Learn R Programming

⚠️There's a newer version (0.12.0) of this package.Take me there.

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 
#> 146.506 
#> 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] "2023-04-02 05:29:24 UTC"
day_length(date, tz = "UTC", geocode = geocode)
#> [1] 13.14049

Installation

Installation of the most recent stable version from CRAN:

install.packages("photobiology")

Once package ‘photobiology’ is installed, installation of the remaining or missing packages in the suite from CRAN:

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, please 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

© 2012-2023 Pedro J. Aphalo (pedro.aphalo@helsinki.fi). Released under the GPL, version 2 or greater. This software carries no warranty of any kind.

Copy Link

Version

Install

install.packages('photobiology')

Monthly Downloads

649

Version

0.10.17

License

GPL (>= 2)

Issues

Pull Requests

Stars

Forks

Maintainer

Pedro Aphalo

Last Published

May 27th, 2023

Functions in photobiology (0.10.17)

D65.illuminant.spct

CIE D65 illuminant data
D2_spectrum

Calculate deuterium lamp output spectrum from fitted constants
A.illuminant.spct

CIE A illuminant data
D2.UV654

Data for typical calibration lamps
D2.UV653

Data for typical calibration lamps
Rfr_normdiff

reflectance:reflectance normalised difference
Rfr_ratio

reflectance:reflectance ratio
A2T

Convert absorbance into transmittance
ET_ref

Evapotranspiration
T2A

Convert transmittance into absorbance.
T2Afr

Convert transmittance into absorptance.
Afr2T

Convert transmittance into absorptance.
Rfr_fraction

reflectance:reflectance fraction
absorptance

Absorptance
FEL.BN.9101.165

Data for typical calibration lamps
D2.UV586

Data for typical calibration lamps
absorptance_spct

Calculate absorptance from spectral absorptance.
as.chroma_spct

Coerce to a spectrum
as.cps_mspct

Coerce to a collection-of-spectra
MathFun

Miscellaneous Mathematical Functions
Ler_leaf_trns_i.spct

Green Arabidopsis leaf spectral transmittance.
Ler_leaf_rflt.spct

Green Arabidopsis leaf spectral reflectance.
Tfr_ratio

transmittance:transmittance ratio
Trig

Trigonometric Functions
Ler_leaf_trns.spct

Green Arabidopsis leaf spectral transmittance.
Rfr_from_n

Reflectance at a planar boundary
as_quantum

Convert spectral energy irradiance into spectral photon irradiance
as.object_mspct

Coerce to a collection-of-spectra
as.calibration_mspct

Coerce to a collection-of-spectra
as.object_spct

Coerce to a spectrum
any2T

Convert filter quantities.
as.reflector_mspct

Coerce to a collection-of-spectra
as.reflector_spct

Coerce to a spectrum
ccd.spct

Spectral response of a back-thinned CCD image sensor.
as.source_mspct

Coerce to a collection-of-spectra
as.solute_spct

Coerce to a solute spectrum
add_attr2tb

Copy attributes from members of a generic_mspct
FEL_spectrum

Incandescent "FEL" lamp emission spectrum
adaptive_smoothing

Custom smoothing
Ler_leaf.spct

Green Arabidopsis leaf reflectance and transmittance.
checkMspctVersion

Check that the "mspct.version" attribute is set
ciexyzCC10.spct

CIE xyz chromaticity coordinates (CC) 10 deg data
absorbance

Absorbance
ciexyzCC2.spct

CIE xyz chromaticity coordinates 2 deg data
as.response_mspct

Coerce to a collection-of-spectra
calc_source_output

Scaled and/or interpolated light-source spectral output
as.response_spct

Coerce to a spectrum
calc_multipliers

Spectral weights
clean

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

Query which is the class of a spectrum
checkSpctVersion

Check that the "spct.version" attribute is set
clear_body.spct

Theoretical clear body
checkTimeUnit

Check the "time.unit" attribute of an existing source_spct object
as_quantum_mol

Convert spectral energy irradiance into spectral photon irradiance
absorbance_spct

