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SPASE and the Heliophysics Virtual Observatories

Authors:

J R Thieman ,

Code 690.1, NASA/GSFC, Greenbelt, MD 20771, USA
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D A Roberts,

Code 672, NASA/GSFC, Greenbelt, MD 20771, USA
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T A King,

UCLA, Institute of Geophys. and Planetary Phys., University of California, 5881 Slichter Hall, Los Angeles, CA 90095-1567, USA
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C C Harvey,

CESR -CNRS, B.P. 4346, 9, avenue du Colonel Roche, 31028 Toulouse CEDEX 4, France
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C H Perry,

Rutherford Appleton Laboratory, Chilton, Oxon OX11 0QX, United Kingdom
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P J Richards

Rutherford Appleton Laboratory, Chilton, Oxon OX11 0QX, United Kingdom
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Abstract

The Space Physics Archive Search and Extract (SPASE) project has developed an information model for interoperable access and retrieval of data within the Heliophysics (also known as space and solar physics) science community. The diversity of science data archives within this community has led to the establishment of many virtual observatories to coordinate the data pathways within Heliophysics subdisciplines, such as magnetospheres, waves, radiation belts, etc. The SPASE information model provides a semantic layer and common language for data descriptions so that searches might be made across the whole of the heliophysics data environment, especially through the virtual observatories.
DOI: http://doi.org/10.2481/dsj.SS_IGY-019
How to Cite: Thieman, J.R. et al., (2010). SPASE and the Heliophysics Virtual Observatories. Data Science Journal. 9, pp.IGY85–IGY93. DOI: http://doi.org/10.2481/dsj.SS_IGY-019
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Published on 25 Feb 2010.
Peer Reviewed

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