SH31A-4109:
Solar Wind Ions at 1 AU: Constraints and Correlations
Wednesday, 17 December 2014
Petr Hellinger, Astronomical Institute, AS CR, Prague 4, Czech Republic and Pavel M. Travnicek, University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States
Abstract:
The solar wind ions at 1 AU exhibit many different correlations and apparent bounds in the multidimensional parameter space. These properties may be imprints of the different processes locally active in the solar wind or remnants of the solar wind origins. We will present a detailed analysis of possible connections between ion temperatures and instability constraints in the solar wind using the large WIND/SWE data set.
