First Mode Schumann Resonance Frequency Variation During a Solar Proton Event

A severe X-ray flare occurred on 06 - 07 March 2012 followed by a solar proton event (SPE). During this event we studied the variation in frequency of the first Schumann resonance (SR) spectra mode from the recorded data over Kolkata (22.56°N, 88.5°E). The first mode frequency enhanced (~8.14 Hz, 3....

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Main Authors: Minu Sanfui, Debasish Biswas
Format: Article
Language:English
Published: Chinese Geoscience Union 2016-04-01
Series:Terrestrial, Atmospheric and Oceanic Sciences
Subjects:
Online Access: http://tao.cgu.org.tw/pdf/v272p253.pdf
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spelling doaj-3e4dbb6c778845759d2b8c02e5cbd7072020-11-25T00:25:59ZengChinese Geoscience UnionTerrestrial, Atmospheric and Oceanic Sciences1017-08391017-08392016-04-0127224125110.3319/TAO.2015.12.02.01(AA)1341First Mode Schumann Resonance Frequency Variation During a Solar Proton EventMinu SanfuiDebasish BiswasA severe X-ray flare occurred on 06 - 07 March 2012 followed by a solar proton event (SPE). During this event we studied the variation in frequency of the first Schumann resonance (SR) spectra mode from the recorded data over Kolkata (22.56°N, 88.5°E). The first mode frequency enhanced (~8.14 Hz, 3.85%) during the solar X-ray bursts and immediately after its value decreased (~7.44 Hz, 5.13%) during the proton event. The influences of SPE and X-ray bursts upon the SR frequency fluctuation are explained in terms of the changes in medium ionization, i.e., the change in dielectric property and two layer reflection height variation in the waveguide. The geomagnetic storm effect on the modification of this frequency variation occurring during that time is also considered. http://tao.cgu.org.tw/pdf/v272p253.pdf Earth-ionosphere cavitySolar flareSchumann resonanceMedium conductivityTwo layer theory
collection DOAJ
language English
format Article
sources DOAJ
author Minu Sanfui
Debasish Biswas
spellingShingle Minu Sanfui
Debasish Biswas
First Mode Schumann Resonance Frequency Variation During a Solar Proton Event
Terrestrial, Atmospheric and Oceanic Sciences
Earth-ionosphere cavity
Solar flare
Schumann resonance
Medium conductivity
Two layer theory
author_facet Minu Sanfui
Debasish Biswas
author_sort Minu Sanfui
title First Mode Schumann Resonance Frequency Variation During a Solar Proton Event
title_short First Mode Schumann Resonance Frequency Variation During a Solar Proton Event
title_full First Mode Schumann Resonance Frequency Variation During a Solar Proton Event
title_fullStr First Mode Schumann Resonance Frequency Variation During a Solar Proton Event
title_full_unstemmed First Mode Schumann Resonance Frequency Variation During a Solar Proton Event
title_sort first mode schumann resonance frequency variation during a solar proton event
publisher Chinese Geoscience Union
series Terrestrial, Atmospheric and Oceanic Sciences
issn 1017-0839
1017-0839
publishDate 2016-04-01
description A severe X-ray flare occurred on 06 - 07 March 2012 followed by a solar proton event (SPE). During this event we studied the variation in frequency of the first Schumann resonance (SR) spectra mode from the recorded data over Kolkata (22.56°N, 88.5°E). The first mode frequency enhanced (~8.14 Hz, 3.85%) during the solar X-ray bursts and immediately after its value decreased (~7.44 Hz, 5.13%) during the proton event. The influences of SPE and X-ray bursts upon the SR frequency fluctuation are explained in terms of the changes in medium ionization, i.e., the change in dielectric property and two layer reflection height variation in the waveguide. The geomagnetic storm effect on the modification of this frequency variation occurring during that time is also considered.
topic Earth-ionosphere cavity
Solar flare
Schumann resonance
Medium conductivity
Two layer theory
url http://tao.cgu.org.tw/pdf/v272p253.pdf
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