The energy spectrum selection for the mission based environment depends on which SPENVIS radiation model has run before. If the trapped radiation models or the Solar particle mission fluences models have run then the options are trapped particles and long-term solar particles respectively.
Next, the user then to give the number of incident particles he wants to simulate in the Monte-Carlo run. As the total time for the run is limited, this number should be chosen as small as possible but large enough to provide statistically meaningful results. As a guideline, users should first make a run with a limited number of incident particles. When the results seem to make sense, a new run with more particles can be made to improve the statistics.
Warning: The particle track visualisation will be disabled when the number of particle is greater than 100!
The type of incident particles can be selected with the menu electronpositronproton neutronalphaiongamma geantino. Only when selecting the ion option, additional inputs are required. These consist of:
Note that the type of incident particles is related to the environment selection and only electron and proton can be available when a mission based environment is chosen.
It is assumed that all of the particle spectra are "omnidirectional", or have been integrated over 4PI, i.e. there are no units for sr-1. The particle spectra can be either flux or fluence spectra. For this reason, the unit (s-1) is placed between brackets. The units for other terms depend on the angular distribution (see below).
As the spectra obtained from the trapped particle, the Solar proton models, and the user-defined spectrum consist of pointwise data, these can be interpolated for other energies using several interpolation methods. The methods available are: linearpower-law exponentialcubic spline.
The energy E is expressed in MeV, and the default values for A and B are 1.0 and 0.0 respectively. The minimum and the maximum energy range must also be specified (these values default to 0.0 MeV and 100.0 MeV).
In this case, the exponent alpha has to be defined by the user (the default value is -1.0). The constant A has the same function as the source strength parameter defined above. In this case, the minimum and maximum energy to be considered have to be defined as well (the default values being 1.0 MeV and 100.0 MeV respectively).
The exponent E0 has to be defined (the default value is 1.0 MeV). As in the previous case, the value of the constant A has the same function as the source strength parameter defined above. Again, the minimum and maximum energy to consider in the spectrum have to be given (the default values being 0.0 MeV and 100.0 MeV respectively).