RESPONSE OF IONOSPHERIC ELECTRON DENSITY PROFILE TO THE ACTION OF POWERFUL HF RADIO-WAVE RADIATION

Journal Title: Solar-Terrestrial Physics - Year 2022, Vol 8, Issue 3

Abstract

Using electron density and temperature equations, we have modeled the dynamics of the electron density profile in the ionosphere due to the expulsion of plasma from localization regions of plasma waves, pumped by high-power HF radio waves, i.e. wave reflection and upper hybrid resonance regions. Causes of the ionospheric plasma expulsion are an increase in the gas-kinetic pressure due to the ohm heating of electrons by plasma waves, and the high-frequency pressure of plasma waves (ponderomotive expulsion). We have established that the ponderomotive expulsion develops more rapidly and is responsible for the formation of local regions of plasma density depletion near plasma resonances, whereas the gas-kinetic pressure increase is responsible for the formation of lower-density region, which is slower in time and more extended and smoother in height. The results obtained qualitatively agree with the data from the experiment conducted at the HAARP facility in 2014.

Authors and Affiliations

Legostaeva Y. K. , Shindin A. V. , Grach S. M.

Keywords

Related Articles

MUON INTENSITY VARIATIONS AND ATMOSPHERIC TEMPERATURE

Muons in the atmosphere are formed during the decay of pions resulting from nuclear interactions of cosmic rays with nuclei of air atoms. The resulting muons are also unstable particles with a short lifetime. Therefore,...

FINE STRUCTURE EVENTS IN MICROWAVE EMISSION DURING SOLAR MINIMUM

The solar minimum is a period with a relatively smaller number of sunspots and solar eruptions, and has been less studied before. Since the radio signal rapidly responds to the change of solar plasma and magnetic field,...

A QUIET DAY EMPIRICAL MODEL OF ELECTRON DENSITY IN THE INDIAN EQUATORIAL F-REGION

In this paper, we present a quiet day empirical model of electron density (Ne) for the Indian equatorial zone at an altitude of 500 km. The model is applicable to all levels of solar activity and is based on the observat...

Large-scale relationships of the geomagnetic indices SYM-H and ASY-H with the north-south IMF component and the solar wind beta parameter

Using annual average values, the relationships are examined of the geomagnetic indices SYM-H, ASY-H, and Dst with solar wind parameters in 1981–2015. The data used was divided into two samples according to the sign of th...

FEATURES OF DEVELOPMENT OF SUSTAINED FLUXES OF HIGH-ENERGY GAMMA-RAY EMISSION AT DIFFERENT STAGES OF SOLAR FLARES

We have studied properties of sustained gamma fluxes having quantum energies of >100 MeV at different stages of flares with 1-min temporal resolution (Fermi/LAT). The most probable process of emergence of high-energy gam...

Download PDF file
  • EP ID EP711648
  • DOI 10.12737/stp-83202211
  • Views 88
  • Downloads 0

How To Cite

Legostaeva Y. K. , Shindin A. V. , Grach S. M. (2022). RESPONSE OF IONOSPHERIC ELECTRON DENSITY PROFILE TO THE ACTION OF POWERFUL HF RADIO-WAVE RADIATION. Solar-Terrestrial Physics, 8(3), -. https://europub.co.uk/articles/-A-711648