The thresholds of ionospheric plasma instabilities pumped by high-frequency radio waves at EISCAT

We test the existing theories regarding the thresholds for the parametric decay instability (PDI), the oscillating two-steam instability (OTSI), and the thermal parametric instability (TPI) using the European Incoherent Scatter (EISCAT) facility's ionospheric heater. In these processes, the pum...

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Bibliographic Details
Published in:Journal of Geophysical Research: Space Physics
Main Authors: Bryers, Carl, Kosch, Michael, Senior, Andrew, Rietveld, M. T., Yeoman, T. K.
Format: Article in Journal/Newspaper
Language:English
Published: 2013
Subjects:
Online Access:https://eprints.lancs.ac.uk/id/eprint/67972/
https://eprints.lancs.ac.uk/id/eprint/67972/1/jgra50698.pdf
https://doi.org/10.1002/2013JA019429
Description
Summary:We test the existing theories regarding the thresholds for the parametric decay instability (PDI), the oscillating two-steam instability (OTSI), and the thermal parametric instability (TPI) using the European Incoherent Scatter (EISCAT) facility's ionospheric heater. In these processes, the pump wave can couple to various electrostatic waves in the F layer ionosphere, which can be observed using the EISCAT UHF radar (PDI and OTSI) or by HF radar (TPI). On 19 October 2012, the heater power was stepped from ∼0.5 MW to ∼100 MW effective radiated power in seven steps using a 1 min on, 1 min off cycle. We use an electric field model, taking into account D region absorption, to compare theory with our observations. In all three cases, we find good agreement. In addition, the growth of striations formed during the TPI causes anomalous absorption of the heater wave, which we observe as decreased UHF ion line and plasma line backscatter power. We show evidence that heating for a prolonged period of time reduces the UHF ion line intensity throughout the experiment.