Sub-ionospheric VLF signal anomaly due to geomagnetic storms: a statistical study

We investigate quantitatively the effect of geomagnetic storms on the sub-ionospheric VLF/LF (Very Low Frequency/Low Frequency) propagations for different latitudes based on 2-year nighttime data from Japanese VLF/LF observation network. Three statistical parameters such as average signal amplitu...

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Main Authors: K. Tatsuta, Y. Hobara, S. Pal, M. Balikhin
Format: Article
Language:English
Published: Copernicus Publications 2015-11-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/33/1457/2015/angeo-33-1457-2015.pdf
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author K. Tatsuta
Y. Hobara
Y. Hobara
S. Pal
S. Pal
M. Balikhin
author_facet K. Tatsuta
Y. Hobara
Y. Hobara
S. Pal
S. Pal
M. Balikhin
author_sort K. Tatsuta
collection DOAJ
description We investigate quantitatively the effect of geomagnetic storms on the sub-ionospheric VLF/LF (Very Low Frequency/Low Frequency) propagations for different latitudes based on 2-year nighttime data from Japanese VLF/LF observation network. Three statistical parameters such as average signal amplitude, variability of the signal amplitude, and nighttime fluctuation were calculated daily for 2 years for 16–21 independent VLF/LF transmitter–receiver propagation paths consisting of three transmitters and seven receiving stations. These propagation paths are suitable to simultaneously study high-latitude, low-mid-latitude and mid-latitude D/E-region ionospheric properties. We found that these three statistical parameters indicate significant anomalies exceeding at least 2 times of their standard deviation from the mean value during the geomagnetic storm time period in the high-latitude paths with an occurrence rate of anomaly between 40 and 50 % presumably due to the auroral energetic electron precipitation. The mid-latitude and low-mid-latitude paths have a smaller influence from the geomagnetic activity because of a lower occurrence rate of anomalies even during the geomagnetically active time period (from 20 to 30 %). The anomalies except geomagnetic storm periods may be caused by atmospheric and/or lithospheric origins. The statistical occurrence rates of ionospheric anomalies for different latitudinal paths during geomagnetic storm and non-storm time periods are basic and important information not only to identify the space weather effects toward the lower ionosphere depending on the latitudes but also to separate various external physical causes of lower ionospheric disturbances.
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spelling doaj.art-1949545e777d4a69a41b0dd55343e8c22022-12-21T18:11:27ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762015-11-01331457146710.5194/angeo-33-1457-2015Sub-ionospheric VLF signal anomaly due to geomagnetic storms: a statistical studyK. Tatsuta0Y. Hobara1Y. Hobara2S. Pal3S. Pal4M. Balikhin5Department of Communication Engineering and Informatics, The University of Electro-Communications, Tokyo, JapanDepartment of Communication Engineering and Informatics, The University of Electro-Communications, Tokyo, JapanEarth Environment Research Station, The University of Electro-Communications, Tokyo, JapanDepartment of Communication Engineering and Informatics, The University of Electro-Communications, Tokyo, JapanIndian Centre for Space Physics, Kolkata, IndiaDepartment of Automatic Control and Systems Engineering, University of Sheffield, Sheffield, UKWe investigate quantitatively the effect of geomagnetic storms on the sub-ionospheric VLF/LF (Very Low Frequency/Low Frequency) propagations for different latitudes based on 2-year nighttime data from Japanese VLF/LF observation network. Three statistical parameters such as average signal amplitude, variability of the signal amplitude, and nighttime fluctuation were calculated daily for 2 years for 16–21 independent VLF/LF transmitter–receiver propagation paths consisting of three transmitters and seven receiving stations. These propagation paths are suitable to simultaneously study high-latitude, low-mid-latitude and mid-latitude D/E-region ionospheric properties. We found that these three statistical parameters indicate significant anomalies exceeding at least 2 times of their standard deviation from the mean value during the geomagnetic storm time period in the high-latitude paths with an occurrence rate of anomaly between 40 and 50 % presumably due to the auroral energetic electron precipitation. The mid-latitude and low-mid-latitude paths have a smaller influence from the geomagnetic activity because of a lower occurrence rate of anomalies even during the geomagnetically active time period (from 20 to 30 %). The anomalies except geomagnetic storm periods may be caused by atmospheric and/or lithospheric origins. The statistical occurrence rates of ionospheric anomalies for different latitudinal paths during geomagnetic storm and non-storm time periods are basic and important information not only to identify the space weather effects toward the lower ionosphere depending on the latitudes but also to separate various external physical causes of lower ionospheric disturbances.https://www.ann-geophys.net/33/1457/2015/angeo-33-1457-2015.pdf
spellingShingle K. Tatsuta
Y. Hobara
Y. Hobara
S. Pal
S. Pal
M. Balikhin
Sub-ionospheric VLF signal anomaly due to geomagnetic storms: a statistical study
Annales Geophysicae
title Sub-ionospheric VLF signal anomaly due to geomagnetic storms: a statistical study
title_full Sub-ionospheric VLF signal anomaly due to geomagnetic storms: a statistical study
title_fullStr Sub-ionospheric VLF signal anomaly due to geomagnetic storms: a statistical study
title_full_unstemmed Sub-ionospheric VLF signal anomaly due to geomagnetic storms: a statistical study
title_short Sub-ionospheric VLF signal anomaly due to geomagnetic storms: a statistical study
title_sort sub ionospheric vlf signal anomaly due to geomagnetic storms a statistical study
url https://www.ann-geophys.net/33/1457/2015/angeo-33-1457-2015.pdf
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