Input data that was used for this simulation.

Version: T96
Year: 1994
DOY: 59
Hour: 13
Latitude: 48.38
Longitude: 21.43
Radius: 1.01
Rigidity step: 0.01 GV
Number of directions simulated: 577
Runtime: 04:42:28.800
Optimization level: Basic optimization
Spectrum: Force field Usoskin JGR 2017

DST: -18 PDYN: 2.34 BY: 4.70 BZ: -0.30

Effective cutoff rigidity sky map evaluated from 576 directions. Incoming directions cover a full half sphere.


contour_plot

contour_plot_2

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. Green histogram displays transmission function for vertical incoming trajectories.


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: T96
Year: 1994
DOY: 59
Hour: 13
Latitude: 48.38
Longitude: 21.43
Radius: 1.01
Rigidity step: 0.01 GV
Number of directions simulated: 577
Runtime: 04:42:28.800
Optimization level: Basic optimization
Spectrum: Force field Usoskin JGR 2017

DST: -18 PDYN: 2.34 BY: 4.70 BZ: -0.30

Effective cutoff rigidity sky map evaluated from 576 directions. Incoming directions cover a full half sphere.


contour_plot

contour_plot_2

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. Green histogram displays transmission function for vertical incoming trajectories.


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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