Irradiation records in regolith materials, II: Solar wind and solar energetic particle components in helium, neon, and argon extracted from single lunar mineral grains and from the Kapoeta howardite by stepwise pulse heating

Geochimica et Cosmochimica Acta

Volumn 66, Issue 16, 2002, Pages 2929-2958

  Palma, R L ^a,b   Becker, R H ^a   Pepin, R O ^a   Schlutter, D J ^a  

^a University of Minnesota ^*  (United States)

^b SAM HOUSTON STATE UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

HOWARDITE; LUNAR SOIL; REGOLITH; SOLAR RADIATION; SOLAR WIND;

EID: 0036692421     PISSN: 00167037     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0016-7037(02)00853-0     Document Type: Article

References (44)

1. Monte Carlo simulation of turnover processes in the lunar regolith
2. Composition of solar wind noble gases released by surface oxidation of a metal separate from the Weston meteorite
3. An acid-etch study of the Kapoeta achondrite: Implications for the argon-36/argon-38 ratio in the solar wind
4. He, Ne, and Ar from the solar wind and solar energetic particles in lunar ilmenites and pyroxenes
5. On the origins of trapped helium, neon and argon isotopic variations in meteorites-I. Gas-rich meteorites, lunar soil and breccia
6. The isotopic composition of solar-flare noble gases
7. Elemental abundances in the solar wind
8. Solar wind radiation damage in lunar dust grains and the characteristics of the ancient solar wind
9. Primordial noble gases in "phase Q" in carbonaceous and ordinary chondrites studied by closed-system stepped etching
10. Speckle interferometry of asteroids
11. The simulated depth history of dust grains in the lunar regolith
12. Trapped solar wind noble gases in Apollo 12 lunar fines 12001 and Apollo 11 breccia 10046
13. Solar wind record in the lunar regolith: Nitrogen and noble gases
14. Composition, structure, and thermal history of metallic particles from 3 Apollo 16 soils, 65701, 68501, and 63501
15. Comparisons between observed and predicted cosmogenic noble gases in lunar samples
16. Isotopic composition of solar wind neon measured by CELIAS/MTOF on board SOHO
17. Radiometry and thermal modeling of asteroids
18. 4He in Jupiter's atmosphere
19. Noble gas abundance and isotope ratios in the atmosphere of Jupiter from the Galileo probe mass spectrometer
20. Lunar atmosphere as a source of lunar surface elements
21. Asteroids and comparative planetology
22. Precise measurement of asteroid sizes and shapes from occultations
23. Helium, neon, and argon abundances in the solar wind: In vacuo etching of meteoritic iron-nickel
24. High-performance double-focusing mass spectrometer
25. Helium and neon isotopes in stratospheric particles
26. Extraction of helium from individual interplanetary dust particles by step-heating
27. An experimental study of the isotopic enrichment in Ar, Kr, and Xe when trapped in water ice
28. A low-temperature origin for the planetesimals that formed Jupiter
29. Comparative studies of solar, Q-gases and terrestrial noble gases, and implications on the evolution of the solar nebula
30. On the origin and early evolution of terrestrial planet atmospheres and meteoritic volatiles
31. Isotopic evidence for a solar argon component in the Earth's mantle
32. Solar wind and spallation neon in small dark fragments separated from the Kapoeta howardite: Evidence for early GCR irradiation?
33. Irradiation records in regolith materials, I: Isotopic compositions of solar-wind neon and argon in single lunar regolith grains
34. 3He problem and estimates of the relative fluxes of solar wind and solar energetic particles in interplanetary space
35. Composition of solar flare noble gases preserved in meteorite parent body regolith
36. Energetic proton irradiation history of the howardite parent body regolith and implications for ancient solar activity
37. Asteroid magnitudes, UBV colors, and IRAS albedos and diameters
38. Passive microwave observations of asteroids
39. Petrographic esoterica in Kapoeta and their relevance to noble gas studies
40. 38Ar isotopic abundance ratio of the solar wind using SOHO/CELIAS/MTOF
41. Noble gases from solar energetic particles revealed by closed system stepwise etching of lunar soil minerals