Plasma Heating and Alfvénic Turbulence Enhancement During Two Steps of Energy Conversion in Magnetic Reconnection Exhaust Region of Solar Wind
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/856/i=2/a=148/pdf
Reference50 articles.
1. Quadrupolar Magnetic Reconnection in Solar Flares. I. Three‐dimensional Geometry Inferred fromYohkohObservations
2. Magnetic Fluctuation Power Near Proton Temperature Anisotropy Instability Thresholds in the Solar Wind
3. Geospace Environmental Modeling (GEM) Magnetic Reconnection Challenge
4. MULTI-SPECIES MEASUREMENTS OF THE FIREHOSE AND MIRROR INSTABILITY THRESHOLDS IN THE SOLAR WIND
5. Global network of slow solar wind
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