The GHO data repository is WHO's gateway to health-related statistics for its 194 Member States. It provides access to over 1000 indicators on priority health topics including mortality and burden of diseases, the Millennium Development Goals (child nutrition, child health, maternal and reproductive health, immunization, HIV/AIDS, tuberculosis, malaria, neglected diseases, water and sanitation), non communicable diseases and risk factors, epidemic-prone diseases, health systems, environmental health, violence and injuries, equity among others.

This collection includes only a subset of indicators from the source dataset.

We report on low-spectral resolution observations of comet 9P/Tempel 1 from 1983, 1989, 1994 and 2005 using the 2.7m Harlan J. Smith telescope of McDonald Observatory. This comet was the target of NASA's Deep Impact mission and our observations allowed us to characterize the comet prior to the impact. In the published paper, we showed that the comet decreased in gas production from 1983 to 2005, with the decrease being different factors for different species. OH decreased by a factor 2.7, NH by 1.7, CN by 1.6, C3 by 1.8, CH by 1.4 and C2 by 1.3. Despite the decrease in overall gas production and these slightly different decrease factors, we found that the ratios of the gas production rates of OH, NH, C3, CH and C2 that of CN were constant over all of the apparitions. We saw no change in the production rate ratios after the impact. We found that the peak gas production occurred about two months prior to perihelion. This data set represents the integrated fluxes and column densities, mentioned in the published paper, which were used to derive the production rates in the paper.

This dataset refers to territorial actors who, in France, produce and publish open public data (at least 1 dataset published on a website, a dedicated platform or a shared platform, including on data.gouv.fr). It contains the 7 GeoJSON layers, one by type of actor, which make it possible to manufacture the map of the open data observatory of territories. These layers are automatically regenerated every day from manually collected data. They are stored and accessible from OpenDataFrance’s GitLab repository.

Users can find data on a range of global health topics like mortality, the burden of disease, infectious diseases, risk factors and health expenditures. Background The Global Health Observatory (GHO) database is the World Health Organization's main health statistics repository. Data is available for 193 World Health Organization member states on topics including but not limited to: Health related millennium goals, mortality, immunization, nutrition, infectious disease, non- communicable disease, tobacco control, violence, injuries, alcohol, HIV/AIDS, tuberculosis, malaria, water and sanitation, maternal and reproductive health, cho lera, child health, child nutrition, and road safety. User FunctionalityUsers can generate tables and charts according to country or region, health indicator, and time period. Data can also be compared across countries. Data can be filtered, tabulated, charted, and downloaded into Excel statistical software. These data are also published in statistical reports covering topics including: Alcohol and health, Child health, Cholera, HIV/AIDS, Malaria, Maternal and reproductive heal th, Non-communicable diseases, Public health and environment, Road safety, Tuberculosis, Tobacco control. Data Notes Data are derived from surveillance and household surveys. Years in which data were collected is indicated with these health statistics. Information is available for each WHO member country and international region. The most recent data is available from 2009.

This bundle collects data taken at McDonald Observatory.

A searchable database of all Solar Dynamics Observatory data including EUV, magnetograms, visible light and X-ray. SDO: The Solar Dynamics Observatory is the first mission to be launched for NASA's Living With a Star (LWS) Program, a program designed to understand the causes of solar variability and its impacts on Earth. SDO is designed to help us understand the Sun's influence on Earth and Near-Earth space by studying the solar atmosphere on small scales of space and time and in many wavelengths simultaneously. SDO's goal is to understand, driving towards a predictive capability, the solar variations that influence life on Earth and humanity's technological systems by determining how the Sun's magnetic field is generated and structured and how this stored magnetic energy is converted and released into the heliosphere and geospace in the form of solar wind, energetic particles, and variations in the solar irradiance.

The Observatory monitors various health R&D related data and incorporates these in comprehensive analyses, with interactive visualizations to help users track and investigate the development in health R&D across many dimensions.

