Community Inversion Codes (CIC) for Inference of Vector Magnetic Fields from Spectro-Polarimetric Data - PowerPoint PPT Presentation

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Community Inversion Codes (CIC) for Inference of Vector Magnetic Fields from Spectro-Polarimetric Data

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High Altitude Observatory (HAO) National Center for Atmospheric Research (NCAR) ... of atom, simultaneously embracing Hanle, Zeeman, and Kemp polarization effects ... – PowerPoint PPT presentation

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Title: Community Inversion Codes (CIC) for Inference of Vector Magnetic Fields from Spectro-Polarimetric Data


1
Community Inversion Codes (CIC) for Inference of
Vector Magnetic Fields from Spectro-Polarimetric
Data
  • Bruce W. Lites
  • High Altitude Observatory
  • National Center for Atmospheric Research
  • HMI Team Meeting, Palo Alto, 1-2 May 2003

1 May 2003
2
Expanding Usage of Inversion codes
  • New Instrumentation
  • Space SDO, Solar-B, Sunrise, (Solar Orbiter?)
  • Ground-Based ASP, DLSP, SOLIS, POLIS, SST
    (LPSP), TIP, THEMIS, .
  • New applications
  • More physics multi-component, MISMA, LOS
    gradients, non-LTE, MHD models, hyperfine
    structure
  • New regimes chromosphere, prominences, weak
    fields

Outlook substantial and expanding community
needing access to polarimetric inversion software
Bruce Lites, HMI Team Mtg., 2 May 2003
3
New Inversion Techniques
Pattern recognition techniques (Fast!)
  • Principal Components Analysis
  • Neural Networks DIANNE
  • Support Vector Machines

More Physics
  • Chromospheric Non-LTE inversions NICOLE
  • Line-of-Sight Gradients of Field, Atm LILIA
  • Sub-resolution structure multi-component MISMA
  • Hyperfine atomic structure

4
New Regimes
Example Inversion of Prominence HeI D3
Measurements
  • Analysis of full spectral profile of HeI D3
    multiplet
  • Embraces full QED treatment of atom,
    simultaneously embracing Hanle, Zeeman, and Kemp
    polarization effects

25 May 02 1633 UT Courtesy of A. Lopez Ariste
R. Casini
5
CIC A Proposed Repository for Standardized
Inversion Methods. GOALS
  • User support
  • Portable codes platform- and UNIX-like
    OS-compatable
  • Efficiency I.e. optimization for parallel
    architecture
  • User-friendly documentation
  • Modular design to allow easy modification by
    users
  • Frequent updates to incorporate new physics
  • Visualization of results (e.g. AZAM)
  • Uniformity of presentation (I.e., like SOLARSOFT)

6
Status of CIC
  • Initially envisioned as part of the
    still-unfunded NSF community program, Solar
    Magnetism Initiative
  • Hector Socas-Navarro maintains some of his codes
    at CIC website http//www.hao.ucar.edu/public/res
    earch/cic/index.html
  • Need for dedicated, full-time programming support
    in order to realize this as a community resource

7
Benefits of CIC to HMI
  • Standardization of inversion software across
    varied inversion techniques
  • Integrated data visualization, analysis (I.e.
    azimuth ambiguity resolution)
  • Community support for ancillary, coordinated
    vector field data (I.e. chromospheric field
    measurements)
  • Explicit presentation of assumptions,
    approximations, validity leading to inversion
    results

8
In Summary ..
This is a blatant solicitation to the HMI
community for advocacy of an NCAR proposal to
support CIC within the framework of the Living
With a Star program.
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