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hyperSpec (version 0.98-20140523)

Interface for hyperspectral data, i.e. spectra + meta info (spatial, time, concentration, ...)

Description

This package is an interface to handle hyperspectral data sets in R. I.e. spatially or time-resolved spectra, or spectra with any other kind of information associated with each of the spectra. The spectra can be data as obtained in XRF, UV/VIS, Fluorescence, AES, NIR, IR, Raman, NMR, MS, etc. More generally, any data that is recorded over a discretized variable, e.g. absorbance = f (wavelength), stored as a vector of absorbance values for discrete wavelengths is suitable.

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Install

install.packages('hyperSpec')

Monthly Downloads

3,847

Version

0.98-20140523

License

GPL (>= 3)

Maintainer

Claudia Beleites

Last Published

May 23rd, 2014

Functions in hyperSpec (0.98-20140523)

apply Computes summary statistics for the spectra of a hyperSpec object.

Barbiturates Spectra from .spc example files A time series of mass spectra in a list of hyperSpec objects.

Identifying Spectra and Spectral Data Points This function allows to identify the spectrum and the wavelength of a point in a plot produced by plotspc.

.DollarNames.hyperSpec

command line completion for $

rbind.fill.matrix

Bind matrices by row, and fill missing columns with NA

Quinine Fluorescence Spectra Fluorescence spectra of different dilutions of quinine forming a calibration set.

read.txt.Shimadzu

Reads Shimadzu GCxGC-qMS - Spectra Files (.txt) as exported by Shimadzu Chrome Solution (v. 2.72) Mass Spectrometer: Shimadzu GCMS-QP 2010 Ultra (www.shimadzu.com)

Logging the processing ot a hyperSpec Object Extracts the slot @log of a hyperSpec object.

Calibration- and Timeseries Plots, Depth-Profiles and the like plotc plots intensities of a hyperSpec object over another dimension such as concentration, time, or a spatial coordinate.

Merge hyperSpec objects

Random Samples and Permutations Take a sample of the specified size from the elements of x with or without replacement.

Plotting hyperSpec Objects

Rubberband baseline correction

Comparison of hyperSpec objects

Quick data frame. Experimental version of as.data.frame that converts a list to a data frame, but doesn't do any checks to make sure it's a valid format. Much faster.

Binding hyperSpec Objects Two S3 functions cbind.hyperSpec and rbind.hyperSpec act as an interfaces to cbind2 and rbind2 because neither rBind and cBind nor S4 versions of cbind and rbind do work at the moment.

Empty hyperSpec object

Interactively select a polygon (grid graphics) and highlight points

Convert Principal Component Decomposition or the like into a hyperSpec Object

scan.txt.Renishaw

import Raman measurements from Renishaw ASCII-files import Raman measurements from Renishaw (possibly compressed) .txt file.

Arithmetical Operators: +, -, *, /, ^, %%, %/%, %*%

Function evaluation on hyperSpec objects

File Import Witec Raman

functions for hyperSpec objects

aggregate hyperSpec objects

hyperSpec-package

Package hyperSpec

Creating a hyperSpec Object Like other S4 objects, a hyperSpec object can be created by new. The hyperSpec object is then initialized using the given parameters.

Multivariate normal random numbers

Polynomial Baseline Fitting These functions fit polynomal baselines.

Plot a Map and Identify/Select Spectra in the Map levelplot functions for hyperSpec objects. An image or map of a summary value of each spectrum is plotted. Spectra may be identified by mouse click.

Laser Emission A time series of an unstable laser emission.

Dimnames for hyperSpec objects

The Number of Rows (Spectra), Columns, and Data Points per Spectrum of an hyperSpec Object)

Get and Set Labels of a hyperSpec Object value may be a list or vector of labels giving the new label for each of the entries specified by which.

Math Functions for hyperSpec Objects

Append a Row to the logbook of a hyperSpec Object A log entry is generated and appended to the log of x.

