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VxOs
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  Link   Earth Observing System Clearinghouse (ECHO)
The EOS ClearingHOuse (ECHO) supports efficient discovery and access to Earth Science data. It is a metadata clearinghouse and order broker being built by NASA's Earth Science Data and Information System (ESDIS).
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  Link   European Virtual Observatory (EURO-VO)
The EURO-VO project aims at deploying an operational Virtual Observatory (VO) in Europe. Its objectives are technology take-up and VO compliant resource provision, building the technical infrastructure and to support its utilization by the scientific
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  Link   Global Auroral Imaging Access (GAIA)
GAIA is a virtual observatory providing quick access to summary data from satellite and ground-based instruments that remote sense auroral precipitation.
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  Link   International Virtual Observatory Alliance (IVOA)
IVOA was formed to facilitate the international coordination and collaboration necessary for the development and deployment of the tools, systems and organizational structures necessary to enable the international utilization of astronomical archives
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  Link   US National Virtual Observatory (NVO)
Education site of the National Virtual Observatory. The NVO is a revolutionary new astronomy project developing a set of online tools to link all the world's astronomy data together.
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  Link   US National Virtual Observatory (NVO for scientists)
NVO's objective is to enable new science by greatly enhancing access to astronomical data and computing resources. NVO makes it easy to locate, retrieve, and analyze data from archives and catalogs worldwide.
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  Link   Virtual Heliospheric Observatory (VHO)
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  Link   Virtual Radiation Belt Observatory (ViRBO)
ViRBO offers open access to near-real-time measurements, historical data, analysis and visualization software, and the predictions of empirical models to help in understanding of the structure and variability of Earth's radiation belts.
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  Link   Virtual Solar Observatory (VSO)
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  Link   Virtual Space Physics Observatory (VSPO)
The VSPO is an evolving system trying to make data easily available from all missions relevant to the global problem of the effects of solar particles and fields on the Earth and the solar system.
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