TY - JOUR
T1 - Nonlinear upper hybrid waves generated in ionospheric hf heating experiments at HAARP
AU - Kuo, Spencer P.
AU - Watkins, Brenton J.
N1 - Funding Information:
Manuscript received September 2, 2019; revised October 21, 2019; accepted October 27, 2019. Date of publication November 22, 2019; date of current version December 11, 2019. This work was supported by the U.S. Air Force High Frequency Active Auroral Research Program (HAARP) and by the Office of Naval Research, Grant No. ONR-N00014-10-1-0856. The review of this article was arranged by Senior Editor S. T. Lai. (Corresponding author: Spencer P. Kuo.) S. P. Kuo is with the New York University Tandon School of Engineering, Brooklyn, NY 11201 USA (e-mail: [email protected]).
Publisher Copyright:
© 1973-2012 IEEE.
PY - 2019/12
Y1 - 2019/12
N2 - Excitation of nonlinear upper hybrid waves by O-mode HF heater in the ionospheric heating experiments was explored via HAARP digisonde operated in a fast mode. The observations are manifested by a bump in the virtual spread, which expands the ionogram echoes upward as much as 140 km and is located below the upper hybrid resonance frequency. The bump is similar to that, occurring in daytime ionograms, caused by the cusp at the E-F2 layer transition, indicating that there is a small ledge in the density profile similar to E-F2 layer transitions. The ionograms also show that the virtual height spread, which exceeds 50 km over a significant frequency range below the upper hybrid resonance frequency, is downward, rather than upward as observed in a natural Spread-F situation. It indicates that density irregularities along the geomagnetic field, rather than field-aligned, were generated. Theory shows that the upper hybrid waves excited by the parametric instabilities evolve into nonlinear periodic and solitary waves that enhance downward virtual height spread and generate density cavity to explain the experimental observations.
AB - Excitation of nonlinear upper hybrid waves by O-mode HF heater in the ionospheric heating experiments was explored via HAARP digisonde operated in a fast mode. The observations are manifested by a bump in the virtual spread, which expands the ionogram echoes upward as much as 140 km and is located below the upper hybrid resonance frequency. The bump is similar to that, occurring in daytime ionograms, caused by the cusp at the E-F2 layer transition, indicating that there is a small ledge in the density profile similar to E-F2 layer transitions. The ionograms also show that the virtual height spread, which exceeds 50 km over a significant frequency range below the upper hybrid resonance frequency, is downward, rather than upward as observed in a natural Spread-F situation. It indicates that density irregularities along the geomagnetic field, rather than field-aligned, were generated. Theory shows that the upper hybrid waves excited by the parametric instabilities evolve into nonlinear periodic and solitary waves that enhance downward virtual height spread and generate density cavity to explain the experimental observations.
KW - Ionosphere
KW - Jacobian elliptic functions
KW - Spread-F
KW - ionospheric density cusp
KW - ionospheric heating and modification
KW - nonlinear upper hybrid waves
KW - nonlinear wave propagation
KW - plasma heating
KW - plasma waves
KW - solitons
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U2 - 10.1109/TPS.2019.2950752
DO - 10.1109/TPS.2019.2950752
M3 - Article
AN - SCOPUS:85076642707
SN - 0093-3813
VL - 47
SP - 5334
EP - 5338
JO - IEEE Transactions on Plasma Science
JF - IEEE Transactions on Plasma Science
IS - 12
M1 - 8910457
ER -