Resonant ULF absorption in storm time conditions

The work deals with ULF radar observations of the high-latitude ionosphere. Doppler data from the Norwegian STARE instrument are analyzed for the moderate magnetic storm observed on December 31, 1999 – January 01, 2000. Upon averaging the Doppler signals along radar beams, the spectral power of sign...

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Main Author: Badin V.I.
Format: Article
Language:English
Published: INFRA-M 2017-03-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/ru/nauka/article/16403/view
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author Badin V.I.
author_facet Badin V.I.
author_sort Badin V.I.
collection DOAJ
description The work deals with ULF radar observations of the high-latitude ionosphere. Doppler data from the Norwegian STARE instrument are analyzed for the moderate magnetic storm observed on December 31, 1999 – January 01, 2000. Upon averaging the Doppler signals along radar beams, the spectral power of signals is determined for each beam as a function of frequency ranging from 1 to 10 mHz. Sharp drops (about 10 dB) of spectral powers with frequency are found for all radar beams. A variational analysis of spectral powers is carried out by least squares, with power drops being modeled by stepwise profiles constructed of mean spectral powers preceding and succeeding the drops. Using this variational analysis, the frequency of the power drop is determined for each radar beam. Being averaged over all beams, this frequency is 4.8±0.5 mHz. The results obtained are interpreted as resonant absorption of ultra-low-frequency (ULF) waves occurring on eigenfrequencies of magnetic field lines over wave propagation from the magnetopause deep into the magnetosphere.
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spelling doaj.art-8913cbedf0c344e49c578770ce2990392022-12-22T03:26:41ZengINFRA-MSolar-Terrestrial Physics2500-05352017-03-013110311310.12737/article_58f97156b06fa5.51468016Resonant ULF absorption in storm time conditionsBadin V.I.0Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation RAS, Moscow, RussiaThe work deals with ULF radar observations of the high-latitude ionosphere. Doppler data from the Norwegian STARE instrument are analyzed for the moderate magnetic storm observed on December 31, 1999 – January 01, 2000. Upon averaging the Doppler signals along radar beams, the spectral power of signals is determined for each beam as a function of frequency ranging from 1 to 10 mHz. Sharp drops (about 10 dB) of spectral powers with frequency are found for all radar beams. A variational analysis of spectral powers is carried out by least squares, with power drops being modeled by stepwise profiles constructed of mean spectral powers preceding and succeeding the drops. Using this variational analysis, the frequency of the power drop is determined for each radar beam. Being averaged over all beams, this frequency is 4.8±0.5 mHz. The results obtained are interpreted as resonant absorption of ultra-low-frequency (ULF) waves occurring on eigenfrequencies of magnetic field lines over wave propagation from the magnetopause deep into the magnetosphere.https://naukaru.ru/ru/nauka/article/16403/viewULF wavesElectric fieldsHigh-latitude ionosphere
spellingShingle Badin V.I.
Resonant ULF absorption in storm time conditions
Solar-Terrestrial Physics
ULF waves
Electric fields
High-latitude ionosphere
title Resonant ULF absorption in storm time conditions
title_full Resonant ULF absorption in storm time conditions
title_fullStr Resonant ULF absorption in storm time conditions
title_full_unstemmed Resonant ULF absorption in storm time conditions
title_short Resonant ULF absorption in storm time conditions
title_sort resonant ulf absorption in storm time conditions
topic ULF waves
Electric fields
High-latitude ionosphere
url https://naukaru.ru/ru/nauka/article/16403/view
work_keys_str_mv AT badinvi resonantulfabsorptioninstormtimeconditions