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Clman-class

* Clman class


Description

Class to store and handle manual continuum lines.

Details

The class is only required if a continuum line is manually adopted or entirely manually created. This is useful if the automatic approaches are not able to identify absorption features because, for instance, the spectrum has two pronounced maxima within the absortion feature of interest.

Clman is defined as Speclib extended by the following two slots:

  • cp: Matrix containing the fix points (continuum points) of each spectrum.

  • hull: Matrix containing the hull of each spectrum.

Normally, it is not necessary to manually change the values in any of the slots above. Use the functions addcp and deletecp to change the hulls manually. Functionality for conversion back to a Speclib with the final hull and the transformed spectra provides function updatecl.

Note

See figure in hsdar-package for an overview of classes in hsdar.

Author(s)

Lukas Lehnert and Hanna Meyer

See Also


hsdar

Manage, Analyse and Simulate Hyperspectral Data

v1.0.3
GPL
Authors
Lukas W. Lehnert [cre, aut] (<https://orcid.org/0000-0002-5229-2282>), Hanna Meyer [ctb], Joerg Bendix [ctb]
Initial release
2020-08-04

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