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

The package supports storage and manipulation of data for radiation quantities and for optical properties of objects.

This package is the core of a suite of R packages for photobiological calculations described at the r4photobiology web site.

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 
#> 146.5044 
#> 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::today(tzone = "UTC")
sunrise_time(date, tz = "UTC", geocode = geocode)
#> [1] "2021-04-03 05:25:39 UTC"
day_length(date, tz = "UTC", geocode = geocode)
#> [1] 13.25112

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

© 2012-2021 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

0.10.6

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GPL (>= 2)

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Last Published

April 4th, 2021

Functions in photobiology (0.10.6)

Afr2T

Convert transmittance into absorptance.
D2_spectrum

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

CIE A illuminant data
FEL_spectrum

Incandescent "FEL" lamp emission spectrum
D2.UV654

Data for typical calibration lamps
D65.illuminant.spct

CIE D65 illuminant data
FEL.BN.9101.165

Data for typical calibration lamps
D2.UV586

Data for typical calibration lamps
D2.UV653

Data for typical calibration lamps
Trig

Trigonometric Functions
A2T

Convert absorbance into transmittance
adaptive_smoothing

Custom smoothing
as.object_spct

Coerce to a spectrum
absorptance_spct

Calculate absorptance from spectral absorptance.
as.reflector_spct

Coerce to a spectrum
as.response_mspct

Coerce to a collection-of-spectra
as.raw_mspct

Coerce to a collection-of-spectra
absorbance_spct

Calculate absorbance from spectral absorbance.
Ler_leaf.spct

Green Arabidopsis leaf reflectance and transmittance.
as.matrix-mspct

Coerce a collection of spectra into a matrix
absorbance

Absorbance
absorptance

Absorptance
T2A

Convert transmittance into absorbance.
auto_hinges

Guess whether insertion of hinges is needed or not
MathFun

Miscellaneous Mathematical Functions
ciev10.spct

Linear energy CIE 2008 luminous efficiency function 10 deg data
average_spct

Average spectral data.
as.generic_mspct

Coerce to a collection-of-spectra
Rfr_from_n

Reflectance at a planar boundary
as.chroma_spct

Coerce to a spectrum
as.chroma_mspct

Coerce to a collection-of-spectra
clear_body.spct

Theoretical clear body
clear_photobio.cache

Clear the spectral weights cache
ciev2.spct

Linear energy CIE 2008 luminous efficiency function 2 deg data
as.generic_spct

Coerce to a spectrum
Ler_leaf_rflt.spct

Green Arabidopsis leaf spectral reflectance.
T2Afr

Convert transmittance into absorptance.
add_attr2tb

Copy attributes from members of a generic_mspct
as_quantum_mol

Convert spectral energy irradiance into spectral photon irradiance
as_energy

Convert spectral photon irradiance into spectral energy irradiance
class_spct

Query which is the class of a spectrum
as_quantum

Convert spectral energy irradiance into spectral photon irradiance
as_tod

Convert datetime to time-of-day
as.object_mspct

Coerce to a collection-of-spectra
as.raw_spct

Coerce to a spectrum
