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photobiology

Package ‘photobiology’ defines a system of classes for storing spectral data and accompanying metadata. For each of these classes specialised summary methods, maths operators and functions are provided. In addition, classes for storing collections of objects of the classes for individual spectra are defined as well as ‘apply’ functions. Extraction and replacement operators are implemented.

Functions for calculation of the position of the sun, times of sunrise and sunset, day length and night length are also implemented.

The package supports storage and manipulation of data for radiation quantities and for optical properties of objects and solutes, as well as response and action spectra for photobiological, photochemical and photoelectrical responses.

This package is the core of a suite of R packages for photobiological calculations described at the r4photobiology web site and in the vignette The R for Photobiology Suite.

Examples

The first example shows you how to estimate solar irradiance in W/m2 under a filter. We use a measured solar spectrum and a measured filter transmission spectrum.

library(photobiology)
e_irrad(sun.spct * yellow_gel.spct)
#>  E_Total 
#> 146.5053 
#> attr(,"time.unit")
#> [1] "second"
#> attr(,"radiation.unit")
#> [1] "total energy irradiance"

The second example shows some simple astronomical calculations for the sun.

geocode <- data.frame(lon = 0, lat = 55)
date <- lubridate::now(tzone = "UTC")
sunrise_time(date, tz = "UTC", geocode = geocode)
#> [1] "2024-08-23 04:50:47 UTC"
day_length(date, tz = "UTC", geocode = geocode)
#> [1] 14.39096

Installation

Installation of the most recent stable version from CRAN:

install.packages("photobiology")

Installation of the current unstable version from R-Universe CRAN-like repository:

install.packages('photobiology', 
                 repos = c('https://aphalo.r-universe.dev', 
                           'https://cloud.r-project.org'))

Once package ‘photobiology’ is installed, installation of the remaining or missing packages in the suite from CRAN (or by adding the repository information as above, from R-Universe):

intalled_pkgs <- installed.packages()[ , 1]
missing_pkgs <- setdiff(photobiology::r4p_pkgs, intalled_pkgs)
if (length(missing_pkgs) > 0) {
 install.packages(missing_pkgs)
}

Installation of the current unstable version from GitHub:

# install.packages("devtools")
devtools::install_github("aphalo/photobiology")

Documentation

HTML documentation is available at (https://docs.r4photobiology.info/photobiology/), including three User Guides.

News on updates to the different packages of the ‘r4photobiology’ suite are regularly posted at (https://www.r4photobiology.info/).

Two articles introduce the basic ideas behind the design of the suite and describe its use: Aphalo P. J. (2015) (https://doi.org/10.19232/uv4pb.2015.1.14) and Aphalo P. J. (2016) (https://doi.org/10.19232/uv4pb.2016.1.15).

A book is under preparation, and the draft is currently available at (https://leanpub.com/r4photobiology/).

A handbook written before the suite was developed contains useful information on the quantification and manipulation of ultraviolet and visible radiation: Aphalo, P. J., Albert, A., Björn, L. O., McLeod, A. R., Robson, T. M., & Rosenqvist, E. (Eds.) (2012) Beyond the Visible: A handbook of best practice in plant UV photobiology (1st ed., p. xxx + 174). Helsinki: University of Helsinki, Department of Biosciences, Division of Plant Biology. ISBN 978-952-10-8363-1 (PDF), 978-952-10-8362-4 (paperback). PDF file available from (https://hdl.handle.net/10138/37558).

Contributing

Pull requests, bug reports, and feature requests are welcome at (https://github.com/aphalo/photobiology).

Citation

If you use this package to produce scientific or commercial publications, please cite according to:

citation("photobiology")
#> To cite package ‘photobiology’ in publications use:
#> 
#>   Aphalo, Pedro J. (2015) The r4photobiology suite. UV4Plants Bulletin,
#>   2015:1, 21-29. DOI:10.19232/uv4pb.2015.1.14
#> 
#> A BibTeX entry for LaTeX users is
#> 
#>   @Article{,
#>     author = {Pedro J. Aphalo},
#>     title = {The r4photobiology suite},
#>     journal = {UV4Plants Bulletin},
#>     volume = {2015},
#>     number = {1},
#>     pages = {21-29},
#>     year = {2015},
#>     doi = {10.19232/uv4pb.2015.1.14},
#>   }

License

© 2012-2024 Pedro J. Aphalo (pedro.aphalo@helsinki.fi). Released under the GPL, version 2 or greater. This software carries no warranty of any kind.

