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An Alternative Explanation for the Praunhofer Sun Lines

机译:普劳恩霍夫太阳行的另一种解释

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Since their observation by J. Fraunhofer, the dark lines in the Sun spectrum have been exploited as markers to calibrate the dispersion spectra produced by glass prisms. G. Kirch-hoff stressed their fundamental meaning by interpreting them as absorption lines typical of each chemical element in the gas state. He based on a thermodynamic principle established by himself, according to which cooler gases above both the Sun's and the Earth's surfaces strip many lines from the continuous Sun emission spectrum, as they can absorb the same wavelengths they can emit. In this paper we argue that, although Fraunhofer lines allow wavelength scale calibration, they can actually be interpreted as an interference pattern produced by collimated Sun light beams.
机译:自从J. Fraunhofer观察到它们以来,太阳光谱中的暗线已被用作标记物,以校准由玻璃棱镜产生的色散光谱。 G. Kirch-hoff通过将它们解释为气态中每种化学元素的典型吸收线来强调其基本含义。他基于自己建立的热力学原理,根据该原理,太阳和地球表面上方的较冷气体会从连续的太阳发射光谱中剥离许多条线,因为它们可以吸收与发射相同的波长。在本文中,我们认为,尽管Fraunhofer线允许进行波长刻度校准,但实际上可以将它们解释为由准直的太阳光束产生的干涉图样。

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