Structure of groups of eigenfrequencies in spectra of geomagnetic pulsations in the nightside magnetosphere

Using a new method of correlation function for amplitude and phase fluctuations (APCF), records of geomagnetic field component fluctuations (observatories Mondy and Borok) have been processed for a number of hour zones of the nightside magnetosphere. This method is meant to detect groups of equidist...

Full description

Bibliographic Details
Main Author: Polyakov A. R.
Format: Article
Language:English
Published: INFRA-M 2022-09-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/en/nauka/article/48924/view
_version_ 1797997339230601216
author Polyakov A. R.
author_facet Polyakov A. R.
author_sort Polyakov A. R.
collection DOAJ
description Using a new method of correlation function for amplitude and phase fluctuations (APCF), records of geomagnetic field component fluctuations (observatories Mondy and Borok) have been processed for a number of hour zones of the nightside magnetosphere. This method is meant to detect groups of equidistant frequencies inside the spectrum of source signal and also to measure a difference between two neighbor frequencies in each of these groups.
first_indexed 2024-04-11T10:31:11Z
format Article
id doaj.art-44795d072ced47898429304b660a390f
institution Directory Open Access Journal
issn 2500-0535
language English
last_indexed 2024-04-11T10:31:11Z
publishDate 2022-09-01
publisher INFRA-M
record_format Article
series Solar-Terrestrial Physics
spelling doaj.art-44795d072ced47898429304b660a390f2022-12-22T04:29:25ZengINFRA-MSolar-Terrestrial Physics2500-05352022-09-0183465010.12737/stp-83202207Structure of groups of eigenfrequencies in spectra of geomagnetic pulsations in the nightside magnetospherePolyakov A. R.0Institute of Solar-Terrestrial Physics SB RAS, Irkutsk, RussiaUsing a new method of correlation function for amplitude and phase fluctuations (APCF), records of geomagnetic field component fluctuations (observatories Mondy and Borok) have been processed for a number of hour zones of the nightside magnetosphere. This method is meant to detect groups of equidistant frequencies inside the spectrum of source signal and also to measure a difference between two neighbor frequencies in each of these groups.https://naukaru.ru/en/nauka/article/48924/viewsignal processing techniquecorrelation functioneigenfrequencies
spellingShingle Polyakov A. R.
Structure of groups of eigenfrequencies in spectra of geomagnetic pulsations in the nightside magnetosphere
Solar-Terrestrial Physics
signal processing technique
correlation function
eigenfrequencies
title Structure of groups of eigenfrequencies in spectra of geomagnetic pulsations in the nightside magnetosphere
title_full Structure of groups of eigenfrequencies in spectra of geomagnetic pulsations in the nightside magnetosphere
title_fullStr Structure of groups of eigenfrequencies in spectra of geomagnetic pulsations in the nightside magnetosphere
title_full_unstemmed Structure of groups of eigenfrequencies in spectra of geomagnetic pulsations in the nightside magnetosphere
title_short Structure of groups of eigenfrequencies in spectra of geomagnetic pulsations in the nightside magnetosphere
title_sort structure of groups of eigenfrequencies in spectra of geomagnetic pulsations in the nightside magnetosphere
topic signal processing technique
correlation function
eigenfrequencies
url https://naukaru.ru/en/nauka/article/48924/view
work_keys_str_mv AT polyakovar structureofgroupsofeigenfrequenciesinspectraofgeomagneticpulsationsinthenightsidemagnetosphere