OBSERVATION OF FREE OSCILLATIONS OF SUN

OBSERVATION OF FREE OSCILLATIONS OF SUN
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DOI:
10.1038/259092a0
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发表时间:
1976-01-01
期刊:
影响因子:
64.8
通讯作者:
VANDERRAAY, HB
VANDERRAAY, HB
中科院分区:
综合性期刊1区
文献类型:
--
作者:
BROOKES, JR;ISAAK, GR;VANDERRAAY, HB

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利用共振光散射方法,将太阳上钾和钠的夫琅和费吸收线与实验室中相应的吸收线进行了比较。观测到的太阳和实验室谱线之间的位移可以用引力红移(GRS)、实验室相对于太阳的运动和可能与太阳振荡有关的振荡项来解释。
The Fraunhofer absorption lines for potassium and sodium on the Sun are compared with the corresponding lines in the laboratory using a resonant optical scattering method. The observed shifts between the Sun and laboratory lines may be interpreted in terms of the gravitational redshift (GRS), motion of the laboratory relative to the Sun and oscillatory terms which may be related to oscillations of the Sun.