any2T

Convert filter quantities.
Ler_leaf_trns.spct

Green Arabidopsis leaf spectral transmittance.
drop_user_cols

Drop user columns
clean

Clean (=replace) off-range values in a spectrum
as.calibration_spct

Coerce to a spectrum
as.calibration_mspct

Coerce to a collection-of-spectra
as.cps_mspct

Coerce to a collection-of-spectra
fluence

Fluence
enable_check_spct

Enable or disable checks
format.solar_time

Encode in a Common Format
e2q

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

Set spectral-data options
fit_peaks

Refine position and value of extremes by fitting
as.reflector_mspct

Coerce to a collection-of-spectra
as.cps_spct

Coerce to a spectrum
c

Combine collections of spectra
format.tod_time

Encode in a Common Format
get_attributes

Get the metadata attributes
getInstrSettings

Get the "instr.settings" attribute
get_peaks

Get peaks and valleys in a spectrum
getInstrDesc

Get the "instr.desc" attribute
as.filter_mspct

Coerce to a collection-of-spectra
as.filter_spct

Coerce to a spectrum
Ler_leaf_trns_i.spct

Green Arabidopsis leaf spectral transmittance.
as.response_spct

Coerce to a spectrum
as.source_mspct

Coerce to a collection-of-spectra
calc_source_output

Scaled and/or interpolated light-source spectral output
ccd.spct

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

Convert a solar_time object into solar_date object
as.source_spct

Coerce to a spectrum
beesxyzCMF.spct

Honeybee xyz chromaticity colour matching function data
black_body.spct

Theoretical black body
checkSpctVersion

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

Check that the "mspct.version" attribute is set
clip_wl

Clip head and/or tail of a spectrum
collect2mspct

Form a new collection
cps2irrad

Conversion from counts per second to physical quantities
checkTimeUnit

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

Spectral weights
check_spct

Check validity of spectral objects
convertThickness

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

Sanity check a spectrum
color_of

Color of an object
ciexyzCC10.spct

CIE xyz chromaticity coordinates (CC) 10 deg data
day_night

Times for sun positions
compare_spct

Coarse-grained comparison of two spectra
energy_ratio

Energy:energy ratio
energy_irradiance

Calculate (energy) irradiance from spectral irradiance
fshift_spct

fshift a spectrum
getRfrType

Get the "Rfr.type" attribute
generic_mspct

Collection-of-spectra constructor
check_w.length

Sanity check of wavelengths (internal function).
clean_spct

Clean a spectrum
clear.spct

Theoretical spectrum of a clear material
diffraction_single_slit

Diffraction
ciexyzCC2.spct

CIE xyz chromaticity coordinates 2 deg data
ciexyzCMF10.spct

Linear energy CIE xyz colour matching function (CMF) 10 deg data
is.solar_time

Query class
is_scaled

Query whether a generic spectrum has been scaled
is_photon_based

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

Query class of spectrum summary objects
copy_attributes

Copy attributes
convolve_each

Convolve function for collections of spectra
ciexyzCMF2.spct

Linear energy CIE xyz colour matching function (CMF) 2 deg data
dim.generic_mspct

