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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)
#>    Total 
#> 146.5044 
#> attr(,"time.unit")
#> [1] "second"
#> attr(,"radiation.unit")
#> [1] "energy irradiance total"

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] "2019-06-08 03:23:05 UTC"
day_length(date, tz = "UTC", geocode = geocode)
#> [1] 17.19741

Installation

Installation of the most recent stable version from CRAN:

install.packages("photobiology")

Installation of the current unstable version from Bitbucket:

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

Documentation

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

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://bitbucket.org/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

© 2012-2019 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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Version

Install

install.packages('photobiology')

Monthly Downloads

1,001

Version

0.9.29

License

GPL (>= 2)

Maintainer

Pedro Aphalo

Last Published

September 11th, 2019

Functions in photobiology (0.9.29)

D2_spectrum

Calculate deuterium lamp output spectrum from fitted constants
D2.UV654

Data for typical calibration lamps
FEL_spectrum

Incandescent "FEL" lamp emission spectrum
Ler_leaf.spct

Green Arabidopsis leaf reflectance and transmittance.
T2Afr

Convert transmittance into absorptance.
T2A

Convert transmittance into absorbance.
absorbance

Absorbance
D2.UV653

Data for typical calibration lamps
D2.UV586

Data for typical calibration lamps
as.reflector_spct

Coerce to a spectrum
as.reflector_mspct

Coerce to a collection-of-spectra
as.calibration_mspct

Coerce to a collection-of-spectra
Ler_leaf_trns.spct

Green Arabidopsis leaf spectral transmittance.
as.raw_mspct

Coerce to a collection-of-spectra
add_attr2tb

Copy attributes from members of a generic_mspct
Ler_leaf_rflt.spct

Green Arabidopsis leaf spectral reflectance.
A.illuminant.spct

CIE A illuminant data
absorbance_spct

Calculate absorbance from spectral absorbance.
as.solar_date

Convert a solar_time object into solar_date object
average_spct

Average spectral data.
as.source_mspct

Coerce to a collection-of-spectra
beesxyzCMF.spct

Honeybee xyz chromaticity colour matching function data
as.raw_spct

Coerce to a spectrum
check_spectrum

Sanity check a spectrum
check_spct

Check validity of spectral objects
A2T

Convert absorbance into transmittance
as.response_mspct

Coerce to a collection-of-spectra
D65.illuminant.spct

CIE D65 illuminant data
as.chroma_spct

Coerce to a spectrum
as.calibration_spct

Coerce to a spectrum
as.chroma_mspct

Coerce to a collection-of-spectra
as_quantum_mol

Convert spectral energy irradiance into spectral photon irradiance
as_quantum

Convert spectral energy irradiance into spectral photon irradiance
FEL.BN.9101.165

Data for typical calibration lamps
Trig

Trigonometric Functions
T2T

Convert transmittance type.
as.cps_spct

Coerce to a spectrum
convolve_each

Convolve function for collections of spectra
as.response_spct

Coerce to a spectrum
copy_attributes

Copy attributes
ccd.spct

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

Check that the "mspct.version" attribute is set
as.object_mspct

Coerce to a collection-of-spectra
as.cps_mspct

Coerce to a collection-of-spectra
as.object_spct

Coerce to a spectrum
c

Combine collections of spectra
black_body.spct

Theoretical black body
Ler_leaf_trns_i.spct

Green Arabidopsis leaf spectral transmittance.
as.filter_mspct

Coerce to a collection-of-spectra
color_of

Color of an object
cps2irrad

Conversion from counts per second to physical quantities
e_response

Energy-based photo-response
findMultipleWl

Find repeated w.length values
energy_as_default

Set spectral-data options
day_night

Times for sun positions
ciexyzCMF2.spct

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

Query which is the class of an spectrum
getInstrSettings

Get the "instr.settings" attribute
find_peaks

Find peaks in a spectrum
clear.spct

Theoretical spectrum of a clear material
MathFun

Miscellaneous Mathematical Functions
checkSpctVersion

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

Get the "when.measured" attribute
getMspctVersion

Get the "mspct.version" attribute
ciexyzCMF10.spct

Linear energy CIE xyz colour matching function (CMF) 10 deg data
ciexyzCC2.spct

CIE xyz chromaticity coordinates 2 deg data
checkTimeUnit

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

Coerce to a spectrum
as.generic_mspct

Coerce to a collection-of-spectra
getWhereMeasured

Get the "where.measured" attribute
integrate_spct

Integrate spectral data.
as.source_spct

Coerce to a spectrum
clean

Clean (=replace) off-range values in a spectrum
ciev2.spct

Linear energy CIE 2008 luminous efficiency function 2 deg data
e2quantum_multipliers

