isofit.configs.sections.input_config
====================================

.. py:module:: isofit.configs.sections.input_config


Classes
-------

.. autoapisummary::

   isofit.configs.sections.input_config.InputConfig


Module Contents
---------------

.. py:class:: InputConfig(sub_configdic: dict = None)

   Bases: :py:obj:`isofit.configs.base_config.BaseConfigSection`


   Base Configuration Section from which all Configuration Sections inherit. Handles shared functionality like getting,
   setting, and cleaning configuration options.


   .. py:attribute:: _measured_radiance_file_type


   .. py:attribute:: measured_radiance_file
      :value: None


      Input radiance file.  Can be either a .mat, .txt, or ENVI formatted binary cube.
      Used for inverse-modeling (radiance -> reflectance).

      :type: str


   .. py:attribute:: _reference_reflectance_file_type


   .. py:attribute:: reference_reflectance_file
      :value: None


      Input reference reflectance (to be compared against) file.  Can be either a .mat, .txt, or ENVI formatted binary cube.
      Used for radiometric calibration.

      :type: str


   .. py:attribute:: _reflectance_file_type


   .. py:attribute:: reflectance_file
      :value: None


      Input reflectance file.  Can be either a .mat, .txt, or ENVI formatted binary cube.
      Used for forward-modeling (reflectance -> radiance).

      :type: str


   .. py:attribute:: _obs_file_type


   .. py:attribute:: obs_file
      :value: None


      Input 'obs', or observation, file.  Can be either a .mat, .txt, or ENVI formatted binary cube.
      Provides information about the conditions during observaiton.  Assumed to be in the band-wise format:
      {path length, to-sensor azimuth, to-sensor zenith, to-sun azimuth, to-sun zenith, phase, slope, aspect, cosine i,
      UTC time}

      :type: str


   .. py:attribute:: _glt_file_type


   .. py:attribute:: glt_file
      :value: None


      Input glt file.  Can be either a .mat, .txt, or ENVI formatted binary cube.
      Provides (x,y) offset information for the spatial location of raw-space input files

      :type: str


   .. py:attribute:: _loc_file_type


   .. py:attribute:: loc_file
      :value: None


      Input 'loc', or location, file.  Can be either a .mat, .txt, or ENVI formatted binary cube.
      Provides per-pixel lat, long, and elevation information.

      :type: str


   .. py:attribute:: _background_reflectance_file_type


   .. py:attribute:: background_reflectance_file
      :value: None


      Background reflectance file used for spatial inference.
      Should be an ENVI formatted binary cube that is the same
      dimensions as the input data cube.

      :type: str


   .. py:attribute:: _radiometry_correction_file_type


   .. py:attribute:: radiometry_correction_file
      :value: None


      Input radiometric correction file.  Can be either a .mat, .txt, or ENVI formatted binary cube.
      Used to make minor channelized corrections to account for slight systematic errors not captured in calibration.

      :type: str


   .. py:attribute:: _skyview_factor_file_type


   .. py:attribute:: skyview_factor_file
      :value: None


      Input Skyview file.  Can be either a .mat, .txt, or ENVI formatted binary cube.
      Used to modulate incoming diffuse radiance from fraction of viewable sky.

      :type: str


   .. py:method:: _check_config_validity() -> List[str]