Dimensions of an Object
div-.generic_spct

Arithmetic Operators
mod-.generic_spct

Arithmetic Operators
convertTimeUnit

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

Multi-spct transform methods
div_spectra

Divide two spectra, even if the wavelengths values differ
findMultipleWl

Find repeated w.length values
getScaled

Get the "scaled" attribute
eq_ratio

Energy:photon ratio
spread

Expanse
cone_fundamentals10.spct

Ten-degree cone fundaamentals
convertTfrType

Convert the "Tfr.type" attribute
find_spikes

Find spikes
head_tail

Return the First and Last Part of an Object
find_wls

Find wavelength values in a spectrum
interpolate_spct

Map a spectrum to new wavelength values.
green_leaf.spct

Green birch leaf reflectance.
find_peaks

Find peaks in a spectrum
fscale_spct

fscale a spectrum
fshift

Shift the scale of a spectrum using a summary function
is.generic_spct

Query class of spectrum objects
interpolate_spectrum

Calculate spectral values at a different set of wavelengths
getWhatMeasured

Get the "what.measured" attribute
photon_ratio

Photo:photon ratio
getNormalized

Get the "normalized" attribute
integrate_spct

Integrate spectral data.
getTimeUnit

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

Gives irradiance from spectral irradiance.
defunct

Defunct functions and methods
is_effective

Is an R object "effective"
photons_energy_ratio

Photon:energy ratio
getResponseType

Get the "response.type" attribute
insert_hinges

Insert wavelength values into spectral data.
wl_max

Wavelength maximum
is.waveband

Query if it is a waveband
insert_spct_hinges

Insert new wavelength values into a spectrum
isValidInstrDesc

Check the "instr.desc" attribute
merge2object_spct

Merge into object_spct
calendar_change

Solar astronomy using Meeus' algorithm
is_normalized

Query whether a generic spectrum has been normalized.
mspct_classes

Names of multi-spectra classes
na.omit

Handle Missing Values in Objects
prod_spectra

Multiply two spectra, even if the wavelengths values differ
q2e

Convert photon-based quantities into energy-based quantities
e_ratio

Energy:energy ratio
filter_cps.mspct

Counts per second from a measurement of a plastic film
despike

Remove spikes from spectrum
e_response

Energy-based photo-response
fscale

Rescale a spectrum using a summary function
formatted_range

Compute range and format it
q_response

Photon-based photo-response
q_ratio

Photon:photon ratio
e2qmol_multipliers

Calculate energy to quantum (mol) multipliers
f_dispatcher_spct

Math function dispatcher for spectra
peaks

Peaks or local maxima
s_median

Median of a collection of spectra
wl_min

Wavelength minimum
minus-.generic_spct

Arithmetic Operators
is.old_spct

Query if an object has old class names
getTfrType

Get the "Tfr.type" attribute
getIdFactor

Get the "idfactor" attribute
getSpctVersion

Get the "spct.version" attribute
irrad

Irradiance
interpolate_wl

Map spectra to new wavelength values.
getHowMeasured

Get the "how.measured" attribute
photobiology-package

photobiology: Photobiological Calculations
l_insert_hinges

Insert wavelength values into spectral data.
photon_irradiance

Photon irradiance
photodiode.spct

Spectral response of a GaAsP photodiode
print.tod_time

Print time-of-day objects
e_fluence

Energy fluence
Extract

Extract or replace parts of a spectrum
e2quantum_multipliers

Calculate energy to quantum multipliers
e_irrad

Energy irradiance
setMultipleWl

Set the "multiple.wl" attribute
s_prod

Product from collection of spectra
setNormalized

Set the "normalized" attribute
print.waveband

Print a "waveband" object
qe_ratio

Photon:energy ratio
r4p_pkgs

Packages in R for Photobiology suite
oper_spectra

Binary operation on two spectra, even if the wavelengths values differ
opaque.spct

Theoretical spectrum of an opaque material
wl_range

Wavelength range
rgb_spct

RGB color values
rmDerivedMspct

Remove "generic_mspct" and derived class attributes.
s_mean

Mean from collection of spectra
rbindspct

Row-bind spectra
getBSWFUsed

Get the "bswf.used" attribute
Extract_mspct

Extract or replace members of a collection of spectra
getFilterProperties

Get the "filter.properties" attribute
rowwise

rowwise functions for collections of spectra
print.solar_time

Print solar time and solar date objects
s_e_irrad2rgb

Spectral irradiance to rgb color conversion
setScaled

Set the "scaled" attribute
spct_classes

Function that returns a vector containing the names of spectra classes.
setTfrType

Set the "Tfr.type" attribute
response

Integrated response
print.summary_generic_spct

Print spectral summary
resp_spct

Calculate response from spectral response
getMspctVersion

Get the "mspct.version" attribute
setInstrDesc

Set the "instr.desc" attribute
s_mean_se

Mean and standard error from collection of spectra
setTimeUnit

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

Set the "instr.settings" attribute
getMultipleWl

Get the "multiple.wl" attribute
s_se

Standard Error of a collection of spectra
s_sd

Standard Deviation of a collection of spectra
s_range

Range of a collection of spectra
setWhatMeasured

Set the "what.measured" attribute
s_sum

Sum from collection of spectra
split_bands

List-of-wavebands constructor
getWhereMeasured

Get the "where.measured" attribute
getWhenMeasured

Get the "when.measured" attribute
irradiance

Photon or energy irradiance from spectral energy or photon irradiance.
subset2mspct

