Description Usage Arguments Details Value Author(s) Examples

This is the correction method available in the ViewSpec Pro software from ASD, which aims at correcting steps in the data (see details).

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`x` |
a |

`locations` |
the wavelengths to cut out and interpolate |

The SWIR1 part of the spectrum (1000-1800 nm) is taken as a reference for corrections as it is stable to the instrument sensitivity drift (Beal and Eamon, 2010)

This is based on a description of the splice correction algorithm described in:

Beal, D. and Eamon, M., 1996. Dynamic, Parabolic Linear Transformations of 'Stepped' Radiometric Data. Analytical Spectral Devices Inc., Boulder, CO.

an object of same class as x

Pierre Roudier pierre.roudier@gmail.com

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