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Arranged by LOIS Space Centre, Växjö and PHISP, IRF, Uppsala
In collaboration with Växjö University and Videum Science Park
Sponsored by CDP, Uppsala University, IBM Sweden and the Swedish National Space Board
Radio frequency pumping of ionospheric plasma with orbital angular momentum

Thomas Leyser
tbl@irfu.se
Swedish Institute of Space Physics (IRF)
Uppsala, Sweden

Abstract

Experimental results are presented of pumping ionospheric plasma with a powerful radio wave carrying orbital angular momentum (OAM). The experiments were performed at the High frequency Active Auroral Research Program (HAARP) near Gakona, Alaska, in February 2008. The pumped plasma turbulence was diagnosed by measuring on the ground optical emissions as well as stimulated electromagnetic emissions (SEE) with frequenices near that of the pump frequency. Optical emission show a ring-shaped emission region when the pump beam carries OAM, consistent with the ring-shaped pump beam. Spectral features of SEE that are attributed to Langmuir turbulence are very well developed for a regular pump beam configuration but are significantly weaker when the beam carries OAM in which case upper hybrid turbulence dominates the SEE.

The presentation (PDF)


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Last modified: 2008-06-19 at 21:06:42
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