Cited by 35Radiation Therapy and DosimetryPlanetary Science and ExplorationAstrophysics and Cosmic Phenomena

Description of light ion production cross sections and fluxes on the Mars surface using the QMSFRG model

Cucinotta, Francis A., Kim, Myung-Hee, Schneider, Susana I., Hassler, Donald M.·2007·Radiation and Environmental Biophysics

Abstract

The atmosphere of Mars significantly attenuates the heavy ion component of the primary galactic cosmic rays (GCR), however, increases the fluence of secondary light ions (neutrons, and hydrogen and helium isotopes) because of particle production processes. We describe results of the quantum multiple scattering fragmentation (QMSFRG) model for the production of light nuclei through the distinct mechanisms of nuclear abrasion and ablation, coalescence, and cluster knockout. The QMSFRG model is shown to be in excellent agreement with available experimental data for nuclear fragmentation cross sections. We use the QMSFRG model and the space radiation transport code, HZETRN to make predictions of the light particle environment on the Martian surface at solar minimum and near maximum. The radiation assessment detector (RAD) experiment will be launched in 2009 as part of the Mars Science Laboratory (MSL). We make predictions of the expected results for time dependent count-rates to be observed by the RAD experiment. Finally, we consider sensitivity assessments of the impact of the Martian atmospheric composition on particle fluxes at the surface.

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  1. [9]9. Cucinotta F A, et al (1997) Computational procedures and data-base development. In: NASA Workshop on Shielding Strategies for Human Space Exploration. Eds. Wilson JW, Miller J, Konradi A, and Cucinotta FA. NASA CP-3360.
  2. [16]16. Cucinotta F A, Wilson J W, Saganti P, Hu X, Kim M Y, Cleghorn T, Zeitlin C, and Tripathi R K (2006) Isotopic dependence of GCR fluence behind shielding. Rad Measurements (in press).
  3. [17]17. Zeitlin C, Fukumura A, Guetersloh S B, Heilbronn L H, Iwata Y, Miller J, and Murakami T (2006) Fragmentation cross sections of 28 Si at beam energies from 290 A to 1200 A MeV. Nucl Phys A (in Press).

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Authors
Cucinotta, F. A., Kim, M.-H., Schneider, S. I., & Hassler, D. M.
Affiliations
  • National Aeronautics and Space Administration (US)
  • Pennsylvania State University (US)
  • Southwest Research Institute (US)
Corresponding author
Cucinotta, Francis A.
Venue
Radiation and Environmental Biophysics
Published
2007-03-07
Volume
46
Issue
2
Pages
101-106
ISSN
  • 0301-634X (ISSN-L)
  • 1432-2099
OpenAlex
W2013459365
Cited by
35
References
2
Citations by year
2026: 3 · 2025: 1 · 2024: 1 · 2023: 2 · 2022: 2 · 2020: 3 · 2019: 1 · 2015: 2 · 2014: 3 · 2013: 4 · 2012: 5
FWCI
1.72
Type
journal article
Language
en
Open access
closed
Locations
  • Radiation and Environmental Biophysics (publishedVersion)
  • PubMed (publishedVersion)
  • NASA STI Repository (National Aeronautics and Space Administration) (submittedVersion)
Topics
  • Health Sciences › Medicine › Pulmonary and Respiratory Medicine › Radiation Therapy and Dosimetry
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Astrophysics and Cosmic Phenomena
Keywords
nuclear fragmentation cross sections, galactic cosmic rays, neutron production, coalescence, HZETRN, Radiation Assessment Detector, Mars Science Laboratory, solar cycle dependence, radiation shielding
MeSH terms
Computer Simulation, Cosmic Radiation, Environmental Exposure, Extraterrestrial Environment, Ions, Models, Theoretical, Radiation Dosage, Radiation Monitoring, Risk Factors, Space Flight, Mars, Risk Assessment

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