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Galactic HZE propagation through the Earth's atmosphere
J W Wilson1, L W Townsend, F F Badavi
1NASA Langley Research Center, Hampton, Virginia 23665, USA.
Radiation Research
|January 1, 1987
Summary
A new physical model simulates galactic heavy ion propagation, simplifying nuclear fragmentation for key processes. Comparisons with atmospheric ion measurements highlight the model's current limitations.
Area of Science:
- Astrophysics and Space Science
- Nuclear Physics
- Atmospheric Physics
Background:
- Galactic cosmic rays, including heavy ions, interact with Earth's atmosphere.
- Understanding heavy ion propagation is crucial for space radiation protection and atmospheric studies.
Purpose of the Study:
- To present a comprehensive physical model for galactic heavy ion propagation.
- To incorporate major nuclear fragmentation processes relevant to galactic ions.
- To compare model predictions with atmospheric ion fluence measurements.
Main Methods:
- Development of a simplified physical model for nuclear fragmentation.
- Simulation of galactic heavy ion propagation through the atmosphere.
- Analysis of atmospheric ion fluence data.
Main Results:
- The presented model accounts for significant nuclear fragmentation processes.
- Comparisons between the model and atmospheric ion measurements were performed.
- Limitations encountered during the comparison analysis were identified.
Conclusions:
- The developed physical model provides a framework for studying galactic heavy ion propagation.
- Further refinement of the model is necessary to improve agreement with experimental data.
- The study underscores the complexities of modeling ion interactions in the atmosphere.