The abundance of 3He in the solar wind - A constraint for models of solar evolution-Reference-Cited by-同舟云学术

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The abundance of 3He in the solar wind - A constraint for models of solar evolution

Published:1990-07 Issue:1 Volume:128 Page:203-215
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Bochsler P.,Geiss J.,Maeder A.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00154157.pdf

Reference39 articles.

1. Anders, E. and Grevesse, N.: 1989, Geochim. Cosmochim. Acta 53, 197.

2. Axford, I. W.: 1986, lecture presented at the University of Bern, September 4.

3. Bania, T. M., Rood, R. T., and Wilson, T. L.: 1987, Astrophys. J. 323, 30.

4. Becker, R. H. and Pepin, R. O.: 1989, Geochim. Cosmochim. Acta 53, 1135.

5. Benkert, J. P., Baur, H., Pedroni, A., Wieler, R., and Signer, P.: 1988, Lunar Planetary Sci. XIX, 59.

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