Global‐Scale Ionospheric Tomography During the March 17, 2015 Geomagnetic Storm

Abstract The correct representation of global‐scale electron density is crucial for monitoring and exploring the space weather. This study investigates whether the ground‐based Global Navigation Satellite System (GNSS) tomography can be used to reflect the global spatial and temporal responses of th...

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Main Authors: F. S. Prol, T. Kodikara, M. M. Hoque, C. Borries
Format: Article
Language:English
Published: Wiley 2021-12-01
Series:Space Weather
Online Access:https://doi.org/10.1029/2021SW002889
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author F. S. Prol
T. Kodikara
M. M. Hoque
C. Borries
author_facet F. S. Prol
T. Kodikara
M. M. Hoque
C. Borries
author_sort F. S. Prol
collection DOAJ
description Abstract The correct representation of global‐scale electron density is crucial for monitoring and exploring the space weather. This study investigates whether the ground‐based Global Navigation Satellite System (GNSS) tomography can be used to reflect the global spatial and temporal responses of the ionosphere under storm conditions. A global tomography of the ionosphere electron density is constructed based on data from over 2,700 GNSS stations. In comparison to previous techniques, advances are made in spatial and temporal resolution, and in the assessment of results. To demonstrate the capabilities of the approach, the developed method is applied to the March 17, 2015 geomagnetic storm. The tomographic reconstructions show good agreement with electron density observations from worldwide ionosondes, Millstone Hill incoherent scatter radar and in‐situ measurements from satellite missions. Also, the results show that the tomographic technique is capable of reproducing plasma variabilities during geomagnetically disturbed periods including features such as equatorial ionization anomaly enhancements and depletion. Validation results of this brief study period show that the accuracy of our tomography is better than the Neustrelitz Electron Density Model, which is the model used as background, and physics‐based thermosphere‐ionosphere‐electrodynamics general circulation model. The results show that our tomography approach allows us to specify the global electron density from ground to ∼900 km accurately. Given the demonstrated quality, this global electron density reconstruction has potential for improving applications such as assessment of the effects of the electron density on radio signals, GNSS positioning, computation of ray tracing for radio‐signal transmission, and space weather monitoring.
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issn 1542-7390
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publishDate 2021-12-01
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series Space Weather
spelling doaj-art-4edf2bd31964480e80b9d10d8775f5cc2025-01-14T16:27:22ZengWileySpace Weather1542-73902021-12-011912n/an/a10.1029/2021SW002889Global‐Scale Ionospheric Tomography During the March 17, 2015 Geomagnetic StormF. S. Prol0T. Kodikara1M. M. Hoque2C. Borries3German Aerospace Center (DLR) Institute for Solar‐Terrestrial Physics Neustrelitz GermanyGerman Aerospace Center (DLR) Institute for Solar‐Terrestrial Physics Neustrelitz GermanyGerman Aerospace Center (DLR) Institute for Solar‐Terrestrial Physics Neustrelitz GermanyGerman Aerospace Center (DLR) Institute for Solar‐Terrestrial Physics Neustrelitz GermanyAbstract The correct representation of global‐scale electron density is crucial for monitoring and exploring the space weather. This study investigates whether the ground‐based Global Navigation Satellite System (GNSS) tomography can be used to reflect the global spatial and temporal responses of the ionosphere under storm conditions. A global tomography of the ionosphere electron density is constructed based on data from over 2,700 GNSS stations. In comparison to previous techniques, advances are made in spatial and temporal resolution, and in the assessment of results. To demonstrate the capabilities of the approach, the developed method is applied to the March 17, 2015 geomagnetic storm. The tomographic reconstructions show good agreement with electron density observations from worldwide ionosondes, Millstone Hill incoherent scatter radar and in‐situ measurements from satellite missions. Also, the results show that the tomographic technique is capable of reproducing plasma variabilities during geomagnetically disturbed periods including features such as equatorial ionization anomaly enhancements and depletion. Validation results of this brief study period show that the accuracy of our tomography is better than the Neustrelitz Electron Density Model, which is the model used as background, and physics‐based thermosphere‐ionosphere‐electrodynamics general circulation model. The results show that our tomography approach allows us to specify the global electron density from ground to ∼900 km accurately. Given the demonstrated quality, this global electron density reconstruction has potential for improving applications such as assessment of the effects of the electron density on radio signals, GNSS positioning, computation of ray tracing for radio‐signal transmission, and space weather monitoring.https://doi.org/10.1029/2021SW002889
spellingShingle F. S. Prol
T. Kodikara
M. M. Hoque
C. Borries
Global‐Scale Ionospheric Tomography During the March 17, 2015 Geomagnetic Storm
Space Weather
title Global‐Scale Ionospheric Tomography During the March 17, 2015 Geomagnetic Storm
title_full Global‐Scale Ionospheric Tomography During the March 17, 2015 Geomagnetic Storm
title_fullStr Global‐Scale Ionospheric Tomography During the March 17, 2015 Geomagnetic Storm
title_full_unstemmed Global‐Scale Ionospheric Tomography During the March 17, 2015 Geomagnetic Storm
title_short Global‐Scale Ionospheric Tomography During the March 17, 2015 Geomagnetic Storm
title_sort global scale ionospheric tomography during the march 17 2015 geomagnetic storm
url https://doi.org/10.1029/2021SW002889
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AT tkodikara globalscaleionospherictomographyduringthemarch172015geomagneticstorm
AT mmhoque globalscaleionospherictomographyduringthemarch172015geomagneticstorm
AT cborries globalscaleionospherictomographyduringthemarch172015geomagneticstorm