Reference42 articles.
1. Anders, E. and Grevesse, N.: 1989, ‘Abundances of the elements: meteoritic and solar’, Geochim. Cosmochim. Acta 53, 197.
2. Becker, R. H., Schlutter, D. J., Rider, P.E., and Pepin, R. O.: 1998, ‘An acid-etch study of the Kapoeta achondrite: Implications for the argon-36/argon-38 ratio in the solar wind’, Meteoritics Planet. Sci. 33, 109.
3. Benkert, J.-P., Baur, H., Signer, P., and Wieler, R.: 1993, ‘He, Ne, and Ar from the solar wind and solar energetic particles in lunar ilmenites and pyroxenes’, J. Geophys. Res. (Planets) 98, 13147.
4. Black, D. C: 1972, ‘On the origins of trapped helium, neon and argon isotopic variations in meteorites-I. Gas-rich meteorites, lunar soil and breccia’, Geochim. Cosmochim. Acta 36, 347.
5. Bochsler, P.: 1984, ‘Helium and oxygen in the solar wind: dynamic properties and abundances of elements and helium isotopes as observed with the ISEE-3 plasma composition experiment’, Habilitation Thesis, Univ. of Bern.
Cited by
3 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Composition Aspects of the Upper Solar Atmosphere;Solar Composition and its Evolution — from Core to Corona;1998
2. Solar Energetic Particle Isotopic Composition;Solar Composition and its Evolution — from Core to Corona;1998
3. Constraints on the FIP Mechanisms from Solar Wind Abundance Data;Solar Composition and its Evolution — from Core to Corona;1998