Bill Peterson

Survey Information

    Institution: LASP, University of Colorado
    Organizational Affiliation:
Observations

    Providing Observations for WHI: Yes
    Observatory: FAST
    Type of Observation: Photoelectrons
    Coverage for WHI: Daily photoelectron flux
    Observation Location for WHI: LEO
    Observation Plans for WHI: Photoelectrons have proven useful in calibrating and validating solar EUV intensity below ~ 27 nm where observations are limited until SDO is launched. I will compare TIMED/SEE solar EUV fluxes in the region below 27 nm with the photoelectron observations using an ionospheric model for photoelectron production.
    Sample Data File
    Sample Image: http://lasp.colorado.edu/timas/papers/Peterson/Peterson_flare_2008_working.pdf
Modeling

    Providing Modeling Support for WHI: No
    Model Name:
    Model Web Site:
    Type of Model:
    Model Coverage:
    Sample Model Output
    Sample Model Image
Data

    Assisting with Data Coordination: No
    Data Service:
    Data Service Website:
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    Organizational Affiliation:
Other

    Other Research Goals:
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