contains carbon dating measurements from geochemical peat cores. It was last updated in April 2010.
Research data investigates larval dispersal as a mechanism for gene flow between Antarctic and South American benthic invertebrate populations. The dataset likely contains plankton samples, hydrographic data, and molecular phylogenetic comparisons from transects across the Drake Passage. The work was conducted by AMD_USAPDC and last updated in January 2010.
A twelve-channel, six-frequency passive-microwave radiometer system measures vertically and horizontally polarized brightness temperatures at frequencies from 6.925 GHz to 89.0 GHz. Spatial resolution of individual measurements varies from 5.4 km to 56 km. The data was collected by the AMSR-E instrument on the EOS platform and processed by AMD_KOPRI, with the latest records from 2009.
Data from the BOUM project details biological production, remineralization, and export processes across distinct oligotrophic systems in the Mediterranean Sea. The project was conducted by federated French teams and involved a research cruise. The dataset's final update was recorded at the end of 2009.
Monthly anomalies in total cloud amount have been empirically corrected to remove spurious variability from satellite orbital changes and instrument calibration. Data covers a 2.5 by 2.5 degree global grid from 1983 to 2009, excluding polar regions beyond 60 degrees latitude. The correction procedure was developed by SCIOPS and applied to the International Satellite Cloud Climatology Project (ISCCP) and Pathfinder Atmospheres - Extended (PATMOS-x) datasets.
Antarctic observations from the CSTAR telescope array at Kunlun Station, Dome A provide photometric data for 21,845 stars around the South Celestial Pole. The dataset includes light curves and a catalog, produced by a collaboration including Purple Mountain Observatory and the National Astronomical Observatories of China. The original CSTAR instrument operated from 2008 to 2011.
Twelve-channel passive-microwave radiometer data measures vertically and horizontally polarized brightness temperatures at six frequencies from 6.925 to 89.0 GHz. Spatial resolution varies from 5.4 km at 89.0 GHz to 56 km at 6.9 GHz. The instrument, operated by AMD_KOPRI, collected data throughout the 2008 calendar year.
SCIOPS research investigates planktonic larval dispersal as a mechanism for gene flow between Antarctic and South American benthic invertebrate populations. The project involves plankton sampling and hydrographic data collection across Drake Passage, combined with molecular phylogenetic analysis of adult forms. Data collection was conducted under a NASA EarthData project last updated in January 2008.
NASA's AMSR-E instrument collected global passive microwave radiometer data throughout 2007. The system recorded vertically and horizontally polarized brightness temperatures at six frequencies ranging from 6.925 GHz to 89.0 GHz. Data was produced by the AMD_KOPRI organization from the NASA Earthdata platform.
Advanced Microwave Scanning Radiometer form EOS (AMSR-E) data provides vertically and horizontally polarized brightness temperature measurements at six frequencies: 6.925, 10.65, 18.7, 23.8, 36.5, and 89.0 GHz. The dataset was produced by AMD_KOPRI and contains observations from the year 2006. Spatial resolution of individual measurements varies from 5.4 km at 89.0 GHz to 56 km at 6.9 GHz.
Biopearl expedition data details sea star specimens collected across the Scotia Arc in 2006. The survey covered 29 stations at four standardized depths using an Epibenthic Sledge. Specimen taxonomy was standardized using the Register of Antarctic Marine Species.
NOAA/WDS Paleoclimatology archives a cosmic ray intensity reconstruction dataset by Usoskin et al. (2002, 2005, 2006). It provides climate forcing parameters for a global geographic location. The temporal coverage spans from 339 to -57 calendar years before present.
Final GPS satellite orbits processed homogeneously using Bernese GPS Software. The data was reprocessed by TU Munich and TU Dresden for the SCIOPS organization. The dataset was last updated in April 2006.
Transmission Electron Microscopy images and spectroscopy data of insoluble particles extracted from an ice core drilled at Law Dome, East Antarctica. The data is organized into three folders corresponding to mean ice ages of 1795, 1838, and 1930 Common Era. The depth/age scale was constructed by matching dissolved ion chemistry and water stable isotope records to the main DSS ice core record.
Global passive microwave radiometer data from the AMSR-E instrument, measuring vertically and horizontally polarized brightness temperatures at six frequencies from 6.925 to 89.0 GHz. The instrument was developed by AMD_KOPRI and data collection occurred throughout 2005. Measurements have spatial resolutions ranging from 5.4 km to 56 km depending on the frequency channel.
ANDEEP3 expedition data contains morphological information on sea stars collected from the deep sea. Specimens were gathered in 2005 from 16 stations in the Powell Basin and Weddell Sea using an Agassiz trawl at depths between 1047 and 4931 meters. The dataset was created by researchers from SCIOPS, who performed detailed taxonomic identification using morphological characters and historical literature.
2004 data from the Advanced Microwave Scanning Radiometer for EOS (AMSR-E), a twelve-channel, six-frequency passive-microwave radiometer system. The instrument measures vertically and horizontally polarized brightness temperatures at frequencies from 6.925 GHz to 89.0 GHz, with spatial resolution varying from 5.4 km to 56 km. It was produced by the organization AMD_KOPRI and collected via a 1.6-meter diameter scanning reflector.
Biological weighting functions quantify the wavelength-dependent effects of ultraviolet radiation on DNA damage in larvae of several Antarctic marine invertebrates. Data was generated by exposing embryos and larvae to artificial light with specific wavelength filters over three days and analyzing for cyclobutane pyrimidine dimers. The dataset was produced by the organization SCIOPS and last updated in December 2004.
Time-stamped data from 2004 and earlier, collected by the Australian Antarctic Data Centre from riometer and magnetometer stations in the Australian Antarctic Territory and Macquarie Island. The dataset captures 30 MHz cosmic noise intensity and three-component geomagnetic field measurements. Data acquisition was synchronized via GPS for precise millisecond-level timing.