Future changes to iris_lmsalpy
7. Future changes to iris_lmsalpy#
Changes to iris_lmsalpy are planned for the future. These are:
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
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: \(IRIS^2+\)
A paper will be released on this.