The Virtual Solar Terrestrial Observatory (VSTO) is a unified semantic environment serving data from diverse data archives in the fields of solar, solar-terrestrial, and space physics (SSTSP), currently:
The VSTO portal uses an underlying ontology (i.e. an organized knowledge base of the SSTSP domain) to present a general interface that allows selection and retrieval of products (ascii and binary data files, images, plots) from heterogenous external data services. More detailed information is available on the About the VSTO ontology page.
Please select a starting point:
Data from the CEDAR archive is available in OPeNDAP or ASCII format. A few parameters can be plotted versus time and height. Data from the MLSO archive is available as PG or FITS images.
Before downloading data from the CEDAR database, users are required to agree to the Rules of the Road, which entitles them to a VSTO login. No login is necessary to plot CEDAR data, or to access MLSO data.
NCAR/ESSL/HAO, NCAR/CISL/SCD, and McGuinness Assocaites are engaged in collaborative work on a new NSF-funded project called the Virtual Solar Terrestrial Observatory (VSTO). The prototype VSTO is proposed to be a distributed, scalable education and research environment for searching, integrating, and analyzing observational, experimental, and model databases in the fields of solar, solar-terrestrial, and space physics (SSTSP).
VSTO will comprise a system that provides virtual access to specific SSTSP data, model, tool, and material archives containing items from a variety of space- and ground-based instruments and experiments, as well as individual and community modeling and software efforts bridging research and educational use. The prototype is intended to be a fully functional system addressing a substantial need within the SSTSP community, allowing science projects to advance more rapidly.
For example, in solar coronal physics there is a need to cohesively assemble multi-wavelength images of the dynamic solar upper atmosphere. Space weather model inter-comparisons, and Assimilative Mapping of Ionospheric Electrodynamics results need to be distributed to their communities.
The overall goal is to integrate a balance of data/model holdings, portals, and client software, and a semantically rich, ontology-enabled framework that provides an environment that researchers can use without undue effort as if all the materials were available on his/her local computer. In discussions with data provides and users, the needs are clear:
"Fast access to 'portable' data, in a way that works with the tools we have; information must be easy to access, retrieve, and work with."
Too often users (and data providers) have to deal with the organizational structure of the data sets which varies significantly. Data may be stored at one site in a small number of large files while similar data may be stored at another site in a large number of relatively smaller files. There is an equally large problem with the range of metadata descriptions for the data. Users often only want subsets of the data and struggle with getting it efficiently. One user expresses it as: "(Please) solve the interface problem." VSTO is aimed directly at this pressing issue that impedes scientific progress.
Datasets alone are not sufficient to build a virtual observatory. The VSTO must address the interface problem to bring data to the users' tools, and to the tools within the VSTO, effectively and in a scalable fashion. VSTO will leverage the development of schema (e.g. VSO, Earth System Grid, VHO) that adequately describe the syntax (name of a variable, its type, dimensions, etc. or the procedure name and argument list, etc.) and semantics (what the variable physically is, its units, etc. or what the procedure does and returns, etc.) of the datasets and tools such that a new level of integration and functionality may be realized
The VSTO ontology which is part of the VSTO framework, as well as a more in-depth discussion of how it powers VSTO, is available on the ontology page.
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