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Titel Correlation length of the magnetosheath fluctuations and their relation to upstream parameters
VerfasserIn Jiri Simunek, Olga Gutynska, Jana Safrankova, Zdenek Nemecek
Konferenz EGU General Assembly 2011
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 13 (2011)
Datensatznummer 250050664
 
Zusammenfassung
The magnetosheath is characterized by a variety of low-frequency fluctuations from different sources. In our previous studies, we analyzed magnetic field fluctuations of multipoint Cluster spacecraft observations near dusk/dawn meridian and we have found that the correlation length of these fluctuations depends on the solar wind speed, on a correlation between IMF and magnetosheath magnetic field fluctuations, and on the amplitude of fluctuations. To determine the correlation length in different magnetosheath places and degree of penetration of solar wind fluctuations into the magnetosheath, we use different solar wind monitors and different separations between the magnetosheath spacecraft (Cluster, Themis) and correlation and wavelet techniques. We discuss the influence of foreshock fluctuations on the correlation between the magnetosheath spacecraft.