Approach to identification of the tail plasma regimes using Interball-1 data.

Details Approach to identification of the tail plasma regimes using Interball-1 data. Approach to identification of the tail plasma regimes using Interball-1 data.

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999czjph..49..599v&link_type=abstract

Czech. J. Phys., Vol. 49, No. 4a, p. 599 - 606

Physics

1

Plasma: Data Processing, Plasma: Space Research

Scientific paper

This method gives one more way to distinguish qualitatively the plasma regimes in the tail when one processes big data sets. The study is based on the orbital data and the key parameters obtained from MIF-M, DOK-2 and CORALL of the Interball-1 mission. The authors sort the data taking into account typical features of the tail plasma regimes, namely the value of magnetic field magnitude and its variability. The technique is based on plots of low-frequency fluctuation level versus magnetic field magnitude. The background of the method was initially proposed and tested for the Geotail mission data.

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