This archive contains raw observations of the 2009-10-09 impact of the LCROSS spacecraft on the moon by the CCD47 camera on the MMT Observatory 6.5m telescope. The archive consists of uncalibrated FITS images of the event. This is one of several data sets of Earth-based observations of the impact.

The database presented here is comprised entirely of observations made utilizing conventional photoelectric photometers and narrowband filters isolating 5 emission species (OH, NH, CN, C3 and C2) and continua. This work was initiated by A'Hearn and Millis in 1976 and includes 2020 observations of 85 comets obtained over 429 nights through the end of 1992. The total number of observations, however, is not evenly distributed over the 85 comets. The median number of observations for a comet is 6, with only a single observation obtained for 14 comets while there were 820 observations of P/Halley. The majority of observations were obtained at either Lowell Observatory or Perth Observatory, however four other observatories were used including an extensive campaign on comet P/Halley from the Cerro Tololo Interamerican Observatory (CTIO). In this archive, results for a subset of 68 comets are presented while the results for P/Halley from this study are archived in the IHW archive.

Daily counts of the Hanko Bird Observatory include following data types since year 1979: (i) counts of local staging birds, (ii) counts of visual diurnal migration, (iii) standardized visual migration counts, (iv) additional observations outside the core observation area, and (v) counts of night migration.

The SmartBay Observatory in Galway Bay is an underwater observatory which uses cameras, probes and sensors to permit continuous and remote live underwater monitoring. It was installed in 2015 on the seafloor 1.5km off the coast of Spiddal, Co. Galway, Ireland at a depth of 20-25m. Underwater observatories allow ocean researchers unique real-time access to monitor ongoing changes in the marine environment. The Galway Bay Observatory is an important contribution by Ireland to the growing global network of real-time data capture systems deployed in the ocean. Data relating to the marine environment at the Galway Observatory site is transferred in real-time through a fibre optic telecommunications cable to the Marine Institute headquarters and then made publically available on the internet. The data includes a live video stream, the depth of the observatory node, the water temperature and salinity, and estimates of the chlorophyll and turbidity levels in the water which give an indication of the volume of phytoplankton and other particles, such as sediment, in the water. Maintenance take place on the observatory every 18 to 24 months. This CTD (Conductivity, Temperature, Depth) and Oxygen Dataset comprises of the raw data that is collected from the Galway Observatory site using an Idronaut Ocean-Seven 304 plus Conductivity-Temperature-Depth (CTD) sensor probe. The sensor measures the temperature and conductivity of the seawater. The conductivity is used to calculate an estimate of the salinity. The pressure exerted by the seawater above is used to calculate the depth of the sensor, and these parameters are also used to estimate the speed of sound within the sea. The Ocean-Seven 304 Plus CTD has also been equipped with a polarographic IDRONAUT dissolved oxygen sensor which measure the dissolved oxygen concentration of the seawater. From the 26th August 2021 a new SeaBird CTD 16CT plus and dissolved Oxygen sensor was deployed and will replace the Idronaut The sensor is deployed on the EMSO Smartbay Cable End Equipment Node in Galway Bay in approx. 25m depth of water. The raw data are stored in txt (ASCII) files generated once a minute with a reading every second. Text files contain ASCII variables separated by tabs. These files may be read by virtually any text editor or spreadsheet program. When interpreted as tabular/spreadsheet data, tabs are equivalent to column divisions, and newline characters are row divisions. For additional information please refer to http://spiddal.marine.ie/data.html None

This worldwide list & map of Astronomical Observatory Sites is issued from this page http://www.eso.org/~ndelmott/obs_sites.html, on the ESO (European Southern Observatory) website.Some of the coordinates are reproduced from The Astronomical Almanac Online and produced by the U.S. Naval Observatory and H.M. Nautical Almanac Office.

Dominion Astrophysical Observatory (DAO) Science Archive data held in the Canadian Astronomy Data Centre (CADC).

The Martha's Vineyard Coastal Observatory (MVCO) is operated by Woods Hole Oceanographic Institution. These datasets include measurements collected from and around the Martha's Vineyard site.

