Development of scalable deconvolution methods for determining secondary target neutron yields from dual-thick-target cosmic-ray ion accelerator experiments

Hunter N. Ratliff, Natalie A. McGirl, Matthew R. Beach, Luis A. Castellanos, Martha S. Clowdsley, Lawrence H. Heilbronn, Chiara LaTessa, John W. Norbury, Adam Rusek, Michael Sivertz, Ashwin P. Srikrishna, Hui Chen Wang, Cary Zeitlin

Research output: Contribution to journalArticlepeer-review

Abstract

Experiments emulating the deep-space radiation environment within an enclosed spacecraft were conducted at the NASA Space Radiation Laboratory; this was achieved by bombarding various combinations of two consecutive thick targets with Galactic Cosmic Ray-like particle beams. While all secondary particles generated in the first of these two targets could be characterized using time-of-flight techniques, characterization of the neutrons produced in the second target, emulating the “back wall” of a spacecraft, required the development and implementation of deconvolution techniques. This work covers this methodology, its validation, and the systematic results present within this benchmark dataset of neutron yields from the secondary target.

Original languageEnglish
Article number165121
JournalNuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms
Volume544
DOIs
StatePublished - Nov 2023
Externally publishedYes

Funding

This work was supported by NASA, United States grants NNX17AL10A , NNX15AD89A , and 80NSSC19M0101 and was supported at the NASA Johnson Space Center by the NASA Human Health and Performance Contract , NNJ15HK11B . Additionally, the authors Ratliff and McGirl were supported by The University of Tennessee Chancellor’s Distinguished Graduate Fellowship .

Keywords

  • Benchmark
  • Deconvolution
  • Neutron
  • Shielding
  • Space radiation
  • Tikhonov regularization

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