spikes | R Documentation |
Function that returns a subset of an R object with observations corresponding to spikes. Spikes are values in spectra that are unusually high compared to neighbors. They are usually individual values or very short runs of similar "unusual" values. Spikes caused by cosmic radiation are a frequent problem in Raman spectra. Another source of spikes are "hot pixels" in CCD and diode arrays.
spikes(x, z.threshold, max.spike.width, na.rm, ...)
## Default S3 method:
spikes(x, z.threshold = NA, max.spike.width = 8, na.rm = FALSE, ...)
## S3 method for class 'numeric'
spikes(x, z.threshold = NA, max.spike.width = 8, na.rm = FALSE, ...)
## S3 method for class 'data.frame'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
...,
y.var.name = NULL,
var.name = y.var.name
)
## S3 method for class 'generic_spct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
var.name = NULL,
...
)
## S3 method for class 'source_spct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
unit.out = getOption("photobiology.radiation.unit", default = "energy"),
...
)
## S3 method for class 'response_spct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
unit.out = getOption("photobiology.radiation.unit", default = "energy"),
...
)
## S3 method for class 'filter_spct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
filter.qty = getOption("photobiology.filter.qty", default = "transmittance"),
...
)
## S3 method for class 'reflector_spct'
spikes(x, z.threshold = 9, max.spike.width = 8, na.rm = FALSE, ...)
## S3 method for class 'solute_spct'
spikes(x, z.threshold = 9, max.spike.width = 8, na.rm = FALSE, ...)
## S3 method for class 'cps_spct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
var.name = "cps",
...
)
## S3 method for class 'raw_spct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
var.name = "counts",
...
)
## S3 method for class 'generic_mspct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
...,
var.name = NULL,
.parallel = FALSE,
.paropts = NULL
)
## S3 method for class 'source_mspct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
unit.out = getOption("photobiology.radiation.unit", default = "energy"),
...,
.parallel = FALSE,
.paropts = NULL
)
## S3 method for class 'response_mspct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
unit.out = getOption("photobiology.radiation.unit", default = "energy"),
...,
.parallel = FALSE,
.paropts = NULL
)
## S3 method for class 'filter_mspct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
filter.qty = getOption("photobiology.filter.qty", default = "transmittance"),
...,
.parallel = FALSE,
.paropts = NULL
)
## S3 method for class 'reflector_mspct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
...,
.parallel = FALSE,
.paropts = NULL
)
## S3 method for class 'solute_mspct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
...,
.parallel = FALSE,
.paropts = NULL
)
## S3 method for class 'cps_mspct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
...,
var.name = "cps",
.parallel = FALSE,
.paropts = NULL
)
## S3 method for class 'raw_mspct'
spikes(
x,
z.threshold = 9,
max.spike.width = 8,
na.rm = FALSE,
...,
var.name = "counts",
.parallel = FALSE,
.paropts = NULL
)
x |
an R object |
z.threshold |
numeric Modified Z values larger than |
max.spike.width |
integer Wider regions with high Z values are not detected as spikes. |
na.rm |
logical indicating whether |
... |
ignored |
var.name, y.var.name |
character Name of column where to look for spikes. |
unit.out |
character One of "energy" or "photon" |
filter.qty |
character One of "transmittance" or "absorbance" |
.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. |
A subset of x
with rows corresponding to spikes.
spikes(default)
: Default returning always NA.
spikes(numeric)
: Default function usable on numeric vectors.
spikes(data.frame)
: Method for "data.frame" objects.
spikes(generic_spct)
: Method for "generic_spct" objects.
spikes(source_spct)
: Method for "source_spct" objects.
spikes(response_spct)
: Method for "response_spct" objects.
spikes(filter_spct)
: Method for "filter_spct" objects.
spikes(reflector_spct)
: Method for "reflector_spct" objects.
spikes(solute_spct)
: Method for "solute_spct" objects.
spikes(cps_spct)
: Method for "cps_spct" objects.
spikes(raw_spct)
: Method for "raw_spct" objects.
spikes(generic_mspct)
: Method for "generic_mspct" objects.
spikes(source_mspct)
: Method for "source_mspct" objects.
spikes(response_mspct)
: Method for "cps_mspct" objects.
spikes(filter_mspct)
: Method for "filter_mspct" objects.
spikes(reflector_mspct)
: Method for "reflector_mspct" objects.
spikes(solute_mspct)
: Method for "solute_mspct" objects.
spikes(cps_mspct)
: Method for "cps_mspct" objects.
spikes(raw_mspct)
: Method for "raw_mspct" objects.
See the documentation for find_spikes
for details of
the algorithm and implementation.
Other peaks and valleys functions:
find_peaks()
,
find_spikes()
,
get_peaks()
,
peaks()
,
replace_bad_pixs()
,
valleys()
,
wls_at_target()
spikes(sun.spct)
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