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Figure 7
Intensities of satellite reflections of NbSe3 as a function of temperature. Below T = 25 K the second-order satellite ([|m| = 2]; [2\delta_1]) is about 16× weaker than the first-order satellite ([|m| = 1]; [\delta_1]). Reprinted with permission from Moudden et al. (1993BB77). J. Phys. (Paris) IV, 3, C2, 121–124.

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ISSN: 2053-2733
Volume 61| Part 1| December 2005| Pages 51-61
doi:10.1107/S0108767304025437
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