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Papers by Pier Giorgio Rancoita
Our back-tracing code (GeoMagSphere) reconstructs the cosmic ray trajectories inside the Earth’s ... more Our back-tracing code (GeoMagSphere) reconstructs the cosmic ray trajectories inside the Earth’s magnetosphere. GeoMagSphere gets the incoming directions of particles entering the magnetopause and disentangles primary from secondary particles (produced in atmosphere) or even particles trapped inside the Earth’s magnetic field. The separation of these particle families allows us to evaluate the geomagnetic rigidity cutoff. The model can be used considering the internal symmetric (IGRF-12) magnetic field only, or adding the asymmetric external one (Tsyganenko models: T89, T96 or TS05). A quantitative comparison among these models is presented for quiet (solar pressure Pdy n < 4 nPa) and disturbed (Pdy n > 4 nPa) periods of solar activity, as well as during solar events like flares, CMEs. In this analysis we focused our attention on magnetic field data in magnetosphere, from Cluster, and simulated cosmic rays for a generic detector on the ISS as for example AMS-02. We found that ...
Nuclear Physics B - Proceedings Supplements, 1999
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, 1995
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1994
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1988
Principles of Radiation Interaction in Matter and Detection, 2011
Principles of Radiation Interaction in Matter and Detection, 2009
Advances in Space Research, 2021
Abstract Evaluation of cosmic ray trajectories and penetration inside the Earth environment is ma... more Abstract Evaluation of cosmic ray trajectories and penetration inside the Earth environment is mandatory for estimation of flux by on-orbit detectors as well as of radiation damage on electronics devices and biological tissues, like those of astronauts onboard the International Space Station. We studied the impact of the external magnetic field on the calculation of some parameters like the rigidity cut-off, by a quantitative comparison among several geomagnetic field models. For this purpose we used GeoMagSphere back-tracing code, performing the particle trajectory reconstruction back-in-time from the chosen position and time up to the borders of the magnetosphere. The analysis done points out the need to combine an external magnetic field model with the internal one (usually IGRF). Several external field models have a different impact on the accuracy as well as on the time needed for calculation, important in case of a large amount of back-traced particles. We also studied cosmic ray propagation inside the magnetosphere, separately for quiet and disturbed solar activity periods. We found that during highly disturbed periods and during magnetic storms, rigidity cut-off, as well as cosmic ray flux, can be appropriately evaluated only by using external field models, like that one proposed by Tsyganenko and Sitnov (2005), well describing those particular conditions.
... FERRI, GIOVANNI FRANZONI, ALESSIO GHEZZI, PIETRO GOVONI, PIETRO NEGRI, MARCO PAGANONI, ANTONI... more ... FERRI, GIOVANNI FRANZONI, ALESSIO GHEZZI, PIETRO GOVONI, PIETRO NEGRI, MARCO PAGANONI, ANTONINO ... L. BRACCI, G. CALAMAI, E. CAMPAGNA, E. CUOCO, G. GUIDI, G. LOSURDO, F ... ANIMAL PET IMAGING MA MILLER, NC ROUZE and GD HUTCHINS, 381. ...
Cosmic Rays for Particle and Astroparticle Physics - Proceedings of the 12th ICATPP Conference ICATPP, 2011
IEEE Transactions on Nuclear Science, 1987
Our back-tracing code (GeoMagSphere) reconstructs the cosmic ray trajectories inside the Earth’s ... more Our back-tracing code (GeoMagSphere) reconstructs the cosmic ray trajectories inside the Earth’s magnetosphere. GeoMagSphere gets the incoming directions of particles entering the magnetopause and disentangles primary from secondary particles (produced in atmosphere) or even particles trapped inside the Earth’s magnetic field. The separation of these particle families allows us to evaluate the geomagnetic rigidity cutoff. The model can be used considering the internal symmetric (IGRF-12) magnetic field only, or adding the asymmetric external one (Tsyganenko models: T89, T96 or TS05). A quantitative comparison among these models is presented for quiet (solar pressure Pdy n < 4 nPa) and disturbed (Pdy n > 4 nPa) periods of solar activity, as well as during solar events like flares, CMEs. In this analysis we focused our attention on magnetic field data in magnetosphere, from Cluster, and simulated cosmic rays for a generic detector on the ISS as for example AMS-02. We found that ...
Nuclear Physics B - Proceedings Supplements, 1999
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, 1995
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1994
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1988
Principles of Radiation Interaction in Matter and Detection, 2011
Principles of Radiation Interaction in Matter and Detection, 2009
Advances in Space Research, 2021
Abstract Evaluation of cosmic ray trajectories and penetration inside the Earth environment is ma... more Abstract Evaluation of cosmic ray trajectories and penetration inside the Earth environment is mandatory for estimation of flux by on-orbit detectors as well as of radiation damage on electronics devices and biological tissues, like those of astronauts onboard the International Space Station. We studied the impact of the external magnetic field on the calculation of some parameters like the rigidity cut-off, by a quantitative comparison among several geomagnetic field models. For this purpose we used GeoMagSphere back-tracing code, performing the particle trajectory reconstruction back-in-time from the chosen position and time up to the borders of the magnetosphere. The analysis done points out the need to combine an external magnetic field model with the internal one (usually IGRF). Several external field models have a different impact on the accuracy as well as on the time needed for calculation, important in case of a large amount of back-traced particles. We also studied cosmic ray propagation inside the magnetosphere, separately for quiet and disturbed solar activity periods. We found that during highly disturbed periods and during magnetic storms, rigidity cut-off, as well as cosmic ray flux, can be appropriately evaluated only by using external field models, like that one proposed by Tsyganenko and Sitnov (2005), well describing those particular conditions.
... FERRI, GIOVANNI FRANZONI, ALESSIO GHEZZI, PIETRO GOVONI, PIETRO NEGRI, MARCO PAGANONI, ANTONI... more ... FERRI, GIOVANNI FRANZONI, ALESSIO GHEZZI, PIETRO GOVONI, PIETRO NEGRI, MARCO PAGANONI, ANTONINO ... L. BRACCI, G. CALAMAI, E. CAMPAGNA, E. CUOCO, G. GUIDI, G. LOSURDO, F ... ANIMAL PET IMAGING MA MILLER, NC ROUZE and GD HUTCHINS, 381. ...
Cosmic Rays for Particle and Astroparticle Physics - Proceedings of the 12th ICATPP Conference ICATPP, 2011
IEEE Transactions on Nuclear Science, 1987