Skip to main content
Ctrl+K
SunPy
  • About
    • Our Mission
    • SunPy Project
    • Presentations
    • Meetings
    • Code of Conduct
  • Documentation
    • sunpy
    • aiapy
    • dkist
    • drms
    • irispy
    • ndcube
    • roentgen
    • scope
    • solarmach
    • sunkit-image
    • sunkit-instruments
    • sunkit-magex
    • sunkit-pyvista
    • sunpy-soar
    • sunraster
    • xrtpy
      • pyflct
      • radiospectra
      • ablog
      • mpl-animators
      • streamtracer
  • Packages
  • Get Help
  • Contribute
  • Blog
  • Cite SunPy
  • About ▾
    • Our Mission
    • SunPy Project
    • Presentations
    • Meetings
    • Code of Conduct
  • Documentation ▾
    • sunpy
    • aiapy
    • dkist
    • drms
    • irispy
    • ndcube
    • roentgen
    • scope
    • solarmach
    • sunkit-image
    • sunkit-instruments
    • sunkit-magex
    • sunkit-pyvista
    • sunpy-soar
    • sunraster
    • xrtpy
      • pyflct
      • radiospectra
      • ablog
      • mpl-animators
      • streamtracer
  • Packages
  • Get Help
  • Contribute
  • Blog
  • Cite SunPy
Logo image

irispy 0.7.0 documentation

  • What is IRIS?
  • The irispy tutorial
    • Installation
    • Acquiring Data
    • IRIS Level 2 Data
    • Calibration of IRIS Observations
    • Data Idiosyncrasies
  • Tutorial Gallery
    • How-to
      • Plot a quick SJI
      • Crop IRIS SJI
      • Manipulate spectrograph data
      • Deal with IRIS v34 rasters
      • Open the IRIS Aligned AIA Cubes
    • Calibration
      • Remove Cosmic Ray Hits from IRIS data
      • Apply Radiometric Calibration
      • Remove Dust from IRIS Slit-Jaw Imager
      • Compare Cosmic Ray Removal Backends
    • Co-align
      • Co-align IRIS SJI to SDO/AIA
      • Reproject IRIS SJI (rolled) to SDO/AIA
      • Potential Offset between SJI and SG data
    • Analysis
      • Fit Spectral Models to Spectra
      • Produce Mg II Dopplergrams
      • Study umbral flashes
      • Calculate Spectral Line Moments
      • Calculate Red-Blue Asymmetry
      • O IV Density-Diagnostic Curves
      • Fit Spectral Models to Spectra - Double Gaussian Fitting
  • Known Issues
  • Contributing to irispy
  • API Reference
    • irispy
      • AIACube
      • RasterCollection
      • SJICube
      • SpectrogramCube
      • SpectrogramCubeSequence
    • IO (irispy.io)
      • fits_info
      • read_files
    • meta (irispy.meta)
      • BaseMeta
      • SGMeta
      • SJIMeta
    • SJI (irispy.sji)
      • AIACube
      • SJICube
    • Spectrograph (irispy.spectrograph)
      • RasterCollection
      • SpectrogramCube
      • SpectrogramCubeSequence
    • utils (irispy.utils)
      • calculate_dust_mask
      • calculate_uncertainty
      • get_detector_type
      • image_clipping
      • record_to_dict
      • remove_cosmic_rays
      • density_diagnostic
      • map_ratio_to_quantity
      • remove_dust
      • calculate_moments
      • calculate_red_blue_asymmetry
      • RBAQualityFlag
      • _fit_xput_lite
      • get_interpolated_effective_area
      • get_latest_response
      • calculate_dn_to_radiance_factor
      • convert_photons_per_sec_to_radiance
      • radiometric_calibration
      • reshape_1d_wavelength_dimensions_for_broadcast
      • generate_wobble_movie
  • Changelog
  • Tutorial Gallery
  • How-to

How-to#

These are examples which demonstrate “how-to” concepts.

Plot a quick SJI

Plot a quick SJI

Crop IRIS SJI

Crop IRIS SJI

Manipulate spectrograph data

Manipulate spectrograph data

Deal with IRIS v34 rasters

Deal with IRIS v34 rasters

Open the IRIS Aligned AIA Cubes

Open the IRIS Aligned AIA Cubes

previous

Tutorial Gallery

next

Plot a quick SJI

© Copyright 2026, IRIS Instrument Team @ LMSAL.

Code • Forum • Chat

Built with Sphinx 9.1.0.