Calculate energy to quantum multipliers
as_energy

Convert spectral photon irradiance into spectral energy irradiance
e_fluence

Energy fluence
ciexyzCC10.spct

CIE xyz chromaticity coordinates (CC) 10 deg data
fshift_spct

fshift a spectrum
fscale_spct

fscale a spectrum
fshift

Shift the scale of a spectrum using a summary function
fscale

Rescale a spectrum using a summary function
absorptance

Absorptance
convertTimeUnit

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

Get the "normalized" attribute
get_peaks

Get peaks and valleys in a spectrum
get_attributes

Get the metadata attributes
getMultipleWl

Get the "multiple.wl" attribute
irradiance

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

Solar astronomy using Meeus' algorithm
l_insert_hinges

Insert wavelength values into spectral data.
is.generic_mspct

Query class of spectrum objects
absorptance_spct

Calculate absorptance from spectral absorptance.
clear_body.spct

Theoretical clear body
e2q

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

Clean a spectrum
Extract

Extract or replace parts of a spectrum
Extract_mspct

Extract or replace members of a collection of spectra
as.generic_spct

Coerce to a spectrum
formatted_range

Compute range and format it
getTfrType

Get the "Tfr.type" attribute
format.solar_time

Encode in a Common Format
getSpctVersion

Get the "spct.version" attribute
defunct

Defunct functions and methods
interpolate_spct

Map a spectrum to new wavelength values.
e_irrad

Energy irradiance
e2qmol_multipliers

Calculate energy to quantum (mol) multipliers
e_ratio

Energy:energy ratio
wl_midpoint

Midpoint
photobiology-package

photobiology: Photobiological Calculations
peaks

Peaks or local maxima
print.solar_time

Print solar time and solar date objects
merge_attributes

Merge and copy attributes
is.waveband

Query if it is a waveband
interpolate_spectrum

Calculate spectral values at a different set of wavelengths
isValidInstrDesc

Check the "instr.desc" attribute
dim.generic_mspct

Dimensions of an Object
energy_irradiance

Calculate (energy) irradiance from spectral irradiance
as.matrix-mspct

Coerce a collection of spectra into a matrix
fluence

Fluence
getInstrDesc

Get the "instr.desc" attribute
find_wls

Find wavelength values in a spectrum
is.solar_time

Query class
getIdFactor

Get the "idfactor" attribute
is.summary_generic_spct

Query class of spectrum summary objects
energy_ratio

Energy:energy ratio
is_absorbance_based

Query if a spectrum contains absorbance or transmittance data
isValidInstrSettings

