Mario Bisi

Survey Information

    Institution: University of California, San Diego
    Organizational Affiliation:
Observations

    Providing Observations for WHI: No
    Observatory: EISCAT/STELab/Ooty IPS analyses and SMEI white-light analyses
    Type of Observation: Near-all-sky 3D tomographic reconstructions
    Coverage for WHI:
    Observation Location for WHI:
    Observation Plans for WHI: No special plans. Will work on analysing interplanetary scintillation (IPS) and SMEI white-light data to perform 3D reconstructions of the inner heliosphere (out to 3AU) and compare with multi-point in-situ spacecraft such as STEREO, Wind, ACE, etc... where appropriate to validate the reconstructed heliosphere. Will assist where possible in the individual analyses of the European Incoherent SCATter radar (EISCAT) IPS data if needed and also involved with a Solar Mass Ejection Imager (SMEI)-based WHI effort and an EISCAT-SOHO|UVCS effort.
    Sample Data File:
Modeling

    Providing Modeling Support for WHI: Yes
    Model Name: 3D Heliospheric Tomography
    Model Web Site: http://ips.ucsd.edu and http://smei.ucsd.edu
    Type of Model: 3D tomographic reconstruction in terms of speed and density (and the input of magnetic field where possible) of the inner heliosphere
    Model Coverage: Around 15 Solar Radii out to around 3AU
    Sample Model Output
    Sample Model Image
Data

    Assisting with Data Coordination: Yes
    Data Service:
    Data Service Website:
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    Organizational Affiliation:
Other

    Other Research Goals:
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