Articles | Volume 14, issue 3
https://doi.org/10.1007/s00585-996-0270-9
© European Geosciences Union 1996
https://doi.org/10.1007/s00585-996-0270-9
© European Geosciences Union 1996
31 Mar 1996
31 Mar 1996
An extended structure-function model and its application to the analysis of solar wind intermittency properties
C.-Y. Tu
E. Marsch
H. Rosenbauer
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34 citations as recorded by crossref.
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- EVIDENCE FOR NONLINEAR DEVELOPMENT OF MAGNETOHYDRODYNAMIC SCALE INTERMITTENCY IN THE INNER HELIOSPHERE A. Greco et al. 10.1088/0004-637X/749/2/105
- Tsallis non-extensive statistics and solar wind plasma complexity G. Pavlos et al. 10.1016/j.physa.2014.12.007
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- Magnetosheath Plasma Turbulence and Its Spatiotemporal Evolution as Observed by the Cluster Spacecraft E. Yordanova et al. 10.1103/PhysRevLett.100.205003
- Magnetic field strength distribution in interplanetary turbulence T. Hartlep et al. 10.1029/1999JA000223
- Influence of Intermittency on the Energy Transfer Rate of Solar Wind Turbulence H. Wu et al. 10.3847/2041-8213/ad0a68
- Radial evolution of solar wind intermittency in the inner heliosphere R. Bruno et al. 10.1029/2002JA009615
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- On the Variation of Intermittency of Fast and Slow Solar Wind With Radial Distance, Heliospheric Latitude, and Solar Cycle A. Wawrzaszek & M. Echim 10.3389/fspas.2020.617113
- Ulysses observations of intermittent heliospheric turbulence T. Horbury et al. 10.1016/S0273-1177(97)00290-1
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