Check the "instr.settings" attribute
print.summary_generic_spct

Print spectral summary
getHowMeasured

Get the "how.measured" attribute
getBSWFUsed

Get the "bswf.used" attribute
photons_energy_ratio

Photon:energy ratio
q_fluence

Photon fluence
photon_ratio

Photo:photon ratio
q2e

Convert photon-based quantities into energy-based quantities
getRfrType

Get the "Rfr.type" attribute
reflectance_spct

Calculate reflectance from spectral reflectance
reflectance

Reflectance
integrate_xy

Gives irradiance from spectral irradiance.
as_tod

Convert date to time-of-day in hours, minutes or seconds
getScaled

Get the "scaled" attribute
green_leaf.spct

Green birch leaf reflectance.
setTfrType

Set the "Tfr.type" attribute
s_mean_se

Mean and standard error from collection of spectra
s_median

Median of a collection of spectra
setTimeUnit

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

Photon irradiance for split spectrum regions
wl_stepsize

Stepsize
is_photon_based

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

Query whether a generic spectrum has been scaled
auto_hinges

Guess whether insertion of hinges is needed or not
sun.data

Solar spectral irradiance (simulated)
wl_min

Wavelength minimum
is.old_spct

Query if an object has old class names
is.generic_spct

Query class of spectrum objects
head_tail

Return the First and Last Part of an Object
minus-.generic_spct

Arithmetic Operators
calc_source_output

Scaled and/or interpolated light-source spectral output
check_w.length

Sanity check of wavelengths (internal function).
calc_multipliers

Spectral weights
mod-.generic_spct

Arithmetic Operators
sun.spct

Solar spectral irradiance (simulated)
is_effective

Is an R object "effective"
normalize_range_arg

Normalize a range argument into a true numeric range
normalized_diff_ind

Calculate a normalized index.
is_normalized

Query whether a generic spectrum has been normalized.
log

Logarithms and Exponentials
labels

Find labels from "waveband" object
qe_ratio

Photon:energy ratio
q_response

Photon-based photo-response
ciev10.spct

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

Theoretical spectrum of an opaque material
msmsply

Multi-spct transform methods
s_prod

Product from collection of spectra
response

Integrated response
slash-.generic_spct

Arithmetic Operators
s_range

Range of a collection of spectra
rgb_spct

RGB color values
se

Standard error of the mean
summary

Summary of a spectral object
setAfrType

Set the "Afr.type" attribute
sign

Sign
wl_range

Wavelength range
oper_spectra

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

Divide two spectra, even if the wavelengths values differ
spread

Expanse
filter_cps.mspct

Counts per second from a measurement of a plastic film
clip_wl

Clip head and/or tail of a spectrum
eq_ratio

Energy:photon ratio
f_dispatcher_spct

Math function dispatcher for spectra
div-.generic_spct

Arithmetic Operators
clear_photobio.cache

Clear the spectral weights cache
generic_mspct

Collection-of-spectra constructor
photodiode.spct

Spectral response of a GaAsP photodiode
upgrade_spct

Upgrade one spectral object
waveband_ratio

Photon or energy ratio
sun_angles

Solar angles
tag

Tag a spectrum
upgrade_spectra

Upgrade one or more spectral objects
summary_spct_classes

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

Use photobiology options
transmittance

Transmittance
times-.generic_spct

Arithmetic Operators
mspct_classes

Names of multi-spectra classes
getAfrType

Get the "Afr.type" attribute
valleys

Valleys or local minima
verbose_as_default

Set error reporting options
v_insert_hinges

Insert spectral data values at new wavelength values.
getWhatMeasured

Get the "what.measured" attribute
getTimeUnit

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

Print a "waveband" object
na.omit

Handle Missing Values in Objects
print

Print a spectral object
^.generic_spct

Arithmetic Operators
wb2rect_spct

Create tagged spectrum from wavebands
insert_hinges

Insert wavelength values into spectral data.
prod_spectra

Multiply two spectra, even if the wavelengths values differ
round

Rounding of Numbers
rbindspct

Row-bind spectra
rmDerivedMspct

Remove "generic_mspct" and derived class attributes.
photon_irradiance

Photon irradiance
s_mean

Mean from collection of spectra
setGenericSpct

Convert an R object into a spectrum object.
setBSWFUsed

Set the "bswf.used" attribute
s_e_irrad2rgb

Spectral irradiance to rgb color conversion
setWhereMeasured

Set the "where.measured" attribute
rowwise

rowwise functions for collections of spectra
white_led.cps_spct

White led bulb spectrum
white_led.raw_spct

White led bulb spectrum
insert_spct_hinges

Insert new wavelength values into a spectrum
interpolate_wl

Map spectra to new wavelength values.
rmDerivedSpct

Remove "generic_spct" and derived class attributes.
s_se

Standard Error of a collection of spectra
s_sd

Standard Deviation of a collection of spectra
setMultipleWl

Set the "multiple.wl" attribute
setNormalized

Set the "normalized" attribute
join_mspct

Join all spectra in a collection
irrad

Irradiance
normalization

Normalization of an R object
merge2object_spct

Merge into object_spct
wl_max

Wavelength maximum
is_tagged

Query if it is an spectrum is tagged
shared_member_class

Classes common to all collection members.
spct_classes

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

Spectral-object constructor
sun.daily.data

Daily solar spectral irradiance (simulated)
s_sum

Sum from collection of spectra
solar_time

Local solar time
smooth_spct

Smooth a spectrum
subt_spectra

Subtract two spectra
s_var

Variance of a collection of spectra
setIdFactor

Set the "idfactor" attribute
setHowMeasured

Set the "how.measured" attribute
wb2spct

Create spectrum from wavebands
sum_spectra

Add two spectra
yellow_gel.spct

Transmittance spectrum of yellow theatrical gel.
wb2tagged_spct

Create tagged spectrum from wavebands
normalize

Normalize spectral data
setWhatMeasured

Set the "what.measured" attribute
sun.daily.spct

Daily solar spectral irradiance (simulated)
trim_spct

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

Trim the "instr.settings" attribute
tz_time_diff

Time difference between two time zones
Subset

Subsetting spectra
split2mspct

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

List-of-wavebands constructor
setWhenMeasured

Set the "when.measured" attribute
subset2mspct

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

Set computation options
water_vp_sat

Water vapour pressure
waveband

Waveband constructor method
untag

Remove tags
white_body.spct

Theoretical white body
plus-.generic_spct

Arithmetic Operators
q_irrad

Photon irradiance
relative_AM

Relative Air Mass (AM)
polyester.spct

Transmittance spectrum of clear polyester film
q_ratio

Photon:photon ratio
setInstrSettings

Set the "instr.settings" attribute
resp_spct

Calculate response from spectral response
setScaled

Set the "scaled" attribute
setInstrDesc

Set the "instr.desc" attribute
setRfrType

Set the "Rfr.type" attribute
trim_tails

Trim (or expand) head and/or tail
split_energy_irradiance

Energy irradiance for split spectrum regions
twilight2angle

twilight argument check and conversion
trim_waveband

Trim (or expand) head and/or tail
trim_wl

Trim head and/or tail of a spectrum
split_irradiance

Energy or photon irradiance for split spectrum regions
w_length_range2rgb

Wavelength range to rgb color conversion
w_length2rgb

Wavelength to rgb color conversion
transmittance_spct

Calculate transmittance from spectral transmittance.
validate_geocode

Validate a geocode
wls_at_target

Find wavelengths values corresponding to a target spectral value
trimInstrDesc

Trim the "instr.desc" attribute
v_replace_hinges

Overwrite spectral data values at existing wavelength values.
white_led.source_spct

White led bulb spectrum