Ruiz, M. E., Dasso, S. R., Matthaeus, W. H., & Weygand, J. M. (2014). Characterization of the turbulent magnetic integral length in the solar wind: From 0.3 to 5 astronomical units. Web
Citación estilo ChicagoRuiz, Maria Emilia, Sergio Ricardo Dasso, W. H. Matthaeus, and J. M. Weygand. Characterization of the Turbulent Magnetic Integral Length in the Solar Wind: From 0.3 to 5 Astronomical Units. 2014.
Cita MLARuiz, Maria Emilia, Sergio Ricardo Dasso, W. H. Matthaeus, and J. M. Weygand. Characterization of the Turbulent Magnetic Integral Length in the Solar Wind: From 0.3 to 5 Astronomical Units. 2014.
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