DocumentCode :
124866
Title :
Multi-station observations of frequency dependence of amplitude and polarization of the ELF waves generated via ionospheric modification
Author :
Maxworth, Ashanthi S. ; Golkowski, Mark ; Cohen, Morris B.
Author_Institution :
Dept. of Electr. Eng., Univ. of Colorado Denver, Denver, CO, USA
fYear :
2014
fDate :
8-11 Jan. 2014
Firstpage :
1
Lastpage :
1
Abstract :
Summary form only given. Generation of Extremely Low Frequency (ELF) and Very Low Frequency (VLF) signals through ionospheric modification has been practiced for many years. In ionospheric heating with high power HF waves, the electron temperature of the lower ionosphere is increased thereby changing the particle collision frequency and conductivity of the medium. Modulating the conductivity allows modulation of natural current systems.Our experiments were carried out at the High Frequency Active Auroral Research Program (HAARP) facility in Alaska, USA. In this experiment, the ionosphere was heated with a vertical amplitude modulating signal and the modulation frequency was changed sequentially within an array of 40 frequencies. The observed magnetic field amplitude and polarization of the generated ELF/VLF signals were analyzed for multiple sites and as a function of modulation frequency. Our three observation sites: Chistochina, Paxon and Paradise are located within 36km (azimuth 47.7°), 50.2km (azimuth -20°) and 99km (azimuth 80.3°) respectively. Based on the experimental results, we can show that the highest magnetic field strength was observed at 2.1 kHz which is the resonance frequency of the ionosphere, and the next highest peaks are observed at 4.1 kHz, 6.1 kHz respectively for all three sites. Out of the three sites Paxon shows the highest circularity in the magnetic field polarization, compared to Chistochina and Paradise which show highly linear polarizations. The experimental results were compared with a theoretical simulation model results and it was clear that in both cases, Hall current dominates in Chistochina and Paradise sites and Paxon is dominated by the Pedersen current. The Chistochina site shows the highest magnetic fieldfield amplitudes in both experimental and simulation environments. Depending upon the experimental and simulation observations at the three sites, a radiation pattern for the HAARP ionospheric heater c- n be mapped.
Keywords :
electromagnetic wave polarisation; ionospheric disturbances; ionospheric electromagnetic wave propagation; ionospheric techniques; radiowave propagation; ELF wave amplitude; ELF wave polarization; HAARP ionospheric heater; Hall current; electron temperature; extremely low frequency signal generation; frequency 2.1 kHz; frequency 4.1 kHz; frequency 6.1 kHz; frequency dependence; high frequency active auroral research program; high power HF wave; ionospheric heating; ionospheric modification; multistation observation; natural current system; very low frequency signal; Frequency modulation; Geophysical measurement techniques; Ground penetrating radar; Heating; Ionosphere; Magnetic fields;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Radio Science Meeting (USNC-URSI NRSM), 2014 United States National Committee of URSI National
Conference_Location :
Boulder, CO
Print_ISBN :
978-1-4799-3119-4
Type :
conf
DOI :
10.1109/USNC-URSI-NRSM.2014.6928083
Filename :
6928083
Link To Document :
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