ITN 42 - How to obtain physical variables from Mg II h&k lines using IRIS² inversions
  • 1. IRIS²: IRIS Inversion based on Representative profiles Inverted by STiC
    • 1.1. Quick start to invert IRIS Mg II h&k lines with IRIS²
    • 1.2. Limitations of IRIS² inversions
    • 1.3. Understanding the quality of the IRIS² results
      • 1.3.1. The weights and the weighting windows: \(w_i\)
      • 1.3.2. The quality of the fit: \(\chi^2\)
      • 1.3.3. The uncertainty: \(\sigma_p\)
    • 1.4. IRIS² elements in SolarSoft
    • 1.5. Acknowledging \(IRIS^{2}\)
  • 2. IRIS² in SolarSoft
    • 2.1. Standalone installation
    • 2.2. Inversion of IRIS Mg II h&k lines with iris2
    • 2.3. Inversion of a large raster file, a region of interest, or a masked area
    • 2.4. The function iris2
      • 2.4.1. IRIS² Tutorial Videos: inverting IRIS Mg h&k lines with iris2
    • 2.5. Inspecting the IRIS² model atmosphere (and beyond)
      • 2.5.1. The IRIS2 3D Model Inspector window
      • 2.5.2. The IRIS2 Model Atmosphere window
      • 2.5.3. The IRIS2 Fit window
      • 2.5.4. The \(\chi^2\)-map, map_index_db, and map_mu_db maps
    • 2.6. The function show_iris2model
      • 2.6.1. IRIS² Tutorial Videos: inspecting the inversion results with show_iris2model
  • 3. IRIS² and deepIRIS² in python
  • 4. Hands-on tutorial of IRIS² in IDL.
    • 4.1. Installation of minimal IRIS SolarSoft branch (including \(IRIS^{2}\))
    • 4.2. Verifying the minimal \(IRIS^{2}\) SolarSoft and the temporary \(IRIS^{2}\) code installation
    • 4.3. First \(IRIS^{2}\) inversion
      • 4.3.1. Calibration of IRIS Level 2 data
      • 4.3.2. Inspecting the Mg II h&k data cube
      • 4.3.3. Loading the \(IRIS^{2}\) database
      • 4.3.4. Lookind for the closest RP in the \(IRIS^{2}\) database
      • 4.3.5. Inversion of Mg II h&k lines based in RPs inverted by STiC
 
ITN 42 - How to obtain physical variables from Mg II h&k lines using IRIS² inversions
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