Tom Berger

Survey Information

    Institution: Lockheed Martin Solar and Astrophysics Lab
    Organizational Affiliation:
Observations

    Providing Observations for WHI: Yes
    Observatory: Hinode SOT
    Type of Observation: Solar filtergrams and dopplergrams
    Coverage for WHI: 100"x100" 200 km resolution solar chromosphere
    Observation Location for WHI: Sun-synch orbit
    Observation Plans for WHI: Will work with filament/prominence program participants to provide SOT observations guidance and post-acquisition data reduction and analysis. Available wavelengths: Ca II H-line 396.8 nm and H-alpha 656.3 nm (filtergrams and dopplergrams).
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Modeling

    Providing Modeling Support for WHI: No
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    Sample Model Output
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Data

    Assisting with Data Coordination: No
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Other

    Other Research Goals:
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