THE FIRST COMPARATIVE ANALYSIS OF METEOR ECHO AND SPORADIC SCATTERING IDENTIFIED BY A SELF-LEARNED NEURAL NETWORK IN EKB AND MAGW ISTP SB RAS RADAR DATA

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

Abstract

The paper describes the current version (v.1.1) of the algorithm for automatic classification of signals received by ISTP SB RAS decameter coherent scatter radars. The algorithm is a self-learning neural network that determines the type of scattered signals from the results of physical modeling of radio wave propagation, using radar data and international reference models of the ionosphere and geomagnetic field. According to MAGW and EKB ISTP SB RAS radar data for 2021, the algorithm self-learns to classify scattered signals into initially unknown classes based on physically interpreted parameters of radio wave propagation and data measured by the radar, with 15 frequently observed out of 20 possible hidden classes identified, 14 of which can be interpreted from a physical point of view. To demonstrate the operation of the algorithm, we present the first statistical analysis of observations of signals assigned by the algorithm to classes which we interpret as scattering by meteor trails and scattering with the sporadic E layer respectively. Through a statistical analysis of EKB and MAGW radar data during 2021–2022, we demonstrate the range-altitude characteristics of signals of these types. A correlation is shown between the hourly average numbers of observations of both classes, as well as between the hourly average line-of-sight velocities obtained for both classes. The results obtained make it possible to interpret these classes as a meteor echo and sporadic scattering respectively, and to use radar data to study the interaction between the neutral atmosphere (studied from meteor scattering data) and the lower ionosphere (studied from observations of sporadic scattering). Currently, this classification algorithm works in ISTP SB RAS radars in automatic mode.

Authors and Affiliations

Berngardt O. I.

Keywords

Related Articles

CHROMOSPHERIC K CAII TELESCOPE OF BAIKAL ASTROPHYSICAL OBSERVATORY. NEW LIGHT

In recent years, most results of CaII studies of the solar chromosphere in H and K lines have been based on observations with narrow passband filters. The Baikal Observatory’s full-disk chromospheric telescope for the K...

METHOD FOR CALCULATING TORSIONAL OSCILLATIONS IN EARTH’S ATMOSPHERE FROM NCEP/NCAR, MERRA-2, ECMWF ERA-40, AND ERA-INTERIM

In this paper, we describe a method for calculating low-frequency zonal-mean zonal wind variations, which we call torsional oscillations. We compare the torsional oscillations calculated from the NCEP/NCAR reanalysis I,...

APPEARANCE OF ACTIVE REGIONS AT THE END OF SOLAR CYCLE 24 AND AT THE BEGINNING OF CYCLE 25

The spatial-temporal picture of appearance of active regions and the relationship of their appearance with the structure and development of a large-scale magnetic field were studied during the transition from solar cycle...

BEHAVIOR OF ELECTRON DENSITY IN THE IONOSPHERE OVER NORILSK DURING THE PERIOD OF DECLINING SOLAR ACTIVITY

We report the results of approximation of electron density Ne array obtained with a digisonde at the high-latitude station Norilsk (69.40° N, 88.10° E) during years of declining solar activity (2003–2006). The calculatio...

LONG-TERM SOLAR FLUX OBSERVATIONS WITH IRKUTSK INCOHERENT SCATTER RADAR (IISR) IN 2011–2019

Irkutsk incoherent scatter radar (IISR) is an oblongish horn antenna that operates in a meter waveband (154–162 MHz), has a 0.5°×20° beam, and a frequency steering allowing us to tilt the beam by 30° to the south. Beside...

Download PDF file
  • EP ID EP711655
  • DOI 10.12737/stp-84202206
  • Views 85
  • Downloads 0

How To Cite

Berngardt O. I. (2022). THE FIRST COMPARATIVE ANALYSIS OF METEOR ECHO AND SPORADIC SCATTERING IDENTIFIED BY A SELF-LEARNED NEURAL NETWORK IN EKB AND MAGW ISTP SB RAS RADAR DATA. Solar-Terrestrial Physics, 8(4), -. https://europub.co.uk/articles/-A-711655