Eulerian decorrelation of fluctuations in the interplanetary magnetic field
A method is devised for estimating the two-time correlation function and the associated Eulerian decorrelation timescale in turbulence.With the assumptions of a single decorrelation time and a frozen-in flow approximation for the single-point analysis, the method compares two-point correlation measu...
| Autores principales: | , , , , |
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
The American Astronomical Society
2010
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 06422caa a22008537a 4500 | ||
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| 001 | PAPER-7641 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230711124139.0 | ||
| 008 | 190410s2010 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-78649253956 | |
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| 100 | 1 | |a Matthaeus, W.H. |4 aut |e autor | |
| 245 | 1 | 0 | |a Eulerian decorrelation of fluctuations in the interplanetary magnetic field |
| 260 | |b The American Astronomical Society |c 2010 | ||
| 270 | 1 | 0 | |m Matthaeus, W. H.; Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, DE, United States |
| 506 | |2 openaire |e Política editorial |f info:eu-repo/semantics/openAccess | ||
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| 520 | 3 | |a A method is devised for estimating the two-time correlation function and the associated Eulerian decorrelation timescale in turbulence.With the assumptions of a single decorrelation time and a frozen-in flow approximation for the single-point analysis, the method compares two-point correlation measurements with single-point correlation measurements at the corresponding spatial lag. This method is applied to interplanetarymagnetic fieldmeasurements from the Advanced Composition Explorer and Wind spacecraft. An average Eulerian decorrelation time of 2.9 hr is found. This measures the total rate of distortion of turbulent fluid elements-including sweeping, nonlinear distortion, and wave propagation. © 2010. The American Astronomical Society. All rights reserved. |l eng | |
| 593 | |a Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, DE, United States | ||
| 593 | |a Instituto de Astronomía y Física Del Espacio (CONICET-UBA), Departamento de Física (FCEN-UBA), Buenos Aires, Argentina | ||
| 593 | |a Institute for Geophysics and Planetary Physics, University of California, Los Angeles, CA, United States | ||
| 690 | 1 | 0 | |a INTERPLANETARY MEDIUM |
| 690 | 1 | 0 | |a MAGNETIC FIELDS |
| 690 | 1 | 0 | |a SOLAR WIND |
| 690 | 1 | 0 | |a TURBULENCE |
| 700 | 1 | |a Dasso, S. |g ID autor FCEN: 2288 |9 2288 |4 aut |e autor | |
| 700 | 1 | |a Weygand, J.M. |4 aut |e autor | |
| 700 | 1 | |a Kivelson, M.G. |4 aut |e autor | |
| 700 | 1 | |a Osman, K.T. |4 aut |e autor | |
| 773 | 0 | |d Institute of Physics Publishing, 2010 |g v. 721 |h pp. L10-L13 |k n. 1 PART 2 |p Astrophys. J. Lett. |x 20418205 |t Astrophysical Journal Letters | |
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| 856 | 4 | 0 | |u https://doi.org/10.1088/2041-8205/721/1/L10 |x doi |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_20418205_v721_n1PART2_pL10_Matthaeus |x handle |y Handle |
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| 901 | |a PAPER |n 10 |q Margarita Zelaya | ||
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