SOLAR MODELS WITH STRONG TURBULENCE

CIVELEK R., KIZILOGLU N.

ASTROPHYSICS AND SPACE SCIENCE, cilt.202, sa.1, ss.77-80, 1993 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 202 Sayı: 1
  • Basım Tarihi: 1993
  • Doi Numarası: 10.1007/bf00626918
  • Dergi Adı: ASTROPHYSICS AND SPACE SCIENCE
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.77-80
  • Orta Doğu Teknik Üniversitesi Adresli: Hayır

Özet

A series of evolutionary models for the Sun were constructed using the strong turbulence model of the variable mixing-length theory (AMLT) of Canuto (1990). The present values of the solar model were obtained by an initial composition X = 0.754, Z = 0.019, and alpha(x) = 1.1. The physical variables which were obtained by applying the strong turbulence case of AMLT were similar to those of weak turbulence model (Kiziloglu and Civelek, 1992) if we focused on the fitting of present solar radius and luminosity.