Calculate absorbance from spectral absorbance.
Tfr_fraction

transmittance:transmittance fraction
as.source_spct

Coerce to a spectrum
as.cps_spct

Coerce to a spectrum
as.matrix-mspct

Coerce a collection of spectra into a matrix
as.generic_spct

Coerce to a spectrum
as.filter_mspct

Coerce to a collection-of-spectra
as_energy

Convert spectral photon irradiance into spectral energy irradiance
Tfr_normdiff

transmittance:transmittance normalised difference
as.filter_spct

Coerce or convert into a filter spectrum
as.generic_mspct

Coerce to a collection-of-spectra
clear_photobio.cache

Clear the spectral weights cache
check_and_rename_vars

check and rename variables
check_spct

Check validity of spectral objects
e2qmol_multipliers

Calculate energy to quantum (mol) multipliers
e2quantum_multipliers

Calculate energy to quantum multipliers
auto_hinges

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

Convert a solar_time object into solar_date object
convolve_each

Convolve function for collections of spectra
copy_attributes

Copy attributes
cps2irrad

Conversion from counts per second to physical quantities
as_tod

Convert datetime to time-of-day
day_night

Times for sun positions
as.solute_mspct

Coerce to a collection-of-spectra
average_spct

Average spectral data.
beesxyzCMF.spct

Honeybee xyz chromaticity colour matching function data
ciev2.spct

Linear energy CIE 2008 luminous efficiency function 2 deg data
ciev10.spct

Linear energy CIE 2008 luminous efficiency function 10 deg data
compare_spct

Coarse-grained comparison of two spectra
collect2mspct

Form a new collection
div-.generic_spct

Arithmetic Operators
clip_wl

Clip head and/or tail of a spectrum
color_of

Color of an object
energy_ratio

Energy:energy ratio
as.raw_spct

Coerce to a spectrum
as.calibration_spct

Coerce to a spectrum
as.raw_mspct

Coerce to a collection-of-spectra
eq_ratio

Energy:photon ratio
as.chroma_mspct

Coerce to a collection-of-spectra
check_spectrum

Sanity check a spectrum
black_body.spct

Theoretical black body
check_w.length

Sanity check of wavelengths (internal function).
c

Combine collections of spectra
e_fluence

Energy fluence
ciexyzCMF10.spct

Linear energy CIE xyz colour matching function (CMF) 10 deg data
e_fraction

Energy:energy fraction
div_spectra

Divide two spectra, even if the wavelengths values differ
defunct

Defunct functions and methods
despike

Remove spikes from spectrum
e_irrad

Energy irradiance
e_ratio

Energy:energy ratio
convertThickness

Convert the "thickness" attribute of an existing filter_spct object.
ciexyzCMF2.spct

