We report results of Reynolds-number measurements, based on multi-point temperature measurements and the elliptic approximation (EA) of He and Zhang (2006 Phys. Rev. E 73 055303), Zhao and He (2009 Phys. Rev. E 79 046316) for turbulent Rayleigh-Bénard convection (RBC) over the Rayleigh-number range Ra 10 2 1 0 11 14≲ ≲ × and for a Prandtl number Pr ≃ 0.8. The sample was a right-circular cylinder with the diameter D and the height L both equal to 112 cm. The Reynolds numbers Re U and Re V were obtained from the mean-flow velocity U and the root-mean-square fluctuation velocity V, respectively. Both were measured approximately at the mid-height of the sample and near (but not too near) the side wall close to a maximum of Re U . A detailed examination, based on several experimental tests, of the applicability of the EA to turbulent RBC in our parameter range is provided. The main contribution to Re U came from a large-scale circulation in the form of a single convection roll with the preferred azimuthal orientation of its down flow nearly coinciding with the location of the measurement probes. First we measured time sequences of Re U (t) and Re V (t) from short (10 s) segments which moved along much longer sequences of many hours. The corresponding probability distributions of Re U (t) and Re V (t) had single peaks and thus did not reveal significant flow reversals. The two averaged Reynolds numbers determined from the entire data sequences were of comparable size. For Ra Ra 2 10 V 0.50 0.02 ∼ ± , consistent with the prediction for = 〈 − 〉 . This was accomplished by using the elliptic approximation (EA) of He and Zhang [1, 2] which permits the determination of the velocities from velocity space-time correlation functions. The EA is based on a second-order Taylor-series expansion of correlation functions which is valid near the origin of the space-time plane. However, He and Zhang postulated that the validity of the EA extends throughout the inertial range of length and time because of flow self-similarity. Analogous derivations and self-similarity assumptions can be applied to a passive scalar, for instance to the temperature in the bulk of turbulent RBC (see [35] and references therein), and thus we were able to make velocity determinations from measurements of the temperature space-time correlation functions. This procedure was used before for smaller Ra and various Pr on several occasions [29,[36][37][38][39].In the present paper, after a description of the apparatus and some measurement procedures in section 2, we first discuss in section 3 measurements of the LSC circulation-plane orientation because this orientation influences U. Then, in section 4, we discuss relevant consequences of the EA. While many of these results have appeared already in the literature, they are scattered among several papers and not always easy to find. Our discussion also includes a derivation of the equivalence between the space and the time domain, which remains valid in the presence of fluctuations and replaces the Taylor frozen-fl...