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aiapy 0.8.dev40+g487a257 documentation

  • Getting Started
  • Preparing AIA data
  • Example gallery
    • Registering and aligning level 1 data
    • Updating pointing and observer keywords in the FITS header
    • Modeling channel degradation over time
    • Correcting for instrument degradation
    • Re-spiking level 1 images
    • Deconvolving images with the instrument Point Spread Function (PSF)
    • Computing wavelength response functions
    • Requesting specific AIA images from the JSOC
  • API reference
    • aiapy (aiapy)
    • Calibration (aiapy.calibrate)
      • correct_degradation
      • degradation
      • estimate_error
      • fetch_spikes
      • fix_observer_location
      • register
      • respike
      • update_pointing
      • get_correction_table
      • get_pointing_table
      • get_error_table
    • Point Spread Functions (aiapy.psf)
      • deconvolve
      • filter_mesh_parameters
      • psf
    • Response (aiapy.response)
      • Channel
    • Utilities (aiapy.util)
      • sdo_location
      • telescope_number
  • Acknowledging or Citing aiapy
  • Changelog
  • Contributing
  • API reference
  • Utilities (aiapy.util)
  • sdo_location

sdo_location#

aiapy.util.sdo_location(time)[source]#

Returns the location of SDO at the given time.

Parameters:

time (astropy.time.Time) – The time can also be supplied in a format compatible with sunpy.time.parse_time().

Return type:

astropy.coordinates.SkyCoord

Notes

This function performs a linear interpolation between the nearest DRMS records on either side of the given time.

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