Intermittency Analysis and Spatial Dependence of Magnetic Field Disturbances in the Fast Solar Wind

Details Intermittency Analysis and Spatial Dependence of Magnetic Field Disturbances in the Fast Solar Wind Intermittency Analysis and Spatial Dependence of Magnetic Field Disturbances in the Fast Solar Wind

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agusmsh31b..03y&link_type=abstract

American Geophysical Union, Spring Meeting 2009, abstract #SH31B-03

Mathematics

Probability

2134 Interplanetary Magnetic Fields, 2149 Mhd Waves And Turbulence (2752, 6050, 7836)

Scientific paper

The intermittency properties of the magnetic field fluctuations in the fast solar wind are investigated here at various heliocentric distances based on the Helios measurements from 0.29 to 1.0 AU during 1974-1981. Seven quantities of normalized PDF (Probability Distribution Function) associated with the magnetic field and its disturbances and the magnetic energy are utilized to characterize the intermittency by fitting the PDF with a Castaing distribution and by using the idea of

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