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Titlebook: Advances in Helio- and Asteroseismology; Proceedings of the 1 J?rgen Christensen-Dalsgaard,S?ren Frandsen Conference proceedings 1988 Inter

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發(fā)表于 2025-3-21 17:48:21 | 只看該作者 |倒序瀏覽 |閱讀模式
期刊全稱Advances in Helio- and Asteroseismology
期刊簡稱Proceedings of the 1
影響因子2023J?rgen Christensen-Dalsgaard,S?ren Frandsen
視頻videohttp://file.papertrans.cn/149/148186/148186.mp4
學(xué)科分類International Astronomical Union Symposia
圖書封面Titlebook: Advances in Helio- and Asteroseismology; Proceedings of the 1 J?rgen Christensen-Dalsgaard,S?ren Frandsen Conference proceedings 1988 Inter
影響因子Helio- and asteroseismology study the interior of the Sun and other stars, by means of observations of oscillations on their surfaces. The last 10 years in the study of the solar interior, to a has witnessed a very rapid evolution point where we can now contemplate investigating the physical state of matter, or the details of rotation and other large-scale motion, in the Sun. The stellar studies are in some respects at the point of the solar studies 10 years ago, but appear poised to take off. Thus the time was deemed ripe for lAO Symposium No 123, to assess the present status of this work, and plan for its future development. Apart from the seismic data, few observations are available to provide information about stellar interiors. Detailed studies, by spectral analysis, can be made of stellar surface properties, including atmospheric temperature and chemical composition. However, the stellar radiative spectrum is almost entirely fixed by the mass, luminosity, radius and surface rotation of the star, and contains essentially no other information about the interior. An important test of stellar evolution theory is provided by observations of stel- lar clusters, whose members can re
Pindex Conference proceedings 1988
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The Basic Questions on Danxia Landformected for analysis. That makes a duty cycle of about 45H, which itself makes of this season a reasonably good one. A complete week of extremely good sky was missed, we could almost say as usually, as the beginning of the season before we could be ready.
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The Basic Questions on Danxia Landform continuity of the observed signal at 160.01 minutes. We find that the previously reported phase stability is no longer present. However, due to uncertainties in calibration we can not exclude the reality of the reported signal.
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The Basic Questions on Danxia Landformurves obtained from data sets of single days. The results imply that the solar rotation rate increases with depth by 0.023 /.Hz reaching a maximum at about 2 Mm below the surface, then decreases by 0.037 /.Hz down to 16 Mm.
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Conference proceedings 1988rs in the study of the solar interior, to a has witnessed a very rapid evolution point where we can now contemplate investigating the physical state of matter, or the details of rotation and other large-scale motion, in the Sun. The stellar studies are in some respects at the point of the solar stud
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Measurements of Solar Internal Rotation Obtained with the Mt. Wilson 60-Foot Solar Tower978-1-4842-1560-9
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