Linear energy CIE xyz colour matching function (CMF) 2 deg data
find_wls

Find wavelength values in a spectrum
clear.spct

Theoretical spectrum of a clear material
cone_fundamentals10.spct

Ten-degree cone fundaamentals
clean_spct

Clean a spectrum
fit_peaks

Refine position and value of extremes by fitting
drop_user_cols

Drop user columns
convertTfrType

Convert the "Tfr.type" attribute
energy_as_default

Set spectral-data options
spread

Expanse
dim.generic_mspct

Dimensions of an Object
Extract

Extract or replace parts of a spectrum
energy_irradiance

Calculate (energy) irradiance from spectral irradiance
diffraction_single_slit

Diffraction
convertTimeUnit

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

Energy-based photo-response
fshift

Shift the scale of a spectrum using a summary function
enable_check_spct

Enable or disable checks
fshift_spct

fshift a spectrum
format.tod_time

Encode in a Common Format
find_spikes

Find spikes
format.solar_time

Encode in a Common Format
getIdFactor

Get the "idfactor" attribute
fluence

Fluence
find_peaks

Find peaks in a spectrum
getInstrDesc

Get the "instr.desc" attribute
e2q

Convert energy-based quantities into photon-based quantities.
filter_cps.mspct

Counts per second from a measurement of a plastic film
getInstrSettings

Get the "instr.settings" attribute
formatted_range

Compute range and format it
getKType

Get the "K.type" attribute
getFilterProperties

Get the "filter.properties" attribute
getWhatMeasured

Get the "what.measured" attribute
fscale_spct

fscale a spectrum
getHowMeasured

Get the "how.measured" attribute
getWhenMeasured

Get the "when.measured" attribute
fscale

Rescale a spectrum using a summary function
findMultipleWl

Find repeated w.length values
generic_mspct

Collection-of-spectra constructor
getBSWFUsed

Get the "bswf.used" attribute
Extract_mspct

Extract or replace members of a collection of spectra
getWhereMeasured

Get the "where.measured" attribute
f_dispatcher_spct

Math function dispatcher for spectra
getScaled

Get the "scaled" attribute
getMspctVersion

Get the "mspct.version" attribute
get_peaks

Get peaks and valleys in a spectrum
getRfrType

Get the "Rfr.type" attribute
getMultipleWl

Get the "multiple.wl" attribute
getTfrType

Get the "Tfr.type" attribute
getTimeUnit

Get the "time.unit" attribute of an existing source_spct object
green_leaf.spct

Green birch leaf reflectance.
get_attributes

Get the metadata attributes
interpolate_wl

Map spectra to new wavelength values.
getSpctVersion

Get the "spct.version" attribute
integrate_spct

Integrate spectral data.
integrate_xy

Gives irradiance from spectral irradiance.
getSoluteProperties

Get the "solute.properties" attribute
getNormalized

Query the "normalized" and "normalization" attributes
is.solar_time

Query class
is.old_spct

Query if an object has old class names
getResponseType

Get the "response.type" attribute
irrad

Irradiance
is_photon_based

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

Query whether a generic spectrum has been scaled
irrad_extraterrestrial

Extraterrestrial irradiance
insert_hinges

Insert wavelength values into spectral data.
insert_spct_hinges

Insert new wavelength values into a spectrum
join_mspct

Join all spectra in a collection
is_tagged

Query if a spectrum is tagged
irradiance

Photon or energy irradiance from spectral energy or photon irradiance.
interpolate_spct