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install.packages('photobiology')

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Version

0.11.3

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Last Published

August 25th, 2024

Functions in photobiology (0.11.3)

D65.illuminant.spct

CIE D65 illuminant data
Tfr_normdiff

transmittance:transmittance normalised difference
Tfr_fraction

transmittance:transmittance fraction
MathFun

Miscellaneous Mathematical Functions
Rfr_fraction

reflectance:reflectance fraction
Rfr_from_n

Reflectance at a planar boundary
A2T

Convert absorbance into transmittance
A.illuminant.spct

CIE A illuminant data
Tfr_ratio

transmittance:transmittance ratio
Trig

Trigonometric Functions
absorptance_spct

Calculate absorptance from spectral absorptance.
absorptance

Absorptance
Rfr_ratio

reflectance:reflectance ratio
Rfr_normdiff

reflectance:reflectance normalised difference
absorbance

Absorbance
absorbance_spct

Calculate absorbance from spectral absorbance.
as.calibration_mspct

Coerce to a collection-of-spectra
any2T

Convert filter quantities.
as.cps_spct

Coerce to a spectrum
as.filter_mspct

Coerce to a collection-of-spectra
as.calibration_spct

Coerce to a spectrum
as.generic_mspct

Coerce to a collection-of-spectra
as.chroma_mspct

Coerce to a collection-of-spectra
as.filter_spct

Coerce or convert into a filter spectrum
as.raw_mspct

Coerce to a collection-of-spectra
as.raw_spct

Coerce to a spectrum
T2Afr

Convert transmittance into absorptance.
T2A

Convert transmittance into absorbance.
auto_hinges

Guess whether insertion of hinges is needed or not
as.object_mspct

Coerce to a collection-of-spectra
as_tod

Convert datetime to time-of-day
add_attr2tb

Copy attributes from members of a generic_mspct
as_quantum

Convert spectral energy irradiance into spectral photon irradiance
adaptive_smoothing

Custom smoothing
as.response_mspct

Coerce to a collection-of-spectra
as.object_spct

Coerce to a spectrum
as.response_spct

Coerce to a spectrum
as.source_mspct

Coerce to a collection-of-spectra
checkSpctVersion

Check that the "spct.version" attribute is set
as.solute_spct

Coerce to a solute spectrum
as_quantum_mol

Convert spectral energy irradiance into spectral photon irradiance
checkTimeUnit

Check the "time.unit" attribute of an existing source_spct object
as.matrix-mspct