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

Access metadata
subt_spectra

Subtract two spectra
sun.data

Solar spectral irradiance (simulated)
trim_wl

Trim head and/or tail of a spectrum
shared_member_class

Classes common to all collection members.
sun.daily.spct

Daily solar spectral irradiance (simulated)
twilight2angle

twilight argument check and conversion
setHowMeasured

Set the "how.measured" attribute
setIdFactor

Set the "idfactor" attribute
is_absorbance_based

Query if a spectrum contains absorbance or transmittance data
labels

Find labels from "waveband" object
isValidInstrSettings

Check the "instr.settings" attribute
sinc

sinc
sign

Sign
is.generic_mspct

Query class of spectrum objects
is_tagged

Query if a spectrum is tagged
join_mspct

Join all spectra in a collection
normalization

Normalization of an R object
log

Logarithms and Exponentials
merge_attributes

Merge and copy attributes
split_energy_irradiance

Energy irradiance for split spectrum regions
slash-.generic_spct

Arithmetic Operators
normalize

Normalize spectral data
normalize_range_arg

Normalize a range argument into a true numeric range
wl_stepsize

Stepsize
sun.spct

Solar spectral irradiance (simulated)
verbose_as_default

Set error reporting options
sun_angles

Solar angles
w_length2rgb

Wavelength to rgb color conversion
setWhenMeasured

Set the "when.measured" attribute
normalized_diff_ind

Calculate a normalized index.
tag

Tag a spectrum
Subset

Subsetting spectra
thin_wl

Thin the density of wavelength values
wb2rect_spct

Create tagged spectrum from wavebands
wb2spct

Create spectrum from wavebands
white_led.source_spct

White led bulb spectrum
white_led.raw_spct

White led bulb spectrum
transmittance_spct

Calculate transmittance from spectral transmittance.
trimInstrDesc

Trim the "instr.desc" attribute
q_fluence

Photon fluence
print

Print a spectral object
^.generic_spct

Arithmetic Operators
q_irrad

Photon irradiance
v_insert_hinges

Insert spectral data values at new wavelength values.
v_replace_hinges

Overwrite spectral data values at existing wavelength values.
untag

Remove tags
setWhereMeasured

Set the "where.measured" attribute
source_spct

Spectral-object constructor
spct_attr2tb

Copy attributes into a tibble
split_irradiance

Energy or photon irradiance for split spectrum regions
plus-.generic_spct

Arithmetic Operators
reflectance

Reflectance
wl_midpoint

Midpoint
reflectance_spct

Calculate reflectance from spectral reflectance
split_photon_irradiance

Photon irradiance for split spectrum regions
times-.generic_spct

Arithmetic Operators
upgrade_spct

Upgrade one spectral object
relative_AM

Relative Air Mass (AM)
polyester.spct

Transmittance spectrum of clear polyester film
replace_bad_pixs

Replace bad pixels in a spectrum
w_length_range2rgb

Wavelength range to rgb color conversion
water_vp_sat

Water vapour pressure
rmDerivedSpct

Remove "generic_spct" and derived class attributes.
se

Standard error of the mean
setFilterProperties

Set the "filter.properties" attribute
round

Rounding of Numbers
setGenericSpct

Convert an R object into a spectrum object.
s_var

Variance of a collection of spectra
setResponseType

Set the "response.type" attribute
tz_time_diff

Time difference between two time zones
transmittance

Transmittance
uncollect2spct

Extract all members from a collection
upgrade_spectra

Upgrade one or more spectral objects
wb2tagged_spct

Create tagged spectrum from wavebands
using_Tfr

Use photobiology options
select_spct_attributes

Merge user supplied attribute names with default ones
smooth_spct

Smooth a spectrum
solar_time

Local solar time
setBSWFUsed

Set the "bswf.used" attribute
summary

Summary of a spectral object
sum_spectra

Add two spectra
trim_tails

Trim (or expand) head and/or tail
split2mspct

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

Spikes
setRfrType

Set the "Rfr.type" attribute
trim_waveband

Trim (or expand) head and/or tail
wb_trim_as_default

Set computation options
validate_geocode

Validate a geocode
white_body.spct

Theoretical white body
valleys

Valleys or local minima
white_led.cps_spct

White led bulb spectrum
wls_at_target

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

Transmittance spectrum of yellow theatrical gel.
sun.daily.data

Daily solar spectral irradiance (simulated)
waveband_ratio

Photon or energy ratio
trim_spct

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

Waveband constructor method
summary_spct_classes

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

Trim the "instr.settings" attribute