Correlation Dependences Determined by Simultaneous Multispacecraft Observations of Solar Wind and IMF Structures

Details Correlation Dependences Determined by Simultaneous Multispacecraft Observations of Solar Wind and IMF Structures Correlation Dependences Determined by Simultaneous Multispacecraft Observations of Solar Wind and IMF Structures

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.277..323d&link_type=abstract

Astrophysics and Space Science, v. 277, Issue 1/2, p. 323-324 (2001).

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Solar wind measurements on board several spacecraft were used to study
the two-points correlations of the solar wind plasma structures. The
factor shaving the most influence on the correlation level are the
density variability and IMF cone angle. The characteristic length of
large solar wind structures is estimated at 500-1000 R E.

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