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Climate models, weather data, oceanography, hydrology, atmospheric science, environmental monitoring
28,646 datasets
CERES BDS Terra FM2 Edition1-CV provides 24 hours of Level-1B data from the CERES-FM2 instrument on the Terra satellite, collected for instrument validation. The National Aeronautics and Space Administration (NASA) produces this data, which includes raw and geolocated science data from normal and short Earth scans in various modes. Data collection for this product is ongoing.
Central Alaska Network of National Parks permafrost monitoring data, updated annually. The dataset includes subdirectories for locations, field notes, active layer surveys, borehole temperatures, rock glacier surveys, and soil temperature logs. Data is maintained by the Department of the Interior, with the most recent authoritative records uploaded as a zip file.
June 1-28, 1992 data from the Atlantic Stratocumulus Transition Experiment (ASTEX) region. The European Centre for Medium-range Weather Forecasts (ECMWF) produced mean vertical velocity analyses using its T213L30 operational model, incorporating about 650 special soundings from the experiment. The data were reformatted into ASCII files by Chris Bretherton of the University of Washington.
The Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) captures images of the Sun at a 12-second cadence in the 94 Ångstrom channel, observing 6.3 million Kelvin flaring plasma. This dataset, provided by the National Aeronautics and Space Administration (NASA), offers full-disk solar imagery with 4k x 4k resolution and a pixel size of 0.6 arcseconds. It supports the Living With a Star program's objectives for space weather monitoring and solar physics research.
Solar Dynamics Observatory Atmospheric Imaging Assembly (SDO/AIA) Level 1 FITS data. The AIA instrument captures high-resolution images of the Sun's atmosphere across multiple ultraviolet and extreme ultraviolet wavelengths. The data is provided by the National Aeronautics and Space Administration (NASA) and was last updated in March 2026.
Essentially uninterrupted viewing at a 12-second cadence for the 193 Å channel, capturing the Sun's corona and hot flare plasma. The Atmospheric Imaging Assembly (AIA) onboard NASA's Solar Dynamics Observatory provides full-disk solar images in 4k x 4k resolution with a pixel size of 0.6 arcseconds. This data focuses on the evolution of the Sun's magnetic environment and its interaction with plasma, supporting space weather research.
SDO/AIA 335 Å Level 1 FITS Data captures images of the Sun's corona in the 335 Angstrom wavelength, observing the Fe xvi line from active regions at approximately 2.5 million Kelvin. The Atmospheric Imaging Assembly (AIA) onboard NASA's Solar Dynamics Observatory provides full-disk 4k x 4k resolution images with a pixel size of 0.6 arcseconds. Data collection occurs at a temporal cadence of 12 seconds for EUV channels, offering essentially uninterrupted viewing for months.
Pakistan's air quality data, likely containing measurements of pollutants like particulate matter or gases. The dataset is hosted on Kaggle, but its specific source, temporal coverage, and collection method are not detailed in the provided metadata. Further verification is required to confirm the exact parameters and time span of the measurements.
Encompassing a three-dimensional seismic slowness model and associated MATLAB and Python processing code derived from P-wave data at Newberry Volcano in central Oregon. The model targets the shallow crust to approximately 10 km depth, combining active-source and teleseismic data from the 2008 Newberry Seismic Experiment. It was produced as part of the DEEPEN geothermal project.
CAMEX-4 Shared Mobile Atmospheric Research and Teaching Radars data was collected by a truck-mounted 5 cm Doppler radar during the Fourth Convection and Moisture Experiment. The radar was deployed in the Florida Keys and later moved to Venice, Florida, to capture landfall of Tropical Storm Gabrielle on September 14, 2001. The dataset is managed by the Global Hydrology Resource Center Distributed Active Archive Center (GHRC_DAAC).
Three distinct protection zones—water catchment areas, a 25-year zone, and a drilling-free zone—are defined around the Aalsterweg/Klotputten and Welschap drinking water abstractions in Eindhoven. This data, published via the GIS service of the Province of North Brabant, is governed by the Provincial Environmental Ordinance (PMV) to protect against contaminants. The dataset originates from the Ministerie van Binnenlandse Zaken en Koninkrijksrelaties and is available in multiple formats including ESRI SHAPE.
Soil moisture data for the year 2020, likely derived from the TIGGE (THORPEX Interactive Grand Global Ensemble) initiative. The dataset appears to be a processed or 'stitched' product, suggesting it combines multiple sources or models. It is hosted on the Kaggle platform, but detailed metadata about its specific creation and variables is unavailable.
2-meter resolution bathymetry and seafloor habitat classification maps for the shallow waters (0-25 meters) of Christmas Island Marine Park. The data was processed using EOMAP's proprietary Watcor-X software and physics-based inversion methods on multi-spectral satellite imagery. These geospatial layers provide an environmental baseline for monitoring and managing the Indian Ocean Territories Marine Parks.
Geoscience Australia's 2015 marine survey (GA-0352) acquired high-resolution bathymetry data to assess CO2 storage potential in the Gippsland Basin. The survey, conducted from April 5th to 24th, 2015, by the vessel MV Duke, collected industry-standard Multi-beam echo-sounder (MBES) and sub-bottom profiling (SBP) data. This precompetitive data supports sequence stratigraphic studies and identification of potential CO2 storage reservoirs.
The Atmospheric Imaging Assembly (AIA) onboard NASA's Solar Dynamics Observatory (SDO) captures images of the Sun's corona and upper transition region at 0.63 MK in the 171 Å channel. It provides full-disk solar imagery at 4k x 4k resolution with a pixel size of 0.6 arcseconds, at a cadence of 12 seconds for EUV channels. The data is produced by the National Aeronautics and Space Administration.
SDO/AIA 131 Å Level 1 FITS Data captures images of the Sun's atmosphere in the 131 Ångstrom channel, observing 10 MK and 16 MK flaring plasma. The Atmospheric Imaging Assembly (AIA) onboard NASA's Solar Dynamics Observatory provides full-disk solar images at 4k x 4k resolution with a pixel size of 0.6 arcseconds. AIA operates at cadences of 12 seconds for EUV channels and 24 seconds for UV channels, offering essentially uninterrupted viewing for months.
The Atmospheric Imaging Assembly (AIA) onboard NASA's Solar Dynamics Observatory captures images of the Sun's chromosphere and transition region at 304 Å wavelength. It provides a 4k x 4k resolution view of the entire Sun with a temporal cadence of 12 seconds in seven EUV band passes. The data is stored in FITS format and supports the Living With a Star program's research on space weather.
The Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) captures images of the Sun's atmosphere at a resolution of 4k x 4k pixels. It provides essentially uninterrupted viewing for months at a temporal cadence of 12 seconds in seven extreme UV band passes, including the 211 Å channel which observes the Fe XIV line from active region corona. This Level 1 FITS data is produced by NASA.
SDO/AIA 1600 Å Level 1 FITS Data captures ultraviolet solar imagery focusing on the transition region and upper photosphere. The Atmospheric Imaging Assembly onboard NASA's Solar Dynamics Observatory provides 4k x 4k resolution images with a temporal cadence of 24 seconds for this UV channel. This dataset supports the Living With a Star program for monitoring space weather and coronal disturbances.
The Atmospheric Imaging Assembly (AIA) onboard NASA's Solar Dynamics Observatory captures images of the Sun's atmosphere. AIA provides full-disk solar images in 4k x 4k resolution with a pixel size of 0.6 arcseconds, covering multiple ultraviolet and extreme ultraviolet wavelengths. The instrument operates at cadences ranging from 12 to 24 seconds, offering essentially uninterrupted viewing for months.