convolve_each

Convolve function for collections of spectra which applies an operation on
all the individual members of the collection(s) of spectra.

Definitions of classes, methods, operators and functions for use
in photobiology and radiation meteorology and climatology. Calculation of
effective (weighted) and not-weighted irradiances/doses, fluence rates,
transmittance, reflectance, absorptance, absorbance and diverse ratios and
other derived quantities from spectral data. Local maxima and minima: peaks,
valleys and spikes. Conversion between energy-and photon-based units.
Wavelength interpolation. Astronomical calculations related solar angles and
day length. Colours and vision. This package is part of the 'r4photobiology'
suite, Aphalo, P. J. (2015) <doi:10.19232/uv4pb.2015.1.14>.

Pedro Aphalo

photobiology

Photobiological Calculations

Pedro J. Aphalo

Titta K. Kotilainen

Glenn Davis

Agnese Fazio

convolve_each function

<dl><dt>e1</dt>
<dd>an object of class <code>generic_mspct</code> or <code>generic_scpt</code> or
<code>numeric</code></dd>
<dt>e2</dt>
<dd>an object of class <code>generic_mspct</code> or <code>generic_scpt</code> or
<code>numeric</code></dd>
<dt>oper</dt>
<dd>function, usually but not necessarily an operator with two
arguments.</dd>
<dt>sep</dt>
<dd>character Used when pasting the names of members of <code>e1</code> and
<code>e2</code> to form the names of members of the returned collection of
spectra.</dd>
<dt>...</dt>
<dd>additional arguments passed to <code>oper</code> if present.</dd></dl>

Arguments

Convolve function for collections of spectra — convolve_each

<dl>

<dt>e1</dt>
<dd>an object of class <code>generic_mspct</code> or <code>generic_scpt</code> or
<code>numeric</code></dd>


<dt>e2</dt>
<dd>an object of class <code>generic_mspct</code> or <code>generic_scpt</code> or
<code>numeric</code></dd>


<dt>oper</dt>
<dd>function, usually but not necessarily an operator with two
arguments.</dd>


<dt>sep</dt>
<dd>character Used when pasting the names of members of <code>e1</code> and
<code>e2</code> to form the names of members of the returned collection of
spectra.</dd>


<dt>...</dt>
<dd>additional arguments passed to <code>oper</code> if present.</dd>

</dl>

convolve_each: Convolve function for collections of spectra

Description

Usage

Arguments

See Also