ITN 42 - How to obtain physical variables from Mg II h&k lines using IRIS² inversions
1. IRIS²:
IRIS
I
nversion based on
R
epresentative profiles
I
nverted by
S
TiC
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
ITN 42
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3. IRIS² and deepIRIS² in python
3. IRIS² and deepIRIS² in python
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