A Non-Solar Origin of the "SEP" Component in Lunar Soils?

COSPAR Colloquia Series

Volumn 11, Issue C, 2001, Pages 507-510

  Wimmer Schweingruber, R F ^b   Bochsler, P ^a  

^a UNIVERSITY OF BERN   (Switzerland)

^b NONE

Author keywords

[No Author keywords available]

Indexed keywords

EID: 77957055667     PISSN: 09642749     EISSN: None     Source Type: Book Series    
DOI: 10.1016/S0964-2749(01)80117-7     Document Type: Chapter

References (12)

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2. Bochsler P. Abundances and charge states of particles in the solar wind. Rev. Geo phys. 38 (2000) 247-266
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8. Skumanich A. Timescales for Ca II emission decay, rotational breaking, and Li depletion. Astrophys. J. 171 (1972) 565-567
9. Soderblom D.R., Duncan D.K., and Johnson D.R.H. The chromospheric emission- age relation for stars of the lower main sequence and its implications for the star forming rate. Astrophys. J. 375 (1991) 722-739
10. Wieler R., Baur H., and Signer P. Noble gases from solar energetic particles revealed by closed system stepwise etching of lunar soil material. Geochim. et Cosmoschim. Acta 50 (1986) 1997-2017
11. Wimmer-Schweingruber R.F. Lunar soils: A long-tern archive for the galactic environment of the solar system?. Habilitation Thesis (2000), Physikalisches Institut, Universität Bern
12. AIP conference proceedings. Wimmer-Schweingruber R.F., and Bochsler P. Is there a record of interstellar pick-up ions in the lunar regolith?. In: Mewaldt R.A., Jokipii J.R., Lee M.A., Moebius E., and Zurbuchen T.H. (Eds). Acceleration and Transport of Energetic Particles Observed in the Heliosphere (2000) 270-273