Coerce a collection of spectra into a matrix
as.generic_spct

Coerce to a spectrum
check_w.length

Sanity check of wavelengths (internal function).
check_spectrum

Sanity check a spectrum
check_spct

Check validity of spectral objects
check_and_rename_vars

check and rename variables
ciexyzCMF10.spct

Linear energy CIE xyz colour matching function (CMF) 10 deg data
black_body.spct

Theoretical optical bodies
ciexyzCMF2.spct

Linear energy CIE xyz colour matching function (CMF) 2 deg data
as.chroma_spct

Coerce to a spectrum
ciev10.spct

Linear energy CIE 2008 luminous efficiency function 10 deg data
ciev2.spct

Linear energy CIE 2008 luminous efficiency function 2 deg data
collect2mspct

Form a new collection
clean_spct

Clean a spectrum
c

Combine collections of spectra
as.cps_mspct

Coerce to a collection-of-spectra
as.reflector_mspct

Coerce to a collection-of-spectra
as.reflector_spct

Coerce to a spectrum
convertTimeUnit

Convert the "time.unit" attribute of an existing source_spct object
clear.spct

Theoretical spectrum of clear and apaque materials
ccd.spct

Spectral response of a back-thinned CCD image sensor.
convolve_each

Convolve function for collections of spectra
checkMspctVersion

Check that the "mspct.version" attribute is set
clear_photobio.cache

Clear the spectral weights cache
clip_wl

Clip head and/or tail of a spectrum
average_spct

Average spectral data.
beesxyzCMF.spct

Honeybee xyz chromaticity colour matching function data
color_of

Color of an object
as.solar_date

Convert a solar_time object into solar_date object
as.solute_mspct

Coerce to a collection-of-spectra
calc_multipliers

Spectral weights
calc_source_output

Scaled and/or interpolated light-source spectral output
copy_attributes

Copy attributes
as.source_spct

Coerce to a spectrum
cps2irrad

Conversion from counts per second to physical quantities
e_fraction

Energy:energy fraction
e_irrad

Energy irradiance
Extract

Extract or replace parts of a spectrum
Extract_mspct

Extract or replace members of a collection of spectra
as_energy

Convert spectral photon irradiance into spectral energy irradiance
despike

Remove spikes from spectrum
compare_spct

Coarse-grained comparison of two spectra
cone_fundamentals10.spct

Ten-degree cone fundaamentals
diffraction_single_slit

Diffraction
ciexyzCC10.spct

CIE xyz chromaticity coordinates (CC) 10 deg data
ciexyzCC2.spct

CIE xyz chromaticity coordinates 2 deg data
e_ratio

Energy:energy ratio
e_response

Energy-based photo-response
getFilterProperties

Get the "filter.properties" attribute
getHowMeasured

Get the "how.measured" attribute
fit_peaks

Refine position and value of extremes by fitting
fluence

Fluence
class_spct

Query which is the class of a spectrum
clean

Clean (=replace) off-range values in a spectrum
irradiance

Photon or energy irradiance from spectral energy or photon irradiance.
is.generic_mspct

Query class of spectrum objects
div_spectra

Divide two spectra, even if the wavelengths values differ
convertTfrType

Convert the "Tfr.type" attribute
convertThickness

Convert the "thickness" attribute of an existing filter_spct object.
getIdFactor

Get the "idfactor" attribute
getInstrDesc

Get the "instr.desc" attribute
drop_user_cols

Drop user columns
e2q

Convert energy-based quantities into photon-based quantities.
is_scaled

Query whether a generic spectrum has been scaled
enable_check_spct

Enable or disable checks
findMultipleWl

Find repeated w.length values
energy_as_default

Set spectral-data options
e2qmol_multipliers

Calculate energy to quantum (mol) multipliers
energy_irradiance

Calculate (energy) irradiance from spectral irradiance
energy_ratio

Energy:energy ratio
insert_hinges

Insert wavelength values into spectral data.
illuminance

Irradiance
getWhatMeasured

Get the "what.measured" attribute
getTimeUnit

Get the "time.unit" attribute of an existing source_spct object
div-.generic_spct

