Solar Wind Ions at 1. Constraints and Correlations
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.
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2014
- Bibcode:
- 2014AGUFMSH31A4109H
- Keywords:
-
- 2139 Interplanetary shocks;
- INTERPLANETARY PHYSICS;
- 7534 Radio emissions;
- SOLAR PHYSICS;
- ASTROPHYSICS;
- AND ASTRONOMY;
- 7829 Kinetic waves and instabilities;
- SPACE PLASMA PHYSICS;
- 7867 Wave/particle interactions;
- SPACE PLASMA PHYSICS