| タイトル | The depth of the solar convection zone |
| 著者（英） | Christensen-Dalsgaard, J.; Gough, D. O.; Thompson, M. J. |
| 著者所属（英） | Aarhus Univ.|Institute of Astronomy|National Center for Atmospheric Research|Joint Inst. for Lab. Astrophysics |
| 発行日 | 1991-09-01 |
| 言語 | eng |
| 内容記述 | The transition of the temperature gradient between being subadiabatic and adiabatic at the base of the solar convection zone gives rise to a clear signature in the sound speed. Helioseismic measurements of the sound speed therefore permit a determination of the location of the base of the convection zone. Two techniques were tested by applying them to artifical data, obtained by adding simulated noise to frequencies computed from two different solar models. The determinations appear to be relatively insensitive to uncertainties of the physics of the solar interior. From an analysis of observed frequencies of solar oscillation it is concluded that the depth of the solar convection zone is (0.287 + or - 0.003) solar radii. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 91A50517 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/346018 |
