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@datafire/amentum_space_cosmic_ray

v3.0.0

Published

DataFire integration for Cosmic Ray API - atmospheric radiation doses and intensities using the PARMA model

Downloads

2

Readme

@datafire/amentum_space_cosmic_ray

Client library for Cosmic Ray API - atmospheric radiation doses and intensities using the PARMA model

Installation and Usage

npm install --save @datafire/amentum_space_cosmic_ray
let amentum_space_cosmic_ray = require('@datafire/amentum_space_cosmic_ray').create();

.then(data => {
  console.log(data);
});

Description

High energy galactic cosmic rays (GCR) and bursts of solar energetic particles (SEP) collide with gases in the atmosphere, leading to a cascade of nuclear and electromagnetic reactions. The result is a complex mix of ionising radiation, the intensity and composition of which varies spatially and temporally. Understanding this mix is important for a variety of applications, including estimating the radiation exposure of aircrew, pilots, and frequent flyers during air travel. The PARMA model, developed by the Japan Atomic Energy Agency (JAEA), can instantaneously estimate cosmic ray fluxes of neutrons, protons, ions, muons, electrons, positrons, and photons for a given date, latitude, longitude, and altitude. A comprehensive description of PARMA can be found in the publications here and here. The Terms and Conditions of PARMA are described here. Use of the API acknowledges you have read and agreed to those Terms and Conditions. We provide access to the PARMA model via an easy-to-use web API. Solar energetic particle effects are not modelled by PARMA. The API is rate limited to 10,000 calls per month and for non commercial use. Contact [email protected] to discuss commercial use. Help us improve the quality of our web APIs by completing our 2 minute survey here. Amentum Pty Ltd is not responsible nor liable for any loss or damage of any sort incurred as a result of using the API. Copyright Amentum Pty Ltd 2020.

Actions

app.api_parma.endpoints.PARMA.ambient_dose

The ambient dose equivalent, H*(10), is an operational quantity that simulates the human body by measuring the dose equivalent at a depth of 10 mm within a tissue equivalent sphere of 300 mm diameter. It is a measurable quantity that is used to calibrate area monitors (radiation detectors) for mixed radiation fields. Use this endpoint if you are comparing model predictions to measurements.

amentum_space_cosmic_ray.app.api_parma.endpoints.PARMA.ambient_dose({
  "latitude": 0,
  "longitude": 0,
  "year": 0,
  "month": 0,
  "day": 0,
  "particle": ""
}, context)

Input

  • input object
    • altitude number: Altitude (in km). The minimum is 0 m, the maximum is 47 km (the upper limit of the stratosphere).
    • atmospheric_depth number: Atmospheric depth from the top of the atmosphere (in units of g/cm2). The minimum is 0.913 g/cm2, the maximum is 1032.66 g/cm2. WARNING: you can specify either altitude OR atmospheric depth, not both.
    • latitude required number: Latitude. -90 (S) to 90 (N).
    • longitude required number: Longitude. -180 (W) to 180 (E).
    • year required integer: Year in YYYY.
    • month required integer: Month in MM.
    • day required integer: Day in DD.
    • particle required string (values: total, e-, e+, mu+, mu-, gamma, neutron, proton, alpha): The particle type as a string. Specifying 'total', only used for the dose calculation, returns the dose for all particle types.

Output

  • output object
    • units string
    • value string

app.api_parma.endpoints.PARMA.differential_intensity

The differential intensity of a particle is a directional quantity that describes the number of particles per unit area, per unit solid angle, per unit energy, and per unit time. The API leverages the functionality of PARMA to calculate differential intensity distributions with energies in units of MeV and Intensity in units of /cm2/sr/MeV/s.

amentum_space_cosmic_ray.app.api_parma.endpoints.PARMA.differential_intensity({
  "latitude": 0,
  "longitude": 0,
  "year": 0,
  "month": 0,
  "day": 0,
  "particle": "",
  "angle": 0
}, context)

Input

  • input object
    • altitude number: Altitude (in km). The minimum is 0 m, the maximum is 47 km (the upper limit of the stratosphere).
    • atmospheric_depth number: Atmospheric depth from the top of the atmosphere (in units of g/cm2). The minimum is 0.913 g/cm2, the maximum is 1032.66 g/cm2. WARNING: you can specify either altitude OR atmospheric depth, not both.
    • latitude required number: Latitude. -90 (S) to 90 (N).
    • longitude required number: Longitude. -180 (W) to 180 (E).
    • year required integer: Year in YYYY.
    • month required integer: Month in MM.
    • day required integer: Day in DD.
    • particle required string (values: total, e-, e+, mu+, mu-, gamma, neutron, proton, alpha): The particle type as a string. Specifying 'total', only used for the dose calculation, returns the dose for all particle types.
    • angle required number: Direction cosine. 1.0 is in the downward direction.

Output

  • output object
    • energies object
      • data array
        • items number
      • units string
    • intensities object
      • data array
        • items number
      • units string

app.api_parma.endpoints.PARMA.effective_dose

Effective dose is a radiation protection quantity defined by the International Commission on Radiological Protection (ICRP) and represents the stochastic health risk to the human body at low levels of radiation. It accounts for the different sensitivities of organs to ionising radiation, as well as the different effectiveness of various types of radiation. Use this endpoint if you need to estimate radiation exposures of personnel.

amentum_space_cosmic_ray.app.api_parma.endpoints.PARMA.effective_dose({
  "latitude": 0,
  "longitude": 0,
  "year": 0,
  "month": 0,
  "day": 0,
  "particle": ""
}, context)

Input

  • input object
    • altitude number: Altitude (in km). The minimum is 0 m, the maximum is 47 km (the upper limit of the stratosphere).
    • atmospheric_depth number: Atmospheric depth from the top of the atmosphere (in units of g/cm2). The minimum is 0.913 g/cm2, the maximum is 1032.66 g/cm2. WARNING: you can specify either altitude OR atmospheric depth, not both.
    • latitude required number: Latitude. -90 (S) to 90 (N).
    • longitude required number: Longitude. -180 (W) to 180 (E).
    • year required integer: Year in YYYY.
    • month required integer: Month in MM.
    • day required integer: Day in DD.
    • particle required string (values: total, e-, e+, mu+, mu-, gamma, neutron, proton, alpha): The particle type as a string. Specifying 'total', only used for the dose calculation, returns the dose for all particle types.

Output

  • output object
    • units string
    • value string

Definitions

This integration has no definitions