Dedicated to Professor Dr. Erich Hückel on his 70th birthday
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- Referenz
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10a Frenkiel, F. N., Étude statistique de la turbulence. Fonctions spectrales et coefficients de correlation. Office National d'Études et des Recherches Aeronautiques (O. N.E.R.A.), Rapport Technique No. 34, 1948. English translation: Statistical study of turbulence - Spectral functions and correlation coefficients. National Advisory Committee for Aeronautics (NACA). Technical Memorandum 1436, Washington, D. C., July 1958.
10 Lumley, J. L., and H. A. Panofsky, The Structure of Atmospheric Turbulence, Interscience Publishers (New York) 1964 § 1.17.
11 Phillips, G. J., and M. Spencer, Proc. Phys. Soc. London B 68 (1955) 481 - 492, § 2.1.
12 Briggs, B. H., G. J. Phillips and D. H. Shinn, Proc. Phys. Soc. London B 63 (1950) 106 - 121, Eq. (6).
13 Ref. [11] § 2.2.
14 Ref. [12] Eq. (8).
15 Dougherty, J. P., Phil. Mag. (1960) 553 - 570, Eq. (6).
16 Ref. [12] Eq. (11).
17 Ref. [11] Fig. 7 (b).
18 Ref. [10] pp. 192/193.
19 Ref. [12] Eq. (15).
1 Booker, H. G., J. A. Ratcliffe and D. H. Shinn, Phil. Trans Roy. Soc. A 242 (1950) 579 - 609, § 5. (a).
20 Ref. [10] p. 193.
21 Ref. [12] pp. 193/194.
22 Ref. [12] § 4. (iii).
23 Gusev, V. D., and S. F. Mirkotan, URSI-CIG Inospheric Symposium, Nice (France), December 1961, Eq. (25).
24 Ref. [12] Eq. (14).
25 Ref. [11] § 2.2.
26 Ref. [11] § 3.1.
27 Ref. [23] end of § 3.
2 Hunger, K., and R. W. Larenz, Z. Physik 163 (1961) 245 - 261, § 5.
3 Montgomery, D. C. and D. A. Tidman, Plasma Kinetic Theory McGraw-Hill (New York) 1964, Sect. 8.
4 Ref. [3] § 14.2.
5 Ref. [3] § 15.2.
6 Ref. [1] § 4.
7 Ref. [1] § 5. (d).
8 Steenbeck, M., Monatsber. Deut. Akad. Wiss. 5 (1963) 625 - 629, Eqs. (2) and (5).
9 Taylor, G. I., Proc. Roy. Soc. London A 164 (1938) 476 - 490, Eq. (8).
- Seitenbereich
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0078 - 0096
- Zusammenfsg.
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With the coefficients of a Taylor expansion of the correlation function <I>C</I> (\documentclass{article}\pagestyle{empty}\begin{document}$ \overrightarrow \xi $\end{document}, τ) up to the second order in \documentclass{article}\pagestyle{empty}\begin{document}$ \overrightarrow \xi $\end{document}, τ three (or four) velocities can be defined to describe the space-time behaviour in a satisfying manner. They have a simple geometrical relationship among each other. The necessary measurements for the computation of these coefficients are discussed.
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