Cited by 36Planetary Science and ExplorationNuclear Physics and ApplicationsAstro and Planetary Science

Neutron background environment measured by the Mars Science Laboratory's Dynamic Albedo of Neutrons instrument during the first 100 sols

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Jun, I., Mitrofanov, I., Litvak, M. L., Sanin, A. B., Kim, W., Behar, A., Boynton, W. V., DeFlores, L. +15 more·2013·Journal of Geophysical Research: Planets

Abstract

The Dynamic Albedo of Neutrons (DAN) instrument on board Mars Science Laboratory has been operating successfully since the landing and has been making measurements regularly along Curiosity's traverse at the surface. DAN measures thermal (E < 0.4 eV) and epithermal neutrons (0.4 eV < E < ~1 keV) while operating in two different modes: active and passive. The active mode uses a pulsed neutron generator (PNG) to study the geological characteristics of the subsurface. In the passive mode, DAN measures the background neutron environment. This paper presents results of measurements in the passive mode from landing through to sol 100 and provides an interpretation of the data based on extensive Monte Carlo simulations. The main observations are summarized as follows: (1) the thermal neutron counts vary strongly along the rover traverse while the epithermal counts do not show much variation; (2) the neutrons from the Multi‐Mission Radioisotope Thermoelectric Generator (MMRTG) are a larger contributor to the DAN passive data than the Galactic Cosmic Ray (GCR)‐induced neutrons; (3) for the MMRTG neutrons, both the thermal and the epithermal counts increase as a function of the subsurface water content; (4) on the other hand, for the GCR‐induced neutrons, the thermal counts increase but the epithermal counts decrease as a function of the subsurface water content; and (5) relative contributions by the MMRTG and GCR to the DAN thermal neutron counts at the Rocknest site, where the rover was stationed from sol 59 to sol 100, are estimated to be ~60% and ~40%, respectively.

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Authors
Jun, I., Mitrofanov, I., Litvak, M. L., Sanin, A. B., Kim, W., Behar, A., Boynton, W. V., DeFlores, L., Fedosov, F., Golovin, D., Hardgrove, C., Harshman, K., Kozyrev, A. S., Kuzmin, R. O., Malakhov, A., Mischna, M., Moersch, J., Mokrousov, M., Nikiforov, S., Shvetsov, V. N., Tate, C., Tret'yakov, V. I., & Vostrukhin, A.
Affiliations
  • Jet Propulsion Laboratory (US)
  • Space Research Institute (RU)
  • University of Arizona (US)
  • University of Tennessee at Knoxville (US)
  • Space Research Institute, RAS Moscow Russia
  • Joint Institute for Nuclear Research (RU)
Corresponding author
Jun, I.
Venue
Journal of Geophysical Research: Planets
Published
2013-11
Volume
118
Issue
11
Pages
2400-2412
ISSN
  • 2169-9097 (ISSN-L)
  • 2169-9100
OpenAlex
W1562842457
Cited by
36
References
0
Citations by year
2026: 3 · 2025: 3 · 2024: 2 · 2023: 1 · 2022: 3 · 2020: 6 · 2019: 3 · 2018: 7 · 2017: 2 · 2016: 1 · 2015: 2 · 2014: 2 · 2013: 1
FWCI
1.08
Type
journal article
Language
en
Open access
Locations
Journal of Geophysical Research Planets (publishedVersion)
Funders
  • National Aeronautics and Space Administration
  • California Institute of Technology
  • Jet Propulsion Laboratory
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Physics and Astronomy › Radiation › Nuclear Physics and Applications
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
Keywords
Mars Science Laboratory, Curiosity rover, neutron background, thermal neutrons, epithermal neutrons, subsurface water content, Monte Carlo simulation, Rocknest, Mars surface

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