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atmosphericRadiationDoseAndFlux

A calculation toolkit for determining radiation dose rates in the atmosphere due to an incoming spectrum of particles from space.

Installation

Requires Python 3.9 or later.

Install from PyPI:

pip install atmosphericRadiationDoseAndFlux

Or, after cloning this repository, create and activate a virtual environment, then install from the cloned directory:

pip install .

For development (including running tests):

pip install -e ".[test]"

Usage

Calculating dose rates from an input spectrum as a function

Radiation dose rates that aircraft experience are dependent on the incoming radiation spectrum from space for each incoming particle type, altitude above ground level and the 'vertical cut-off rigidity' (which is a function of latitude and longitude).

You can directly calculate radiation dose rates from an incoming rigidity spectrum using the calculate_from_rigidity_spec function. calculate_from_rigidity_spec takes in an input rigidity specrum as a Python function, as well as an altitude or a list of altitudes, and outputs the dose rates aircraft will experience at that altitude. You can optionally also include a vertical cut-off rigidity (the default vertical cut-off rigidity is set to 0.0 GV).

The usage of calculate_from_rigidity_spec is:

calculate_from_rigidity_spec(rigiditySpectrum:Function, 
                             altitudesInkm:float|list, 
                             particleName="proton", 
                             inputRigidityBins=None,
                             verticalCutOffRigidity=0.0)

where the input parameters are:

parameter description
rigiditySpectrum callable function: must be specified in units of particles/cm2/sr/GV/s, and as a function of rigidity in GV. rigiditySpectrum can be specified as any callable single argument function, representing an incoming particle spectrum with any distribution. You may wish to use Python's lambda function to do this.
altitudesInkm float or list: if specified as a list, calculations will be performed in a loop over each of the specified altitudes and returned in the output Pandas DataFrame.
particleName str: must be either "proton" or "alpha". Currently using the setting "alpha" actually calculates dose rates associated with all particles species with atomic numbers 2 and greater rather than just for alpha particles. Default = "proton".
inputRigidityBins list: an optional input parameter, do not use unless experienced with using this library. Setting this parameter to a value overrides this module's internal application of the rigiditySpectrum parameter to an internal default set of energy bins for the purpose of calculating dose rates and fluxes.
verticalCutOffRigidity float: units of gigavolts (GV). Default = 0.0.

For example, after importing the module using

from atmosphericRadiationDoseAndFlux import doseAndFluxCalculator as DAFcalc

and defining an input rigidity spectrum as a function;

testA = 2.77578789
testmu = 2.82874076

testRigiditySpectrum = lambda x:testA*(x**(-testmu))

running

DAFcalc.calculate_from_rigidity_spec(testRigiditySpectrum, 
                                    particleName="proton",altitudesInkm=18.5928, verticalCutOffRigidity=0.0)

will return

   altitude (km)      edose      adose      dosee        tn1       tn2  \
0        18.5928  62.219856  41.774429  34.169926  12.323553  7.639987   

        tn3           SEU           SEL  
0  5.108492  7.639987e-13  7.639987e-08 

as a Pandas DataFrame. Here testRigiditySpectrum is a power law distribution in rigidity, with a spectral index of testmu and a value at x = 1 of testA.

The outputted dose rate (or flux) labels represent the following dose rate/flux types:

label dose rate/flux type
adose ambient dose equivalent in µSv/hr
edose effective dose in µSv/hr
dosee dose equivalent in µSv/hr
tn1 >1 MeV neutron flux, in n/cm2/s
tn2 >10 MeV neutron flux, in n/cm2/s
tn3 >60 MeV neutron flux, in n/cm2/s
SEU single event upset rate for an SRAM device in upsets/second/bit
SEL single event latch-up rate for an SRAM device in latch-ups/second/device

Dose rates can also be generated from an energy spectrum using calculate_from_energy_spec, which has the same syntax as calculate_from_rigidity_spec, but where the incoming spectrum (now in units of particles/cm2/sr/(MeV/n)/s) must be specified in terms of kinetic energy per nucleon in MeV/n instead of rigidity and the optional inputRigidityBins parameter is instead inputEnergyBins in MeV/n. For protons, MeV/n is identical to total MeV. For alpha particles and heavier ions, the default energy grid is the MAIRE 50-bin MeV/n grid; converting that grid to rigidity uses the total kinetic energy (A \times E_n).

Calculating dose rates from an input spectrum as an array

While it is recommended that the user uses functions as the method of inputting spectra, you can also use the calculate_from_rigidity_spec_array and calculate_from_energy_spec_array functions to calculate dose rates directly from an array of spectral flux values and energy bins.

The general syntax for inputs to these are:

calculate_from_rigidity_spec_array(
                            inputRigidityBins:list,
                            inputFluxesGV:list, 
                            altitudesInkm:list, 
                            particleName="proton",
                            verticalCutOffRigidity = 0.0)

where inputRigidityBins is the full list of rigidity bin edge locations in GV that the input fluxes specified by inputFluxesGV are specified for. As inputRigidityBins represent the bin edge locations for inputFluxesGV, the length of inputRigidityBins must therefore be exactly 1 greater than the length of inputFluxesGV.

calculate_from_energy_spec_array has a nearly identical syntax to calculate_from_rigidity_spec_array, where the only difference is that the first argument of calculate_from_energy_spec_array must be specified in MeV/n instead of GV, and the second argument is the energy spectrum in particles/cm2/sr/(MeV/n)/s instead of the rigidity spectrum in particles/cm2/sr/GV/s. Rigidity bins are total GV.

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