Input data that was used for this simulation.

Version: IGRF
Year: 2010
DOY: 283
Hour: 10
Latitude: 0
Longitude: 0
Radius: 1
Rigidity step: 0.01 GV
Number of directions simulated: 1
Optimization level: No optimization
Spectrum: Force field Usoskin JGR 2017

Spectra of allowed rigidities in selected directions.


rig_spectrum

Full asymptotic cone where intensity of incoming particles from different asymptotic direction is indicated by colors representing a part of the total registered intensity in percents. As spectrum at 1AU was used AMS-01 spectrum from region 10 (most poleward region, where influence of magnetosphere to cosmic rays was smallest).


proton_plot

proton_plot

proton_plot

proton_plot

Transmission function, denoted by black line, shows probability of particles from all directions with rigidity R to reach selected point inside magnetosphere.


transmission_function

Differential flux at the top of the atmosphere from vertically incoming trajectories (denoted by green color) and from multidirectional simulation(denoted by orange color). Spectrum ať the magnetopause is denoted by blue color.


proton_flux

Input data that was used for this simulation.

Version: IGRF
Year: 2010
DOY: 283
Hour: 10
Latitude: 0
Longitude: 0
Radius: 1
Rigidity step: 0.01 GV
Number of directions simulated: 1
Optimization level: No optimization
Spectrum: Force field Usoskin JGR 2017

Spectra of allowed rigidities in selected directions.


rig_spectrum

Full asymptotic cone where intensity of incoming particles from different asymptotic direction is indicated by colors representing a part of the total registered intensity in percents. As spectrum at 1AU was used AMS-01 spectrum from region 10 (most poleward region, where influence of magnetosphere to cosmic rays was smallest).


proton_plot

proton_plot

proton_plot

proton_plot

Transmission function, denoted by black line, shows probability of particles from all directions with rigidity R to reach selected point inside magnetosphere.


transmission_function

Differential flux at the top of the atmosphere from vertically incoming trajectories (denoted by green color) and from multidirectional simulation(denoted by orange color). Spectrum ať the magnetopause is denoted by blue color.


proton_flux

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