Data Provider Elements

SEET Radiation Accumulated Dose By Thickness

Computes the radiation dose as it accumulates over time for the requested time interval(s), using the step size to perform the numerical integration of dose rate with time. The report is divided into subsections, where each subsection corresponds to a different shielding thickness. Valid for vehicles whose central body is earth.

Available for these objects: LaunchVehicle, Missile, Satellite

Type: Time-varying data. Intended to be used only with elements from this same data provider.

Availability: Reports | Graphs

Data Provider Elements

NameDimensionTypeDescription
TimeDateReal Number or TextTime.
Electron doseRadiationDoseReal NumberThe accumulated radiation dose due to electrons for the shielding thickness indicated, at the given time. Valid when using NASA or CRRES models.
Electron-Bremsstrahlung doseRadiationDoseReal NumberThe accumulated radiation dose due to Bremsstrahlung electrons, at the given time. Valid when using NASA or CRRES models.
Proton doseRadiationDoseReal NumberThe accumulated radiation dose due to protons for the shielding thickness indicated, at the given time. Valid when using NASA or CRRES models.
Combined doseRadiationDoseReal NumberThe accumulated total radiation dose from all constituents, at the given time.
Mag field intensityMagneticFieldReal NumberThe magnitude of the magnetic field at the vehicle's location.
Dipole L-shell parameterUnitlessReal NumberThe L value for the field line passing through the vehicle's location computed using the dipole approximation to the magnetic field. For a dipole field line, the L value corresponds to the distance, measured in earth mean radii, at the point on the field line at the magnetic equator. (For a dipole field, this point is also the furthest extent of the field line from the earth.).
McIlwain L-shell parameterUnitlessReal Number or TextA measure that indicates a particle's drift shell in the magnetic field at the vehicle's location, as defined by Carl McIlwain (J. Geophys. Res. 1961). The value is computed as a function of several magnetic invariants along a field line and thus its computation requires field line tracing. It is not strictly a constant over the entire field line. In cases where the field line is close to the dipole field line (i.e., the field line traced using only the dipole component of the magnetic field model), the value will be close to the dipole L-shell parameter.
McIlwain Abs(L-shell) parameterUnitlessReal Number or TextThe absolute value of the McIlwain L-shell parameter.
B/BeqUnitlessReal Number or TextThe ratio of the magnetic intensity at the vehicle's location to the minimum magnetic intensity along the field line through the vehicle's location.
BeqMagneticFieldReal Number or TextThe minimum magnetic intensity along the field line through the vehicle's location. The minimum value occurs at the magnetic equator, at the furthest extent of the field line from the earth.
LatLatitudeReal Number or TextThe detic latitude (i.e., angle between the detic subpoint's surface normal vector and the XY plane.).
LonLongitudeReal Number or TextThe detic longitude (i.e., angle from the X-axis locating the projection of the detic subpoint's surface normal vector onto the XY plane.) Longitude increases in the direction found using the right-hand rule about the Z-axis.
AltDistanceReal NumberThe altitude value (i.e., magnitude of the relative position vector between the object and its detic subpoint).
15 day Avg ApUnitlessReal NumberThe average of the daily Ap value, over the previous 15 days. The Ap value is set according to the settings on the SEET radiation panel. When using a flux file to set Ap, the 15 day average is computed for each day and then the table of values is interpolated to determine the value at the given time.