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Title: Solar-flare-implanted [sup 4]He/[sup 3]He and solar-proton-produced Ne and Ar concentration profiles preserved in lunar rock 61016

Journal Article · · Journal of Geophysical Research; (United States)
DOI:https://doi.org/10.1029/93JA00002· OSTI ID:6427162
 [1];  [2];  [3];  [4]
  1. Lunar Planetary Inst., Houston, TX (United States)
  2. Lockheed Engineering and Sciences Co., Houston, TX (United States) NASA, Houston, TX (United States)
  3. NASA, Houston, TX (United States)
  4. Los Alamos National Lab., NM (United States)

The authors report on isotopic measurements made on lunar rock 61016, which is one of the limited number with a known orientation history. They measure solar flare implanted [sup 4]He/[sup 3]He ratios and the depth profiles of [sup 21]Ne, [sup 22]Ne, and [sup 38]Ar isotopes produced from in situ nuclear reactions of solar flare protons with the silicate rock. They are able to distinguish solar flare from galactic cosmic ray sources of these isotopes. They find that the helium isotope ratios are energy dependent, reporting measurements for solar wind nuclei, with energies down to keV amu[sup [minus]1], and for solar flare nuclei with energies above 1 and 4 MeV amu[sup [minus]1]. Respective ratios are 2695[-+]81, 3450[-+]725, and 770[-+]316.

OSTI ID:
6427162
Journal Information:
Journal of Geophysical Research; (United States), Vol. 98:A5; ISSN 0148-0227
Country of Publication:
United States
Language:
English