Plotting Spectra Plot the spectra of a hyperSpec object, i.e. intensity over wavelength. Instead of the intensity values of the spectra matrix summary values calculated from these may be used.

hyperSpec-class

Class "hyperSpec"

Plot spectra matrix

Wavelength Binning In order to reduce the spectral resolution and thus gain signal to noise ratio or to reduce the dimensionality of the spectral data set, the spectral resolution can be reduced.

Options for package hyperSpec Functions to access and set hyperSpec's options.

Getting and Setting the Wavelength Axis wl returns the wavelength axis, wl<- sets it.

Sorting the Wavelengths of a hyperSpec Object Rearranges the hyperSpec object so that the wavelength vector is in increasing (or decreasing) order.

hyperSpec unit tests If svUnit is available, run the unit tests and display the results.

Plot multivariate data into colour channels

mark.dendrogram

Mark groups in hclust dendrograms

Distance based on Pearson's $R^2$

Spectra plotting with ggplot2

Validation of hyperSpec objects

spc.smooth.spline

Spectral smoothing by splines

Convert a hyerSpec object to character strings for Display print, show, and summary show the result of as.character.

read.spc.Kaiser

read Kaiser .spc files

read.ENVI.Nicolet

Nicolet uses some more keywords in their header file. read.ENVI.Nicolet therefore appends "description", "z plot titles", and "pixel size" to keys.hdr2log before calling read.ENVI. They are then interpreted as follows: ll{ description giving the position of the first spectrum z plot titles wavelength and intensity axis units, comma separated pixel size interpreted as x and y step size }

Conversion between Wavelength and Spectra Matrix Column Index wl2i returns the column indices for the spectra matrix for the given wavelengths. i2wl converts column indices into wavelengths.

Spectra plotting with ggplot2

Split a hyperSpec object according to groups split divides the hyperSpec object into a list of hyperSpec objects according to the groups given by f.

Covariance matrices for hyperSpec objects

Raman spectra of 2 Chondrocytes in Cartilage A Raman-map (laterally resolved Raman spectra) of chondrocytes in cartilage.

Extract and Replace parts of hyperSpec objects

Mean and Standard Deviation Calculate mean and standard deviation, and mean, mean $\pm$ one standard deviation, respectively.

Interactively select a polygon (grid graphics)

Spectra plotting with ggplot2

spc.NA.linapprox

Impute missing data points

Sweep Summary Statistic out of an hyperSpec Object sweep for hyperSpec objects.

wc word count of ASCII files

Evaluate function on wavelengths of hyperSpec object

read.txt.Horiba

Import Horiba Labspec exported ASCII files

Import for Cytospec mat files

scale,hyperSpec-method

Center and scale hyperSpec object

Conversion of a hyperSpec object into a data.frame or matrix as.data.frame returns x@data (as data.frame) as.matrix returns the spectra matrix x@data$spc as matrix

Paracetamol Spectrum A Raman spectrum of a paracetamol tablet.

Matlab-like Palettes Two palettes going from blue over green to red, approximately as the standard palette of Matlab does. The second one has darker green values and is better suited for plotting lines on white background.

Normalize numbers -> [0, 1]

qplotmap with colour mixing for multivariate overlay

Sequence generation along spectra or wavelengths This function generates sequences along the spectra (rows) or wavelengths of hyperSpec objects.

trellis.factor.key

Color coding legend for factors Modifies a list of lattice arguments (as for levelplot, etc.) according to the factor levels. The colorkey will shows all levels (including unused), and the drawing colors will be set accordingly.

Collapse hyperSpec objects

Import and Export of hyperSpec objects Besides save and load, two general ways to import and export data into hyperSpec objects exist.

Import for Thermo Galactic's spc file format These functions allow to import .spc files. A detailed description of the .spc file format is available at https://ftirsearch.com/features/converters/SPCFileFormat.htm.

JCAMP-DX Import for Shimadzu Library Spectra

loess smoothing interpolation for spectra Spectra can be smoothed and interpolated on a new wavelength axis using loess.