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Turbulent eddy-time-correlation in the solar convective zone

  • Belkacem K
  • Samadi R
  • Goupil M
  • et al.
Astronomy & Astrophysics (2010) 522 L2
DOI: 10.1051/0004-6361/201015706
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Abstract

Ai . Precise abundance ratios are determined for 94 dwarf stars with 5200 < Teff < 6300K, −1.6 < −0.4, and distances Met D

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Belkacem, K., Samadi, R., Goupil, M. J., Baudin, F., Salabert, D., & Appourchaux, T. (2010). Turbulent eddy-time-correlation in the solar convective zone. Astronomy & Astrophysics, 522, L2. https://doi.org/10.1051/0004-6361/201015706

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