Vertical profile of atmospheric conductivity that matches Schumann resonance observations
نویسندگان
چکیده
We introduce the vertical profile of atmospheric conductivity in the range from 2 to 98 km. The propagation constant of extremely low frequency (ELF) radio waves was computed for this profile by using the full wave solution. A high correspondence is demonstrated of the data thus obtained to the conventional standard heuristic model of ELF propagation constant derived from the Schumann resonance records performed all over the world. We also suggest the conductivity profiles for the ambient day and ambient night conditions. The full wave solution technique was applied for obtaining the corresponding frequency dependence of propagation constant relevant to these profiles. By using these propagation constants, we computed the power spectra of Schumann resonance in the vertical electric field component for the uniform global distribution of thunderstorms and demonstrate their close similarity in all the models. We also demonstrate a strong correspondence between the wave attenuation rate obtained for these conductivity profiles and the measured ones by using the ELF radio transmissions.
منابع مشابه
Relativistic Magnetospheric Electrons: Lower Ionospheric Conductivity and Long-term Atmospheric Variability
Long-term (1979-88) observations of relativistic electrons in the earth's outer magnetosphere show a strong solar cycle dependence with a prominent intensity maximum during the approach to solar minimum (1983-85). This population therefore closely corresponds to the presence of high-speed solar wind streams emanating from solar coronal holes. Using a numerical code, we have calculated the preci...
متن کاملThree-dimensional finite difference time domain modeling of the Schumann resonance parameters on Titan, Venus, and Mars
[1] The conducting ionosphere and conducting surface of Titan, Venus, and Mars form a concentric resonator, which would support the possibility of the existence of global electromagnetic resonances. On Earth, such resonances are commonly referred to as Schumann resonances and are excited by lightning discharges. The detection of such resonances on other planets would give a support for the exis...
متن کاملThree-dimensional finite difference time domain modeling of the diurnal and seasonal variations in Schumann resonance parameters
[1] The diurnal and seasonal variations of Schumann resonances (SR) have been reported in a number of experiments. In this paper, a three-dimensional FDTD model of the Earth-ionosphere cavity with a day-night asymmetric conductivity profile is employed to study the diurnal and seasonal variability of the power and frequency of the first Schumann resonance (SR) mode. Comparison of the FDTD resul...
متن کاملPower variations of Schumann resonances related to El Niño and La Niña phenomena
[1] A three dimensional Finite Difference Time Domain (FDTD)model of the Earth-ionosphere cavitywith the realistic conductivity profile is employed to study the intensity variations of Schumann resonances (SR) associated with the El Niño and La Niña phenomena. Comparison of the results derived from our FDTD model and the previous studies by other authors on related subjects shows that the inten...
متن کاملA Technique for Recovering the Vertical Number Density Profile of Atmospheric Gases from Planetary Occultation Data
The occultation technique of determining the properties of the atmosphere using absorption spectroscopy is examined. The intensity of a star, in certain atmospheric absorption bands, is monitored by a satellite tracking the star during occultation by the Earth’s atmosphere. The intensity data in certain wavelength intervals, where absorption is attributed to a single species, are related to the...
متن کامل