INFLUENCE OF STRONG SOLAR PROTON EVENTS ON PROPAGATION OF RADIO SIGNALS IN THE VLF RANGE IN A HIGH-LATITUDE REGION

Journal Title: Solar-Terrestrial Physics - Year 2023, Vol 9, Issue 3

Abstract

In this paper, we examine the features of RSDN-20 signal propagation in a high-latitude Earth–ionosphere waveguide during solar proton events, using computational experiment methods. We have analyzed two proton ground-level enhancement (GLE) events of December 13, 2006 (GLE70) and September 10, 2017 (GLE72). Electron density profiles were constructed using the Global Dynamic Model of Ionosphere (GDMI) and the RUSCOSMICS model, developed at PGI. We present estimated phase and amplitude changes in RSDN-20 signals during precipitation of high-energy protons in the high-latitude region of the Earth–ionosphere waveguide. From the results of computational experiments and the analysis of the electromagnetic signal attenuation based on analytical Maxwell’s equation system solution in magnetized ionospheric plasma, we have found a pattern in the signal attenuation frequency dependence associated simultaneously with the signal reflection height, electron density profiles, and the collision frequency of electrons with neutral particles and ions. We discuss limitations of the computational experiment method and compare simulation results with data from Lovozero and Tuloma observatories.

Authors and Affiliations

Akhmetov O. I. , Mingalev I. V. , Mingalev O. V. , Belahovskiy V. B. , Maurchev E. A. , Larchenko A. V. , Suvorova Z. V. , Balabin Y. V.

Keywords

Related Articles

MEASUREMENT OF SIBERIAN RADIOHELIOGRAPH CABLE DELAYS

To achieve the maximum dynamic range of solar radio images obtained using aperture synthesis in relatively wide frequency bands 0.1−0.5 % of the operating frequency, it is necessary to compensate the signal propagation d...

GLOBAL DISTURBANCE OF EARTH’S MAGNETOSPHERE AND ITS CONNECTION WITH SPACE WEATHER

This paper deals with extreme conditions of the global magnetosphere disturbance: very quiet and greatly disturbed, and their relationship with interplanetary medium parameters. The degree of global magnetosphere disturb...

Manifestation of solar activity and dynamics of the atmosphere in variations of 577.7 and 630.0 nm atmospheric emissions in solar cycle 24

In the paper, variations of the night emission intensities in the 557.7 and 630 nm atomic oxygen lines [OI] in 2011–2019 have been analyzed. The analysis is based on data from the ISTP SB RAS Geophysical Observatory. The...

Observation at radio frequencies of the hydroxyl (OH) absorption line in filaments and prominences above active regions of the Sun

When observing the Sun with RATAN-600 radio telescope using a spectropolarimetric complex in the range 1–3 GHz, as well as when observing coronal rain, absorption in the radio emission was discovered in the spectral regi...

TURBULENT PARAMETERS AT DIFFERENT HEIGHTS IN THE ATMOSPHERE. SHACK–HARTMANN WAVEFRONT SENSOR DATA

The paper presents the results of studies of wavefront distortions at different heights in the atmosphere. We have used measurement wavefront data to determine optical turbulence parameters along the line of sight of the...

Download PDF file
  • EP ID EP722178
  • DOI 10.12737/stp-93202305
  • Views 37
  • Downloads 0

How To Cite

Akhmetov O. I. , Mingalev I. V. , Mingalev O. V. , Belahovskiy V. B. , Maurchev E. A. , Larchenko A. V. , Suvorova Z. V. , Balabin Y. V. (2023). INFLUENCE OF STRONG SOLAR PROTON EVENTS ON PROPAGATION OF RADIO SIGNALS IN THE VLF RANGE IN A HIGH-LATITUDE REGION. Solar-Terrestrial Physics, 9(3), -. https://europub.co.uk./articles/-A-722178