Response of mesospheric ozone to the heating of the lower ionosphere by high-power HF radio emission

2013 ◽  
Vol 53 (1) ◽  
pp. 96-103 ◽  
Author(s):  
Yu. Yu. Kulilov ◽  
V. L. Frolov ◽  
G. I. Grigor’ev ◽  
V. M. Demkin ◽  
G. P. Komrakov ◽  
...  
2020 ◽  
Author(s):  
N.V. Bakhmetieva ◽  
◽  
V.L. Frolov ◽  
Y.Y. Kulikov ◽  
◽  
...  

We present some results of microwave observations of the middle atmosphere ozone under perturbation of the ionosphere by a power HF radio emission by the mid-latitude SURA heating facility (56N, 46E). New experiment was a continuation of studies to clarify the physical nature of the new phenomenon a decrease of the intensity of the microwave emission of the mesosphere in the ozone line when artificially impact on the lower ionosphere [1].


1977 ◽  
Vol 20 (12) ◽  
pp. 1230-1239 ◽  
Author(s):  
A. V. Gurevich ◽  
G. M. Milikh ◽  
I. S. Shlyuger

2021 ◽  
Vol 61 (3) ◽  
pp. 389-398
Author(s):  
Yu. K. Legostaeva ◽  
A. V. Shindin ◽  
S. M. Grach

2013 ◽  
Vol 22 (1) ◽  
Author(s):  
N. V. Bakhmetieva ◽  
G. I. Grigoriev ◽  
A. V. Tolmacheva

AbstractWe present a new perspective ground-based method for diagnostics of the ionosphere and atmosphere parameters. The method uses one of the numerous physical phenomena observed in the ionosphere illuminated by high-power radio waves. It is a generation of the artificial periodic irregularities (APIs) in the ionospheric plasma. The APIs were found while studying the effects of ionospheric high-power HF modification. It was established that the APIs are formed by a standing wave that occurs due to interference between the upwardly radiated radio wave and its reflection off the ionosphere. The API studies are based upon observation of the Bragg backscatter of the pulsed probe radio wave from the artificial periodic structure. Bragg backscatter occurs if the spatial period of the irregularities is equal to half a wavelength of the probe signal. The API techniques makes it possible to obtain the following information: the profiles of electron density from the lower D-region up to the maximum of the F-layer; the irregular structure of the ionosphere including split of the regular E-layer, the sporadic layers; the vertical velocities in the D- and E-regions of the ionosphere; the turbulent velocities, turbulent diffusion coefficients and the turbopause altitude; the neutral temperatures and densities at the E-region altitudes; the parameters of the internal gravity waves and their spectral characteristics; the relative concentration of negative oxygen ions in the D-region. Some new results obtained by the API technique are discussed.


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