Plasma signatures of radial field power dropouts

Details Plasma signatures of radial field power dropouts Plasma signatures of radial field power dropouts

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..475l&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 475-478 (1999).

Physics

Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

A class of small scale structures, with a near-radial magnetic field and a drop in magnetic field fluctuation power, have recently been identified in the polar solar wind. An earlier study of 24 events, each lasting for 6 hours or more, identified no clear plasma signature. In an extension of that work, radial intervals lasting for 4 hours or more (89 in total), have been used to search for a statistically significant plasma signature. It was found that, despite considerable variations between intervals, there was a small but significant drop, on average, in plasma temperature, density and β during these events.

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