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Lyman series vacuum

Two measurements [31,10] were conducted at a low-inductance vacuum spark plasma and a tokamak plasma respectively. In both cases only the w line was reported. The first study used a double Johann spectrograph and characteristic K lines were used for calibration [31]. The energy of the w was 5.20558(55) keV or a 105 ppm result The second study [10] used a tokamak plasma and claimed an uncertainty of 40 ppm. Close lying Lyman series lines were used for calibration so this was a relative measurement chain assuming one-electron QED. Shorter wavelength calibration lines and helium-like resonances were observed in second order diffraction suggesting the significant systematic shifts discussed above. The third study [11] was a relative measurement to the w line and, as such, can not be compared to absolute measurements. [Pg.710]

Representative emission spectra are shown schematically in Fig. 2.2 for hydrogen, potassium, and mercury on a common wavelength scale from the near infrared to the ultraviolet. Under the coarse wavelength resolution of this figure, the emitted light intensities are concentrated at single, well-defined emission lines. In H, the displayed emission consists of four convergent series of lines, the so-called Ritz-Paschen and Pfund series in the near infrared, the Lyman series in the vacuum ultraviolet, and the Balmer series in the visible. Johann Balmer, a schoolteacher in Basel in the late nineteenth century. [Pg.34]

Very accurate high-resolution vacuum-UV data with an error of 0.000 1A for the Lyman series of the line spectrum of the hydrogen atom are reported in [8]. This error, translated into wave numbers, constitutes an error of about 0.01 cm in the wave numbers around 100,000 cm ... [Pg.59]

Figure 2.4 Hydrogen atom energy levels and transitions. The Lyman, Balmer, Ritz-Paschen, and Brackett series occur in the vacuum ultraviolet, visible, near-infrared, and infrared regions of the electromagnetic spectrum, respectively. Figure 2.4 Hydrogen atom energy levels and transitions. The Lyman, Balmer, Ritz-Paschen, and Brackett series occur in the vacuum ultraviolet, visible, near-infrared, and infrared regions of the electromagnetic spectrum, respectively.
Fig. 2 The plot of Eq. (5) for the Lyman vacuum-UV series of the hydrogen atom for which the quantum number of the final state is n = 1. See discussion in the text. The data are from Sansonetti [8]... Fig. 2 The plot of Eq. (5) for the Lyman vacuum-UV series of the hydrogen atom for which the quantum number of the final state is n = 1. See discussion in the text. The data are from Sansonetti [8]...
The atomic line-spectral data for the Lyman vacuum-UV series of the hydrogen atom are given in Table 1. The plot of the line wave number vs 1/nf-, following Eqs. (7) and (8), is displayed in Fig. 2. The least-squares fitting is excellent, with = 1.000 and ct = 0.41 cm . The values obtained for the constant of proportionality from the least-squares fitting are ... [Pg.59]


See other pages where Lyman series vacuum is mentioned: [Pg.161]    [Pg.57]    [Pg.97]   
See also in sourсe #XX -- [ Pg.54 , Pg.59 ]




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