IDENTIFICATION OF SPECTRUM OF SECONDARY ACOUSTIC-GRAVITY WAVES IN THE MIDDLE AND UPPER ATMOSPHERE IN A HIGH-RESOLUTION NUMERICAL MODEL

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

Abstract

Considerable attention has recently been paid to the study of so-called “secondary” acoustic-gravity waves (AGWs) that arise as a result of instability and nonlinear interactions of “primary” wave modes propagating from atmospheric sources, among themselves, and with the mean flow. In this paper, for the first time, the horizontal spatial spectra of primary and secondary AGWs are separated at fixed altitude levels in the middle and upper atmosphere at different time moments, which are simulated using a three-dimensional nonlinear high-resolution model AtmoSym. It is shown that in a short time after switching on the plane wave source at the lower boundary of the model, the spectrum consists of a peak corresponding to primary AGW and quasi-white noise generated by random atmospheric disturbances and the numerical model. Later, secondary peaks appear in the spectra at horizontal wave numbers, which are multiples of the wave numbers of primary AGW. The proposed separation of the spectra of primary and secondary AGWs makes it possible to estimate the relative contribution of secondary AGW at different altitudes, at different times, and with different stability of background temperature and wind profiles in the atmosphere.

Authors and Affiliations

Gavrilov N. M. , Kshevetskii S. P.

Keywords

Related Articles

STATISTICAL PROPERTIES OF AURORAL KILOMETER RADIATION: BASED ON ERG (ARASE) SATELLITE DATA

In this work, we have studied the signals of auroral kilometer radiation (AKR) from sources in the auroral regions of the Northern and Southern hemispheres simultaneously recorded by one satellite. We have carried out a...

SCIENTIFIC GOALS OF OPTICAL INSTRUMENTS OF THE NATIONAL HELIOGEOPHYSICAL COMPLEX

Studies of the upper atmosphere have to be performed using optical photometric and spectrometric means. Modern devices allow precise photometry of the glow of the night atmosphere — airglow — with high temporal spatial a...

Hysteresis phenomena in the response of geomagnetic activity and cosmic ray parameters to variations in the interplanetary medium during a magnetic storm

The dynamics of the intensity of cosmic rays is known to be different on the ascending and descending branches of the 11-year solar cycle, i.e., hysteresis phenomena are observed. Recently, it has been obtained that at s...

STUDYING THE RESPONSE OF THE MID-LATITUDE IONOSPHERE OF THE NORTHERN HEMISPHERE TO MAGNETIC STORMS IN MARCH 2012

We have studied variations in ionospheric and geomagnetic parameters in the Northern Hemisphere during a series of magnetic storms in March 2012 by analyzing data from the Eurasian mid-latitude ionosonde chain, mid- and...

ELECTROMAGNETIC POLLUTION OF NEAR-EARTH SPACE BY POWER LINE EMISSION

We present an overview, based on satellite observations at low Earth orbits, on electromagnetic radiation from ground power transmission lines at an industrial frequency 50–60 Hz. Particular attention has been given to C...

Download PDF file
  • EP ID EP722183
  • DOI 10.12737/stp-93202310
  • Views 58
  • Downloads 0

How To Cite

Gavrilov N. M. , Kshevetskii S. P. (2023). IDENTIFICATION OF SPECTRUM OF SECONDARY ACOUSTIC-GRAVITY WAVES IN THE MIDDLE AND UPPER ATMOSPHERE IN A HIGH-RESOLUTION NUMERICAL MODEL. Solar-Terrestrial Physics, 9(3), -. https://europub.co.uk/articles/-A-722183