Constructing a Data System to Support Analysis of the Whole Heliosphere Interval

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2162 Solar Cycle Variations (7536), 2784 Solar Wind/Magnetosphere Interactions, 6025 Interactions With Solar Wind Plasma And Fields, 7536 Solar Activity Cycle (2162), 7538 Solar Irradiance

Scientific paper

The Whole Heliosphere Interval is an internationally coordinated observing and modeling effort to characterize the 3-dimensional interconnected solar-heliospheric-planetary system. The WHI observing campaigns began with the 3-D solar structure from solar Carrington Rotation 2068, which ran from March 20 to April 16, 2008, and traced these structures through the heliosphere and into geospace. The WHI team has developed a data and modeling clearinghouse to create a unified point of entry into the disparate data sets spanning across the traditional disciplinary boundaries. Linkages are provided to data from the special observing programs conducted by many observatories for the WHI effort, models that looked in detail at the WHI and the many other data sets and models from the interval. We also explore the Virtual Observatory landscape and highlight their contributions to the development of a more complete understanding of the entire heliophysical system.

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