SOI Team Science Investigations

The core scientific program of SOI is to be achieved through a set of well-defined team science objectives. The activities of the science teams are summarized here and described in more detail under the individual home pages.

The SOI science teams individually define the scientific activities, both observation and analysis, needed to achieve their objectives. Each team has a Team Leader who is responsible for organizing the team and its activities. Actual development and conduct of the required observing procedures and data processing at the Science Support Center is directed by a Local Coordinator, a scientist resident at either Stanford or Lockheed and an active member of the team if possible. The Local Coordinator works closely with a designated Lead Programmer in development efforts and operations. The Local Coordinator is also responsibile for the relevant descriptive pages, and forms for updating the information are provided.

Note: Not all of the Team Science Working Groups have completed the WWW pages describing the Team's science objectives. Please see the Original SOI Science Objectives for a terse summary of the topics involved.

Internal Rotation (2-D Inversions) - Jesper Schou; SOI-Rotation@solar.stanford.edu
Structure Inversions - Alexander Kosovichev; SOI-Structure@solar.stanford.edu
Hilbert Transform Analysis - Alexander Kosovichev; SOI-Hilbert@solar.stanford.edu
Ring Diagram Analyis for Convective Structures - Rick Bogart; SOI-Rings@solar.stanford.edu
Time-Distance Analysis for Convective Structures - Tom Duvall; SOI-TimeDistance@solar.stanford.edu
Active Region Seismology - Ted Tarbell; SOI-ActiveRegions@solar.stanford.edu
GOLF Intercomparison - Rick Bogart; SOI-GOLF@solar.stanford.edu
VIRGO Intercomparison - Todd Hoeksema; SOI-VIRGO@solar.stanford.edu
Limb Figure Analysis - Rick Bogart; SOI-Limb@solar.stanford.edu
Surface Flows and Structures - Neal Hurlburt; SOI-Flows@solar.stanford.edu
Coronal Synoptic Field - Xue Pu Zhao; SOI-Corona@solar.stanford.edu
Photospheric Magnetic Field - Todd Hoeksema; SOI-Magnetic@solar.stanford.edu
Summary Data - Rock Bush; SOI-Summary@solar.stanford.edu

The following function as interest groups only:

Excitation and Damping of Modes; SOI-Excitation@solar.stanford.edu
Flux Budget; SOI-FluxBudget@solar.stanford.edu
MDI Instrument Performance; SOI-Performance@solar.stanford.edu
Mode Physics; SOI-Modes@solar.stanford.edu
Structure of the Solar Atmosphere; SOI-Atmosphere@solar.stanford.edu
SOHO Joint Observing Programs; SOI-JOPs@solar.stanford.edu
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Page last revised Wednesday, 05-Jan-2000 14:51:15 PST