Low-frequency Magnetic Field Fluctuations: Dependence of the Correlation Length on Upstream Parameters

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F09%3A00206475" target="_blank" >RIV/00216208:11320/09:00206475 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Low-frequency Magnetic Field Fluctuations: Dependence of the Correlation Length on Upstream Parameters
Original language description
The paper presents a statistical study of magnetic field fluctuations observed by the Cluster spacecraft near the dusk/dawn meridian at the magnetosheath in the vicinity of the magnetopause. We have found that the correlation length of such fluctuationsdepends on the solar wind speed, distance to the magnetopause and amplitude of magnetic field magnitude fluctuations. The fluctuations with anticorrelation between density and magnetic field fluctuations (for separations up to 1 RE) have shorter correlation lengths. The slopes of FFT spectra of magnetic field magnitude fluctuations decrease with larger solar wind speed and larger distance to the magnetopause
Czech name
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Czech description
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year
2009
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
WDS´09 Proceedings of Contributed Papers: Part II - Physics of Plasmas and Ionized Media
ISBN
978-80-7378-102-6
ISSN
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e-ISSN
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Number of pages
7
Pages from-to
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Publisher name
Matfyzpress
Place of publication
Prague
Event location
Prague
Event date
Jan 1, 2009
Type of event by nationality
EUR - Evropská akce
UT code for WoS article
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