Map a spectrum to new wavelength values.
make_wl_consistent

Make wavelengths consistent
wl_max

Wavelength maximum
merge_attributes

Merge and copy attributes
merge2object_spct

Merge into object_spct
is.generic_mspct

Query class of spectrum objects
is.generic_spct

Query class of spectrum objects
wl_min

Wavelength minimum
net_irradiance

Net radiation flux
wl_midpoint

Midpoint
na.omit

Handle Missing Values in Objects
illuminance

Irradiance
mspct_classes

Names of multi-spectra classes
log

Logarithms and Exponentials
is_absorbance_based

Query if a spectrum contains absorbance or transmittance data
is_mole_based

Query if a spectrum contains mole or mass based data
normalization

Normalization of an R object
is.waveband

Query if it is a waveband
head_tail

Return the First and Last Parts of an Object
is.summary_generic_spct

Query class of spectrum summary objects
is_normalized

Query whether a generic spectrum has been normalized.
labels

Find labels from "waveband" object
minus-.generic_spct

Arithmetic Operators
photobiology-package

photobiology: Photobiological Calculations
normalize

Normalize spectral data
interpolate_spectrum

Calculate spectral values at a different set of wavelengths
calendar_change

Solar astronomy using Meeus' algorithm
isValidInstrDesc

Check the "instr.desc" attribute
isValidInstrSettings

Check the "instr.settings" attribute
plus-.generic_spct

Arithmetic Operators
photons_energy_ratio

Photon:energy ratio
print.waveband

Print a "waveband" object
oper_spectra

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

Multiply two spectra, even if the wavelengths values differ
opaque.spct

Theoretical spectrum of an opaque material
print

Print spectral collection summary
normalize_range_arg

Normalize a range argument into a true numeric range
print.solar_time

Print solar time and solar date objects
is_effective

Is an R object "effective"
polyester.spct

Transmittance spectrum of clear polyester film
photodiode.spct

Spectral response of a GaAsP photodiode
^.generic_spct

Arithmetic Operators
normalized_diff_ind

Calculate a normalized difference.
q2e

Convert photon-based quantities into energy-based quantities
photon_irradiance

Photon irradiance
msmsply

Multi-spct transform methods
l_insert_hinges

Insert wavelength values into spectral data.
photon_ratio

Photo:photon ratio
q_fluence

Photon fluence
wl_range

Wavelength range
q_fraction

Photon:photon fraction
mod-.generic_spct

Arithmetic Operators
q_ratio

Photon:photon ratio
rbindspct

Row-bind spectra
r4p_pkgs

Packages in R for Photobiology suite
qe_ratio

Photon:energy ratio
print.tod_time

Print time-of-day objects
phenylalanine.spct

Molar spectral attenuation coefficient of phenylalanine
peaks

Peaks or local maxima
print.summary_generic_spct

Print spectral summary
reflectance

Reflectance
reflectance_spct

Calculate reflectance from spectral reflectance
relative_AM

Relative Air Mass (AM)
replace_bad_pixs

Replace bad pixels in a spectrum
response

Integrated response
resp_spct

Calculate response from spectral response
s_e_irrad2rgb

Spectral irradiance to rgb color conversion
rowwise

rowwise functions for collections of spectra
q_response

Photon-based photo-response
s_mean

Mean from collection of spectra
s_mean_se

Mean and standard error from collection of spectra
s_mean_se_band

Mean plus and minus standard error from collection of spectra
rmDerivedMspct

Remove "generic_mspct" and derived class attributes.
s_median

Median of a collection of spectra
rgb_spct

RGB color values
s_prod

Product from collection of spectra
s_range

Range of a collection of spectra
setGenericSpct

Convert an R object into a spectrum object.
setFilterProperties

Set the "filter.properties" attribute
setBSWFUsed

Set the "bswf.used" attribute
select_spct_attributes

Merge user supplied attribute names with default ones
s_sum

Sum from collection of spectra
rmDerivedSpct

Remove "generic_spct" and derived class attributes.
q_irrad

Photon irradiance
round

Rounding of Numbers
setKType

Set the "K.type" attribute
s_sd

Standard Deviation of a collection of spectra
se.p

Standard error of the mean
setMultipleWl

Set the "multiple.wl" attribute
s_se

Standard Error of a collection of spectra
setSoluteProperties

Set the "solute.properties" attribute
setIdFactor

Set the "idfactor" attribute
setTfrType

Set the "Tfr.type" attribute
setHowMeasured

Set the "how.measured" attribute
s_var

Variance of a collection of spectra
se.m

Standard error of the mean
sample_spct

Random sample from collection of spectra
setInstrDesc

Set the "instr.desc" attribute
setInstrSettings

Set the "instr.settings" attribute
shared_member_class

Classes common to all collection members.
setRfrType

Set the "Rfr.type" attribute
sign

Sign
setWhenMeasured

Set the "when.measured" attribute
solar_time

Local solar time
smooth_spct

Smooth a spectrum
setScaled

Set the "scaled" attribute
setWhereMeasured

Set the "where.measured" attribute
split_bands

List-of-wavebands constructor
split2mspct

Convert a 'wide' or untidy data frame into a collection of spectra
spct_wide2long

Convert spectrum from wide to long form
spikes

Spikes
split_energy_irradiance

Energy irradiance for split spectrum regions
split_irradiance

Energy or photon irradiance for split spectrum regions
summary_spct_classes

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

Summary of a collection of spectra
spct_classes

Function returning a vector containing the names of spectra classes.
wl_stepsize

Stepsize
setWhatMeasured

Set the "what.measured" attribute
spct_metadata

Access metadata
setTimeUnit

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

Photon irradiance for split spectrum regions
sum_spectra

Add two spectra
subt_spectra

Subtract two spectra
setResponseType

Set the "response.type" attribute
slash-.generic_spct

Arithmetic Operators
se

Standard error of the mean
Subset

Subsetting spectra
spct_attr2tb

Copy attributes into a tibble
tag

Tag a spectrum
setNormalized

Set the "normalized" and "normalization" attributes
source_spct

Spectral-object constructors
sinc

sinc
sun.daily.data

Daily solar spectral irradiance (simulated)
sun_angles

Solar angles
sun.daily.spct

Daily solar spectral irradiance (simulated)
sun.data

Solar spectral irradiance (simulated)
trimInstrDesc

Trim the "instr.desc" attribute
trimInstrSettings

Trim the "instr.settings" attribute
two_irrads

Compute two irrads for ratio, fraction or normalised difference
two_transmittances

Compute two transmittances for ratio, fraction or normalised difference
two_reflectances

Compute two reflectances for ratio, fraction or normalised difference
twilight2angle

twilight argument check and conversion
untag

Remove tags
trim_tails

Trim (or expand) head and/or tail
subset2mspct

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

Trim (or expand) head and/or tail of a spectrum
transmittance

Transmittance
transmittance_spct

Calculate transmittance from spectral transmittance.
valleys

Valleys or local minima
validate_geocode

Validate a geocode
thin_wl

Thin the density of wavelength values
times-.generic_spct

Arithmetic Operators
trim_waveband

Trim (or expand) head and/or tail
trim_wl

Trim head and/or tail of a spectrum
upgrade_spectra

Upgrade one or more spectral objects
using_Tfr

Use photobiology options
water_vp_sat

Water vapour pressure
w_length_range2rgb

Wavelength range to rgb color conversion
w_length2rgb

Wavelength to rgb color conversion
water.spct

Molar spectral attenuation coefficient of water
verbose_as_default

Set error reporting options
white_led.raw_spct

White led bulb spectrum
upgrade_spct

Upgrade one spectral object
wb2spct

Create spectrum from wavebands
wb2tagged_spct

Create tagged spectrum from wavebands
white_led.cps_spct

White led bulb spectrum
white_led.source_spct

White led bulb spectrum
wl2wavenumber

Wavelength conversions
waveband

Waveband constructor method
waveband_ratio

Photon or energy ratio
wb2rect_spct

Create tagged spectrum from wavebands
uncollect2spct

Extract all members from a collection
tz_time_diff

Time difference between two time zones
white_body.spct

Theoretical white body
wb_trim_as_default

Set computation options
v_insert_hinges

Insert spectral data values at new wavelength values.
wls_at_target

Find wavelengths values corresponding to a target spectral value
sun.spct

Solar spectral irradiance (simulated)
v_replace_hinges

Overwrite spectral data values at existing wavelength values.
yellow_gel.spct

Transmittance spectrum of yellow theatrical gel.