The input parameters and options for the models are described below. When the input form has been completed, pressing the button will start the calculation and bring up the "Results" page.
First, the user can specify the IGRF epoch. The next input is the particle type: H He Li Be B C N O F Ne Na Mg Al Si P S Cl Ar K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr Rb Sr Y Zr Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe Cs Ba La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po At Rn Fr Ra Ac Th Pa U . The user has also the possibility to provide the energy of the particle in units of [MeV/nucleon] and its charge state singly ionized +2 ... fully ionized Note that the charge state options are adapted according to the particle type selection.
Finally, for the geomagnetic shielding the user can select between a quiet and a stormy magnetosphere.
When a single geographical point grid is used, the IGRF epoch becomes a variable parameter. Then, the user must provide in addition the last value for IGRF epoch and specify the step or the number of IGRF epoch values.
The report file spenvis_cop.html contains the input parameters. The spenvis_coo.txt file contains the transmission factor for each grid point.
spenvis_cop.html
spenvis_coo.txt
To generate plots, select the plot type(s), options and graphics format, and click the or button. The current page will be updated with the newly generated plot files.