Arithmetic Operators
find_peaks

Find peaks in a spectrum
dim.generic_mspct

Dimensions of an Object
e2quantum_multipliers

Calculate energy to quantum multipliers
is_tagged

Query if a spectrum is tagged
isValidInstrDesc

Check the "instr.desc" attribute
is.waveband

Query if it is a waveband
format.solar_time

Encode in a Common Format
getScaled

Get the "scaled" attribute
getNormalized

Query the "normalized" and "normalization" attributes
format.tod_time

Encode in a Common Format
make_var_labels

Column or variable labels
log

Logarithms and Exponentials
fscale_spct

fscale a spectrum
na.omit

Handle Missing Values in Objects
fshift

Shift the scale of a spectrum using a summary function
getInstrSettings

Get the "instr.settings" attribute
get_attributes

Get the metadata attributes
getKType

Get the "K.type" attribute
get_peaks

Get peaks and valleys in a spectrum
is_mole_based

Query if a spectrum contains mole or mass based data
is_effective

Is an R object "effective"
day_night

Times for sun positions
defunct

Defunct functions and methods
interpolate_spectrum

Calculate spectral values at a different set of wavelengths
formatted_range

Compute range and format it
eq_ratio

Energy:photon ratio
e_fluence

Energy fluence
spread

Expanse
filter_cps.mspct

Counts per second from a measurement of a plastic film
fscale

Rescale a spectrum using a summary function
f_dispatcher_spct

Math function dispatcher for spectra
normalization

Normalization of an R object
wl_min

Wavelength minimum
wl_midpoint

Midpoint
interpolate_wl

Map spectra to new wavelength values.
fshift_spct

fshift a spectrum
generic_mspct

Collection-of-spectra constructor
insert_spct_hinges

Insert new wavelength values into a spectrum
find_spikes

Find spikes
getWhenMeasured

Get the "when.measured" attribute
head_tail

Return the First and Last Parts of an Object
getWhereMeasured

Get the "where.measured" attribute
green_leaf.spct

Green birch leaf reflectance.
is_normalized

Query whether a generic spectrum has been normalized.
getMspctVersion

Get the "mspct.version" attribute
find_wls

Find wavelength values in a spectrum
normalize

Normalize spectral data
is.old_spct

Query if an object has old class names
merge_attributes

Merge and copy attributes
is.generic_spct

Query class of spectrum objects
msmsply

Multi-spct transform methods
getSoluteProperties

Get the "solute.properties" attribute
getSpctVersion

Get the "spct.version" attribute
getMultipleWl

Get the "multiple.wl" attribute
interpolate_spct

Map a spectrum to new wavelength values.
integrate_xy

Gives irradiance from spectral irradiance.
minus-.generic_spct

Arithmetic Operators
net_irradiance

Net radiation flux
irrad_extraterrestrial

Extraterrestrial irradiance
irrad

Irradiance
wl_max

Wavelength maximum
photons_energy_ratio

Photon:energy ratio
q2e

Convert photon-based quantities into energy-based quantities
photon_ratio

Photo:photon ratio
isValidInstrSettings

Check the "instr.settings" attribute
print.tod_time

Print time-of-day objects
integrate_spct

Integrate spectral data.
is.solar_time

Query class
oper_spectra

Binary operation on two spectra, even if the wavelengths values differ
is_photon_based

