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Anisotropy in fast and slow solar wind fluctuations

Dasso, Sergio Ricardo et al · IOP Publishing · 2005

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Using 5 years of spacecraft data from near Earth orbit, we investigate the correlation anisotropy of solar wind magnetohydrodynamic-scale fluctuations and show that the nature of the anisotropy differs in fast (>500 km/s) slow (<400 km/) streams. In particular, fast streams are relatively more dominated by fluctuations with wavevectors quasi-parallel to the local magnetic field, while slow streams, which appear to be more fully evolved turbulence, are more dominated by quasi-perpendicular fluctuation wavevectors. Fil: Dasso, Sergio Ricardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Milano, L. J.. University of Delaware; Estados Unidos

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APA 7

Dasso, S. R. E. A. (2005). Anisotropy in fast and slow solar wind fluctuations. http://hdl.handle.net/11336/21326

MLA

Dasso, Sergio Ricardo et al. "Anisotropy in fast and slow solar wind fluctuations." 2005. http://hdl.handle.net/11336/21326.

Chicago

Dasso, Sergio Ricardo et al. 2005. "Anisotropy in fast and slow solar wind fluctuations.". http://hdl.handle.net/11336/21326.

Harvard

Dasso, S. R. E. A. 2005, Anisotropy in fast and slow solar wind fluctuations, IOP Publishing, available at: http://hdl.handle.net/11336/21326 [Accessed 10 Aug. 2026].

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Title
Anisotropy in fast and slow solar wind fluctuations
Author / contributors
Dasso, Sergio Ricardo et al
Publisher
IOP Publishing
Publication year
2005
ISSN
0004-637X
ISSN
0004-637X
Language
English

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