Geomagnetic observatory vector (X, Y, Z) and scalar (F) definitive data (quasi-definitive data are available until the definitive data are ready) recorded by the Ebre Observatory institute. Units: nanoteslas (nT). Recording location: Horta de Sant Joan. Instrumentation: Variometers: LEMI-025 suspended 3-axis fluxgate magnetometer sampled at 1 s rate (filtered). Scalar magnetometers: GEM Systems GSM-90 sampled at 10 s rate. Absolute instrument: D/I-fluxgate magnetometer type TDJ6E-NM/FLM-4. Data are available in different interval types: 1-sec data; 1-min, 1-hour, 1-day and 1-month means.

WHO’s GHO (Global Health Observatory) dataset is published in accordance to the WHO report ”Global burden of disease: 2004 update”. The aim of GHO is to provide access to data and analyses for monitoring the global health situation. Specifically, it contains statistical information regarding the mortality and burden of disease classified according to the death and DALY (disability-adjusted life year) estimates grouped by countries and regions. The dataset has been converted to RDF using the RDF Data Cube Vocabulary.

This data set, acquired with an oceanographic bottom-anchored mooring, includes sea-ice draft and depth data, conductivity, temperature, pressure, salinity, and ocean current measurements such as speed and direction. Each mooring contains vertically distributed instruments, which measure ocean properties at fixed depths and record data internally. These data are retrieved annually when the mooring is recovered. Located on the Pole Abyssal Plain about 50 kilometers from the North Pole, the original 2001 mooring was chosen because it provided a suitable landing site for the supporting aircraft. Ocean depth was approximately 4300 m. Data were recorded half-hourly to hourly. The North Pole Environmental Observatory (NPEO) is a year-round, automated scientific observatory, deploying various instruments each April in order to learn how the world's northernmost sea helps regulate global climate. It consists of a set of unmanned scientific platforms that record oceanographic, cryospheric, and atmospheric data throughout the year. Data are in ASCII text format.

Comprehensive dataset of 176 Observatories in Mexico as of July, 2025. Includes verified contact information (email, phone), geocoded addresses, customer ratings, reviews, business categories, and operational details. Perfect for market research, lead generation, competitive analysis, and business intelligence. Download a complimentary sample to evaluate data quality and completeness.

Geomagnetic observatory vector (X, Y, Z) and scalar (F) definitive data (quasi-definitive data are available until the definitive data are ready) recorded by the Ebre Observatory institute. Units: nanoteslas (nT). Recording location: Horta de Sant Joan. Instrumentation: Variometers: LEMI-025 suspended 3-axis fluxgate magnetometer sampled at 1 s rate (filtered). Scalar magnetometers: GEM Systems GSM-90 sampled at 10 s rate. Absolute instrument: D/I-fluxgate magnetometer type TDJ6E-NM/FLM-4. Data are available in different interval types: 1-sec data; 1-min, 1-hour, 1-day and 1-month means.

The NOAA National Centers for Environmental Information (formerly National Geophysical Data Center) / World Data Center, Boulder maintains an active database of worldwide geomagnetic observatory data. Historically, magnetic observatories were established to monitor the secular change (variation), of the Earth's magnetic field, and this remains one of their most important functions. This generally involves absolute measurements sufficient in number to monitor instrumental drift and to produce annual means. While the current global network of geomagnetic observatories involves over 70 countries operating more than 200 observatories, the historic database includes observations from more than 600 observatories since the early 1800s. The magnetic observatory data are crucial to the studies of secular change, investigations into the Earth's interior, navigation, communication, and to global modeling efforts. The Earth's magnetic field is described by seven parameters. These are declination (D), inclination (I), horizontal intensity (H), vertical intensity (Z), total intensity (F) and the north (X) and east (Y) components of the horizontal intensity. By convention, declination is considered positive when measured east of north, inclination and vertical intensity positive down, X positive north, and Y positive east. The magnetic field observed on Earth is constantly changing.