PECULIARITIES OF ULF WAVE CHARACTERISTICS IN A MULTICOMPONENT IONOSPHERIC PLASMA

Journal Title: Solar-Terrestrial Physics - Year 2022, Vol 8, Issue 4

Abstract

We have examined the properties of low-frequency electromagnetic waves in multicomponent ionospheric plasma in the 1–30 Hz band, using the magnetoionic theory. Complex permittivity tensor components and refractive indices of normal waves (ordinary and extraordinary) were calculated at altitudes from 80 to 750 km. The calculations show that the refractive indices are highly dependent on frequency and height. Polarization of ordinary and extraordinary waves is elliptical over the entire range of the frequencies investigated. The refractive index and the polarization of normal waves are demonstrated to tend to magnetohydrodynamic (MHD) values only at frequencies lower than 1 Hz. The group velocity vector of an extraordinary wave is not directed along the magnetic field, as follows from the MHD approximation, but it lies inside a cone within ±(5–10) degrees, depending on frequency. The group velocity vector of an ordinary wave is practically independent of the angle with the geomagnetic field as in the MHD approximation. The proposed method for calculating the characteristics of normal waves in the ionosphere can be used to study ULF wave propagation from both natural and artificial ionospheric sources, which arise under the action of powerful HF radio waves in the lower and upper ionosphere.

Authors and Affiliations

Kotik D. S. , Orlova E. V. , Yashnov V. A.

Keywords

Related Articles

PITCH-ANGLE ANISOTROPY AND DIFFERENTIAL RIGIDITY SPECTRA OF COSMIC RAYS DURING GLE ON MAY 2 AND 6, 1998

Using data from the worldwide network of neutron monitors (39 stations) and the method of global spectrographic survey, we have studied pitch-angle anisotropy and differential rigidity spectra of cosmic rays during the g...

RELATION BETWEEN THE AREA OF POLAR CORONAL HOLES AND THE SOLAR WIND SPEED AT A MINIMUM BETWEEN SOLAR CYCLES 22 AND 23

We have used data from the space telescope SOHO/EIT and the spectrometer VEIS on the Wind spacecraft to compare the solar wind (SW) speed near Earth's orbit with changes in the area of polar coronal holes (CHs) on the Su...

COMPLEX OF HELIOGEOPHYSICAL INSTRUMENTS OF NEW GENERATION

The paper discusses the importance of the problem of adverse effects of cosmic processes and phenomena (space weather factors) on the ground engineering and technical infrastructure, space-born radio-electronic facilitie...

TOROIDAL MODELS OF MAGNETIC FIELD WITH TWISTED STRUCTURE

We present and discuss properties of the following magnetic field models in a magnetic cloud: Miller and Turner solution, modified Miller–Turner solution, Romashets–Vandas toroidal and integral models, and Krittinatham–R...

ALFVÉN WAVES: TO THE 80TH ANNIVERSARY OF DISCOVERY

The article is dedicated to the anniversary of the discovery of Alfvén waves. The concept of Alfvén waves has played an outstanding role in the formation and development of cosmic electrodynamics. A distinctive feature o...

Download PDF file
  • EP ID EP711654
  • DOI 10.12737/stp-84202205
  • Views 94
  • Downloads 0

How To Cite

Kotik D. S. , Orlova E. V. , Yashnov V. A. (2022). PECULIARITIES OF ULF WAVE CHARACTERISTICS IN A MULTICOMPONENT IONOSPHERIC PLASMA. Solar-Terrestrial Physics, 8(4), -. https://www.europub.co.uk/articles/-A-711654