Computer Science – Numerical Analysis
Scientific paper
Mar 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1216..109g&link_type=abstract
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, Volume 1216, pp. 109-114 (2010).
Computer Science
Numerical Analysis
1
Solar Wind, Astrophysical Plasma, Plasma Turbulence, Magnetic Fields, Plasma Alfven Waves, Numerical Analysis, Particle Emission, Solar Wind, Magnetohydrodynamics And Plasmas, Plasma Turbulence, Electric And Magnetic Fields, Solar Magnetism, Magnetohydrodynamic Waves, Numerical Simulations Of Chaotic Systems
Scientific paper
The interplanetary medium provides a vast natural laboratory for studying many fundamental questions about astrophysical plasmas. In this paper I make a short review on what we know about turbulent fluctuations which behave differently at low (f<1 Hz) and high (f> Hz) frequencies. Particular attention is made about anisotropy at low frequency and its MHD modeling as well as the origin of a second inertial range at high frequencies characterized by steep power law spectra which cannot be associated with MHD fluctuations.
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