response {photobiology} | R Documentation |
Integrated response
Description
Calculate average photon- or energy-based photo-response.
Usage
response(
spct,
w.band,
unit.out,
quantity,
time.unit,
scale.factor,
wb.trim,
use.hinges,
...
)
## Default S3 method:
response(
spct,
w.band,
unit.out,
quantity,
time.unit,
scale.factor,
wb.trim,
use.hinges,
...
)
## S3 method for class 'response_spct'
response(
spct,
w.band = NULL,
unit.out = getOption("photobiology.radiation.unit", default = "energy"),
quantity = "total",
time.unit = NULL,
scale.factor = 1,
wb.trim = getOption("photobiology.waveband.trim", default = TRUE),
use.hinges = getOption("photobiology.use.hinges", default = NULL),
naming = "default",
...
)
## S3 method for class 'response_mspct'
response(
spct,
w.band = NULL,
unit.out = getOption("photobiology.radiation.unit", default = "energy"),
quantity = "total",
time.unit = NULL,
scale.factor = 1,
wb.trim = getOption("photobiology.waveband.trim", default = TRUE),
use.hinges = getOption("photobiology.use.hinges", default = NULL),
naming = "default",
...,
attr2tb = NULL,
idx = "spct.idx",
.parallel = FALSE,
.paropts = NULL
)
Arguments
spct |
an R object of class "generic_spct". |
w.band |
waveband or list of waveband objects or a numeric vector of length two. The waveband(s) determine the region(s) of the spectrum that are summarized. If a numeric range is supplied a waveband object is constructed on the fly from it. |
unit.out |
character Allowed values |
quantity |
character string One of |
time.unit |
character or lubridate::duration object. |
scale.factor |
numeric vector of length 1, or length equal to that of
|
wb.trim |
logical if |
use.hinges |
logical Flag indicating whether to insert "hinges" into the spectral data before integration so as to reduce interpolation errors at the boundaries of the wavebands. |
... |
other arguments (possibly used by derived methods). |
naming |
character one of |
attr2tb |
character vector, see |
idx |
character Name of the column with the names of the members of the collection of spectra. |
.parallel |
if TRUE, apply function in parallel, using parallel backend provided by foreach |
.paropts |
a list of additional options passed into the foreach function when parallel computation is enabled. This is important if (for example) your code relies on external data or packages: use the .export and .packages arguments to supply them so that all cluster nodes have the correct environment set up for computing. |
Value
A named numeric
vector in the case of methods for individual
spectra, with one value for each waveband
passed to parameter
w.band
. A data.frame
in the case of collections of spectra,
containing one column for each waveband
object, an index column with
the names of the spectra, and optionally additional columns with metadata
values retrieved from the attributes of the member spectra.
Whether returned values are expressed in energy-based or photon-based units
depends on unit.out
. By default values are only integrated, but
depending on the argument passed to parameter quantity
they can be
re-expressed as relative fractions or percentages. In the case of vector
output, names
attribute is set to the name of the corresponding
waveband unless a named list is supplied in which case the names of the
list members are used.
Methods (by class)
-
response(default)
: Default for generic function -
response(response_spct)
: Method for response spectra. -
response(response_mspct)
: Calculates response from aresponse_mspct
Note
The parameter use.hinges
controls speed optimization. The
defaults should be suitable in most cases. Only the range of wavelengths
in the wavebands is used and all BSWFs are ignored.
See Also
Other response functions:
e_response()
,
q_response()