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Future changes to |IRISLMSALgit|
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Changes to |IRISLMSALgit| are planned for the future.
These are:

* ``extract_irisL2data``

  * Radiative flux calibration from DN to:

    * CGS_LAMBDA: erg cm^-2 s^-1 sr^-1 Å^-1
    * SI_LAMBDA: W m^-2 sr^-1 nm^-1
    * CGS_NU: erg cm^-2 s^-1 sr^-1 Hz^-1
    * SI_NU: W m^-2 sr^-1 Hz^-1
    * PHOTONS: photon s^-1

* ``raster.quick_look()``

  * Identification of spectral lines, including filtering of lines, e.g: "Mg II, Fe"
  * Helioprojective X-Y coordinates
  * Temporal information of each acquisition
  * Getting the data-only from the label of a spectral range
  * Getting the header-only from the label of a spectral range
  * New function returns all the wavelengths observed in a data set.

* A collection of colormaps exported from IDL and NCAR Command Language (NCL)
* Fit of Gaussians to the IRIS lines.
* Recovery of non-thermal velocities for the optical thin lines observed by IRIS (M. Woods)

* A new Python package to invert the IRIS Level 2 raster data: :math:`IRIS^2+`

  * A paper will be released on this.