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Titel Limits on the core temperature anisotropy of solar wind protons
VerfasserIn E. Marsch, L. Zhao, C.-Y. Tu
Medientyp Artikel
Sprache Englisch
ISSN 0992-7689
Digitales Dokument URL
Erschienen In: Annales Geophysicae ; 24, no. 7 ; Nr. 24, no. 7 (2006-08-09), S.2057-2063
Datensatznummer 250015609
Publikation (Nr.) Volltext-Dokument vorhandencopernicus.org/angeo-24-2057-2006.pdf
 
Zusammenfassung
We analyse the temperature anisotropy of the protons in the solar wind and thereby concentrate on plasma data obtained in the year 1976 of the Helios 1 and Helios 2 missions. We derive the core proton temperatures $T_perp$ and $T_parallel$, in the directions perpendicular and parallel to the magnetic field, as well as the core parallel plasma beta, $beta_parallel$. The data are separately analysed for two distance ranges, $R{leq}0.4$AU and $R{>}0.4$AU, and divided into 24 bins for the plasma beta, in the range from $beta_parallel {=} 0.1$ to $beta_parallel {=}10$, and into 72 bins for the total temperature anisotropy, $A{=}1{-}T_perp/T_parallel$, which is here considered in the range from −0.9 to 0.9. The number of spectra in each bin is determined to obtain distributions. The statistical results are presented in two-dimensional histograms. For each column we define a critical upper and lower limit of the anisotropy. The resulting empirical points are compared with the known theoretical instability thresholds. The protons are found to come with increasing radial distance closer to the fire-hose instability threshold.
 
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