Models at 1 AU

On this page, the outputs from the statistical models can be viewed in more detail, in the form of For models based on proton spectra, an abundance scaling to five ion species can be performed as well.

Model selection

After selecting a previously run model, the page reloads to display further options: Once all mandatory selections have been made, the Run button can be pressed to generate the resuls.

Results

The format of the results depends on the statistical model type.

For time above threshold and event duration models, and for flux/fluence model based on a response function, the output is a series of curves of the model parameter as a function of mission length, for each confidence level. The results are presented as an on-screen table, a data file and a plot.

For flux and fluence models, the outputs consist of a series of particle spectra as a function of energy. The spectra are grouped by confidence level and mission length. The results are presented as an on-screen table, a data file and a series of plots (one per confidence level).

For flux and fluence models based on proton spectra, the original probability curves (at lower resolution) are reproduced after abundance scaling to the selected ion species.




Last modified on: 30 September 2011.