Features of Earth’s lower ionosphere during solar eclipse and sunset and sunrise hours according to measurements by the API method near Nizhny Novgorod

Journal Title: Solar-Terrestrial Physics - Year 2024, Vol 10, Issue 3

Abstract

We present the results of experimental studies into the response of Earth’s lower ionosphere to a partial solar eclipse. The studies have been carried out using the method of resonant scattering of radio waves by artificial periodic irregularities (APIs) in ionospheric plasma. The irregularities were created in the field of a standing wave when a powerful radio wave, generated by radiation to the zenith by transmitters of the mid-latitude SURA heating facility, was reflected from the ionosphere. During the eclipse, the scattered signal amplitude increased by 30–40 dB, and the relaxation time increased 1.5–2.0 times. In some cases, stratification of the signal amplitude in the D-region was observed due to stratification of the electron density profile. By analyzing altitude profiles of relaxation time, we obtained neutral component temperature and density, height of the turbopause, and turbulent velocity. The velocity of vertical regular motion of plasma at each height was measured from the time variation in the scattered signal phase. From the results of measurements of scattered signal characteristics during four partial eclipses, we have obtained that the neutral component temperature decreases, on average, 50–70 K. Variations in the temperature, vertical plasma velocity, and turbopause level exhibited deep quasi-periodic variations with periods from 15 min to several hours, typical of internal gravity wave propagation. The vertical temperature and velocity profiles showed changes with altitude on scales ranging from 5 to 30 km. Comparison between the results of studies of the lower ionosphere during sunrise-sunset hours has revealed that its response during a partial eclipse and the transition to the night regime is identical. According to the measurements by the partial reflection method, during the August 01, 2008 eclipse there was a decrease in the electron density in the D-region 3–5 times. We have concluded that during an eclipse there was a significant change in both the ionized and neutral components of the atmosphere in the lower ionosphere.

Authors and Affiliations

Bahmetieva N. V. , Grigoriev G. I. , Zhemyakov I. N. , Kalinina E. E. , Lisov A. A.

Keywords

Related Articles

OPTICAL EFFECTS OF RUNNING SPACECRAFT ENGINES IN THE LOWER THERMOSPHERE

This paper provides a brief overview on optical effects during operation of spacecraft (SC) onboard engines in the lower thermosphere according to observational data from the ISTP SB RAS Geophyisical Observatory. We pres...

ESTIMATED EQUIVALENT RADIATION DOSE AT DIFFERENT ALTITUDES IN EARTH’S ATMOSPHERE

The paper reports the results of simulation of cosmic ray proton transport through Earth’s atmosphere. The main objective of this work is to obtain characteristics of secondary particle fluxes at different altitudes and...

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...

THE PROCESSES OF ENERGY RELEASE IN LOW-POWER SOLAR FLARES

Using flare patrol data for 1972–2010 [http://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-features/solar-flares/], we have conducted statistical studies of small solar flares. We have established a correlation b...

DIAMAGNETIC STRUCTURES AS A BASIS OF QUASI-STATIONARY SLOW SOLAR WIND

The results presented in this review reflect the fundamentals of the modern understanding of the nature of the structure of the slow solar wind (SW) along the entire length from the Sun to the Earth's orbit. It is known...

Download PDF file
  • EP ID EP753797
  • DOI 10.12737/stp-103202414
  • Views 8
  • Downloads 0

How To Cite

Bahmetieva N. V. , Grigoriev G. I. , Zhemyakov I. N. , Kalinina E. E. , Lisov A. A. (2024). Features of Earth’s lower ionosphere during solar eclipse and sunset and sunrise hours according to measurements by the API method near Nizhny Novgorod. Solar-Terrestrial Physics, 10(3), -. https://europub.co.uk/articles/-A-753797