Observations and measurements in the solar wind, the Jovian atmosphere and the gases trapped in lunar surface material provide the main evidence from which the isotopic composition of H, He and Ne in the Protosolar Cloud (PSC) is derived. These measurements and...
CITATION STYLE
Geiss, J., & Gloeckler, G. (2003). Isotopic Composition of H, He and Ne in the Protosolar Cloud (pp. 3–18). https://doi.org/10.1007/978-94-010-0145-8_1
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