Query if a spectrum contains photon- or energy-based data.
is_absorbance_based

Query if a spectrum contains absorbance or transmittance data
rowwise

rowwise functions for collections of spectra
peaks

Peaks or local maxima
print.waveband

Print a "waveband" object
is.summary_generic_spct

Query class of spectrum summary objects
join_mspct

Join all spectra in a collection
s_prod

Product from collection of spectra
replace_bad_pixs

Replace bad pixels in a spectrum
s_range

Range of a collection of spectra
Subset

Subsetting spectra
relative_AM

Relative Air Mass (AM)
mspct_classes

Names of multi-spectra classes
reflectance

Reflectance
reflectance_spct

Calculate reflectance from spectral reflectance
labels

Find labels from "waveband" object
q_fluence

Photon fluence
l_insert_hinges

Insert wavelength values into spectral data.
normalize_range_arg

Normalize a range argument into a true numeric range
rmDerivedSpct

Remove "generic_spct" and derived class attributes.
merge2object_spct

Merge into object_spct
normalized_diff_ind

Calculate a normalized difference.
q_ratio

Photon:photon ratio
split_irradiance

Energy or photon irradiance for split spectrum regions
calendar_change

Solar astronomy using Meeus' algorithm
^.generic_spct

Arithmetic Operators
mod-.generic_spct

Arithmetic Operators
plus-.generic_spct

Arithmetic Operators
q_response

Photon-based photo-response
make_wl_consistent

Make wavelengths consistent
tag

Tag a spectrum
setTfrType

The "Tfr.type" attribute
setTimeUnit

Set the "time.unit" attribute of an existing source_spct object
photodiode.spct

Spectral response of a GaAsP photodiode
pull_sample

Random sample of spectra
prod_spectra

Multiply two spectra, even if the wavelengths values differ
rbindspct

Row-bind spectra
setWhenMeasured

Set the "when.measured" attribute
se.p

Standard error of the mean
setInstrSettings

Set the "instr.settings" attribute
s_sum

Sum from collection of spectra
photon_irradiance

Photon irradiance
print.solar_time

Print solar time and solar date objects
r4p_pkgs

Packages in R for Photobiology suite
s_se

Standard Error of a collection of spectra
q_fraction

Photon:photon fraction
trim_spct

Trim (or expand) head and/or tail of a spectrum
photobiology-package

photobiology: Photobiological Calculations
round

Rounding of Numbers
setMultipleWl

Set the "multiple.wl" attribute
subt_spectra

Subtract two spectra
print.summary_generic_spct

Print spectral summary
s_mean_se

Mean and standard error from collection of spectra
s_sd

Standard Deviation of a collection of spectra
sun_evening.spct

Time series of solar spectral irradiance (measured)
select_spct_attributes

Merge user supplied attribute names with default ones
rgb_spct

RGB color values
wl_range

Wavelength range
tz_time_diff

Time difference between two time zones
phenylalanine.spct

Molar spectral attenuation coefficient of phenylalanine
trim_waveband

Trim (or expand) head and/or tail
subset2mspct

Convert 'long' or tidy spectral data into a collection of spectra
setKType

Set the "K.type" attribute
setWhatMeasured

Set the "what.measured" attribute
subset_attributes

Subset the metadata attributes
v_replace_hinges

Overwrite spectral data values at existing wavelength values.
trimInstrSettings

Trim the "instr.settings" attribute
se

Standard error of the mean
se.m

Standard error of the mean
using_Tfr

Use photobiology options
solar_time

Local solar time
spikes

Spikes
source_spct

Spectral-object constructors
wl_stepsize

Stepsize
uncollect2spct

Extract all members from a collection
resp_spct

Calculate response from spectral response
white_led.source_spct

White led bulb spectrum
split_bands

List-of-wavebands constructor
validate_geocode

Validate a geocode
split_energy_irradiance

Energy irradiance for split spectrum regions
wb_trim_as_default

Set computation options
valleys

Valleys or local minima
wb2tagged_spct

Create tagged spectrum from wavebands
response

Integrated response
s_mean_se_band

Mean plus and minus standard error from collection of spectra
s_median

Median of a collection of spectra
upgrade_spectra

Upgrade one or more spectral objects
split2mspct

Convert a 'wide' or untidy data frame into a collection of spectra
sum_spectra

Add two spectra
sun_daily.spct

Daily solar spectral irradiance (simulated)
trim_tails

Trim (or expand) head and/or tail
smooth_spct

Smooth a spectrum
s_mean

Mean from collection of spectra
qe_ratio

Photon:energy ratio
setHowMeasured

Set the "how.measured" attribute
rmDerivedMspct

Remove "generic_mspct" and derived class attributes.
setSoluteProperties

Set the "solute.properties" attribute
setIdFactor

Set the "idfactor" attribute
print.metadata

Print methods for metadata records
setWhereMeasured

Set the "where.measured" attribute
q_irrad

Photon irradiance
setResponseType

Set the "response.type" attribute
print.generic_spct

Print spectral objects
setBSWFUsed

The "bswf.used" attribute
water_vp_sat

Water vapour pressure
setNormalized

Set the "normalized" and "normalization" attributes
setGenericSpct

Convert an R object into a spectrum object.
summary_spct_classes

Function that returns a vector containing the names of spectral summary classes.
w_length_range2rgb

Wavelength range to rgb color conversion
wls_at_target

Find wavelengths values corresponding to a target spectral value
v_insert_hinges

Insert spectral data values at new wavelength values.
s_e_irrad2rgb

Spectral irradiance to rgb color conversion
wl2wavenumber

Wavelength conversions
water.spct

Molar spectral attenuation coefficient of water
w_length2rgb

Wavelength to rgb color conversion
setFilterProperties

Set the "filter.properties" attribute
s_var

Variance of a collection of spectra
setScaled

Set the "scaled" attribute
spct_metadata

Access metadata
spct_attr2tb

Copy attributes into a tibble
spct_classes

Function returning a vector containing the names of spectra classes.
slash-.generic_spct

Arithmetic Operators
sun_angles

Solar angles
waveband

Waveband constructor method
sun.spct

Solar spectral irradiance (simulated)
sinc

sinc
setInstrDesc

Set the "instr.desc" attribute
two_filters.spct

Transmittance spectrum of plastic films
two_irrads

Compute two irrads for ratio, fraction or normalised difference
setRfrType

The "Rfr.type" attribute
spct_wide2long

Convert spectrum from wide to long form
trimInstrDesc

Trim the "instr.desc" attribute
transmittance_spct

Calculate transmittance from spectral transmittance.
summary.generic_spct

Summary of one or more spectra
times-.generic_spct

Arithmetic Operators
untag

Remove tags
shared_member_class

Classes common to all collection members.
waveband_ratio

Photon or energy ratio
transmittance

Transmittance
wb2rect_spct

Create tagged spectrum from wavebands
upgrade_spct

Upgrade one spectral object
two_transmittances

Compute two transmittances for ratio, fraction or normalised difference
two_reflectances

Compute two reflectances for ratio, fraction or normalised difference
wb2spct

Create spectrum from wavebands
sign

Sign
thin_wl

Thin the density of wavelength values
trim_wl

Trim head and/or tail of a spectrum
split_photon_irradiance

Photon irradiance for split spectrum regions
verbose_as_default

Set error reporting options
twilight2angle

twilight argument check and conversion
ET_ref

Evapotranspiration
D2_spectrum

Calculate deuterium lamp output spectrum from fitted constants
Afr2T

Convert transmittance into absorptance.
FEL_spectrum

Incandescent "FEL" lamp emission spectrum
Ler_leaf.spct

Green Arabidopsis leaf reflectance and transmittance.
D2.UV653

Data for typical calibration lamps