Current Sheets Observed by ACE and Ulyssess at Different Heliospheric Distances

Details Current Sheets Observed by ACE and Ulyssess at Different Heliospheric Distances Current Sheets Observed by ACE and Ulyssess at Different Heliospheric Distances

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh51f..07m&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SH51F-07

Physics

Plasma Physics

[7524] Solar Physics, Astrophysics, And Astronomy / Magnetic Fields, [7833] Space Plasma Physics / Mathematical And Numerical Techniques, [7863] Space Plasma Physics / Turbulence

Scientific paper

Current sheets are common structures in the solar wind. They may be the boundaries of flux tubes that originated from the surface structure of the Sun. Using an automatic searching code, the boundary of those flux tubes, i.e. the current sheets, are identified. Through the observations made by the ACE and Ulyssess spacecraft at the different heliospheric distance, the variation of the size and occurrences of those current sheets related to the heliospheric distance are investigated. Two kinds of current sheet populations are distinguished. The implication of our results on the solar wind MHD turbulence, in particular, the intermittency will be discussed.

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