Temporal evolution of pump beam self‐focusing at the High‐Frequency Active Auroral Research Program
2007; American Geophysical Union; Volume: 112; Issue: A8 Linguagem: Inglês
10.1029/2007ja012264
ISSN2156-2202
AutoresM. J. Kosch, T. R. Pedersen, Е. В. Мишин, M. Starks, E. Gerken‐Kendall, D. D. Sentman, Shin‐ichiro Oyama, B. J. Watkins,
Tópico(s)Astro and Planetary Science
ResumoOn 4 February 2005 the High‐Frequency Active Auroral Research Program (HAARP) facility was operated at 2.85 MHz to produce artificial optical emissions in the ionosphere while passing through the second electron gyroharmonic. All‐sky optical recordings were performed with 15 s integration, alternating between 557.7 and 630 nm. We report the first optical observations showing the temporal evolution of large‐scale pump wave self‐focusing in the magnetic zenith, observed in the 557.7 nm images. These clearly show that the maximum intensity was not reached after 15 s of pumping, which is unexpected since the emission delay time is <1 s, and that the optical signature had intensified in a much smaller region within the beam after 45 s of pumping. In addition, adjacent regions within the beam lost intensity. Radar measurements indicate a plasma depletion of ∼1% near the HF reflection altitude. Ray tracing of the pump wave through the plasma depletion region, which forms a concave reflecting radio wave mirror, reproduces the optical spatial morphology. A radio wave flux density gain of up to ∼30 dB may occur. In addition, the ray trace is consistent with the observed artificial optical emissions for critical plasma frequencies down to ∼0.5 MHz below the pump frequency.
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