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Ann. Geophys., 24, 2057-2063, 2006
www.ann-geophys.net/24/2057/2006/
© European Geosciences Union 2006

Limits on the core temperature anisotropy of solar wind protons

E. Marsch¹, L. Zhao², and C.-Y. Tu^3
1Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany
²Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, Michigan, USA
³Department of Geophysics, Peking University, Beijing, China

Abstract. 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 and , in the directions perpendicular and parallel to the magnetic field, as well as the core parallel plasma beta, . The data are separately analysed for two distance ranges, AU and AU, and divided into 24 bins for the plasma beta, in the range from to , and into 72 bins for the total temperature anisotropy, , 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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Citation: Marsch, E., Zhao, L., and Tu, C.-Y.: Limits on the core temperature anisotropy of solar wind protons, Ann. Geophys., 24, 2057-2063, 2006.   Bibtex   EndNote   Reference Manager