Spacecraft.ParticleFlux(Variable, Variable, Variable, TimeSpan, Variable) Method

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Description

The ParticleFlux method uses the NASA AP-8 and AE-8 particle flux maps to calculate the omnidirectional flux of the specified particle type with the energy level specified by minimumEnergy. The AP/AE maps contain collected data of proton and electron fluxes in the Earth's radiation belt with energy ranges from 0.04 MeV to 7 MeV for electrons and from 0.1 MeV to 400 MeV for protons. See the help file for links to more detailed documentation on the AP/AE maps. The user has the option to specify epoch and longitude offsets to include in the flux calculation.

 

Timing Precision Mode

This page describes functionality in nanosecond timing precision mode.

Click here to see the documentation for this object in millisecond timing precision mode.

 

Method Signature

Spacecraft.ParticleFlux(

Variable minimumEnergy,


Variable particleType,


Variable solarActivity,


TimeSpan igrfEpochOffset,


Variable longitudeOffset)

 

 

Arguments

minimumEnergy


Description:

Minimum energy of particles contributing to the flux. Energy values for electrons range from 0.1 to 7.0 MeV; for protons from 0.1 to 400.0 MeV.

Units:

MeV

Valid Range:

minimumEnergy > 0

 

 

particleType


Description:

The type of particle for which flux will be computed.

Valid Values:

Value

Label

0

electrons

1

protons

 

 

 

solarActivity


Description:

The solar activity level of the flux model. The AP-8/AE-8 flux maps use the 1964 IGRF Magnetic Field model when modeling solar minimum, and the 1970 IGRF Magnetic Field model when modeling solar maximum.

Valid Values:

Value

Label

0

solar minimum

1

solar maximum

 

 

 

igrfEpochOffset


Description:

An offset added to the epoch of the IGRF Magnetic Field model, used to determine the epoch of the magnetic field. Generally this argument should be between 0 and 365, signifying the number of days after the base epoch of the Magnetic Field model.

 

The epoch of the IGRF Magnetic Field model, when modeling solar minimum, is Jan 01 1964 12:00:00.000.

The epoch of the IGRF Magnetic Field model, when modeling solar maximum, is Jan 01 1970 12:00:00.000.

Units:

day

 

 

longitudeOffset


Description:

An offset added to the Longitude of the Spacecraft when computing the local magnetic field strength; the Latitude and Altitude are held constant. A positive offset is applied in the West direction.

Units:

deg

 

 

 

Return Value

Type:

number

Units:

particles/(cm^2 s)

 

 

Returns the particle flux evaluated at the Spacecraft's Earth-relative position using the magnetic field model at the epoch of the flux model specified by particleType and solarActivity.

 

Syntax

myVariable1 = mySpacecraft1.ParticleFlux(myVariable2, myVariable3, myVariable4, myTimeSpan1, myVariable5);

 

 

See also

Spacecraft Object

Spacecraft.ParticleFlux

Spacecraft Propagation Guide

Coverage and Contact Analysis Guide