Impact of ICME- and SIR/CIR-Driven Geomagnetic Storms on the Ionosphere over Hungary

We investigate the differences between the effects of geomagnetic storms due to Interplanetary Coronal Mass Ejections (ICME) and due to Stream Interaction Regions or Corotating Interaction Regions (SIR/CIR) on the ionospheric F2-layer during the maximum of solar cycle 24. We have created a unique li...

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Published in:Atmosphere
Main Authors: Kitti Alexandra Berényi, Andrea Opitz, Zsuzsanna Dálya, Árpád Kis, Veronika Barta
Format: Article
Language:English
Published: MDPI AG 2023-08-01
Subjects:
Online Access:https://www.mdpi.com/2073-4433/14/9/1377
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author Kitti Alexandra Berényi
Andrea Opitz
Zsuzsanna Dálya
Árpád Kis
Veronika Barta
author_facet Kitti Alexandra Berényi
Andrea Opitz
Zsuzsanna Dálya
Árpád Kis
Veronika Barta
author_sort Kitti Alexandra Berényi
collection DOAJ
container_title Atmosphere
description We investigate the differences between the effects of geomagnetic storms due to Interplanetary Coronal Mass Ejections (ICME) and due to Stream Interaction Regions or Corotating Interaction Regions (SIR/CIR) on the ionospheric F2-layer during the maximum of solar cycle 24. We have created a unique list of the ICME- and SIR/CIR-driven geomagnetic storm events for the time interval between November 2012 and October 2014. Finally, 42 clear ICME and 34 clear SIR/CIR events were selected for this analysis. The individual geomagnetic storm periods were grouped by seasons, time of day, and local time of Dst<sub>min</sub> and were analyzed using three different methods: linear correlation analysis using 4-h averages of foF2 parameters and the geomagnetic indices (1st), daily variation of deltafoF2 (2nd), and 3D plotting: geomagnetic indices vs. time vs. deltafoF2 (3rd). The main phase day of the ICME- and SIR/CIR-induced geomagnetic storms was our main focus. We used manually evaluated ionospheric foF2 parameters measured at the Sopron ionosonde station and the geomagnetic indices (Kp, Dst, and AE) for this analysis. We have found that in most cases, the variation of the Dst index is the best indicator of the impact caused in the F2 layer. We conclude as well that the representation of the data by the third method gives a better description of the ICME and SIR/CIR-triggered storm behavior. In addition, our investigation shows that the SIR/CIR-related perturbations can be predicted with greater accuracy with the second method.
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spelling doaj-art-e5448acf31e44cd1b3c17330e15563102025-08-19T22:39:03ZengMDPI AGAtmosphere2073-44332023-08-01149137710.3390/atmos14091377Impact of ICME- and SIR/CIR-Driven Geomagnetic Storms on the Ionosphere over HungaryKitti Alexandra Berényi0Andrea Opitz1Zsuzsanna Dálya2Árpád Kis3Veronika Barta4ELKH-ELTE Space Research Group, H-1117 Budapest, HungaryWigner Research Centre for Physics, H-1121 Budapest, HungaryWigner Research Centre for Physics, H-1121 Budapest, HungaryInstitute of Earth Physics and Space Science, H-9400 Sopron, HungaryInstitute of Earth Physics and Space Science, H-9400 Sopron, HungaryWe investigate the differences between the effects of geomagnetic storms due to Interplanetary Coronal Mass Ejections (ICME) and due to Stream Interaction Regions or Corotating Interaction Regions (SIR/CIR) on the ionospheric F2-layer during the maximum of solar cycle 24. We have created a unique list of the ICME- and SIR/CIR-driven geomagnetic storm events for the time interval between November 2012 and October 2014. Finally, 42 clear ICME and 34 clear SIR/CIR events were selected for this analysis. The individual geomagnetic storm periods were grouped by seasons, time of day, and local time of Dst<sub>min</sub> and were analyzed using three different methods: linear correlation analysis using 4-h averages of foF2 parameters and the geomagnetic indices (1st), daily variation of deltafoF2 (2nd), and 3D plotting: geomagnetic indices vs. time vs. deltafoF2 (3rd). The main phase day of the ICME- and SIR/CIR-induced geomagnetic storms was our main focus. We used manually evaluated ionospheric foF2 parameters measured at the Sopron ionosonde station and the geomagnetic indices (Kp, Dst, and AE) for this analysis. We have found that in most cases, the variation of the Dst index is the best indicator of the impact caused in the F2 layer. We conclude as well that the representation of the data by the third method gives a better description of the ICME and SIR/CIR-triggered storm behavior. In addition, our investigation shows that the SIR/CIR-related perturbations can be predicted with greater accuracy with the second method.https://www.mdpi.com/2073-4433/14/9/1377ionosphereionospheric stormsgeomagnetic stormsgeomagnetic indicesspace weathersolar eruptions
spellingShingle Kitti Alexandra Berényi
Andrea Opitz
Zsuzsanna Dálya
Árpád Kis
Veronika Barta
Impact of ICME- and SIR/CIR-Driven Geomagnetic Storms on the Ionosphere over Hungary
ionosphere
ionospheric storms
geomagnetic storms
geomagnetic indices
space weather
solar eruptions
title Impact of ICME- and SIR/CIR-Driven Geomagnetic Storms on the Ionosphere over Hungary
title_full Impact of ICME- and SIR/CIR-Driven Geomagnetic Storms on the Ionosphere over Hungary
title_fullStr Impact of ICME- and SIR/CIR-Driven Geomagnetic Storms on the Ionosphere over Hungary
title_full_unstemmed Impact of ICME- and SIR/CIR-Driven Geomagnetic Storms on the Ionosphere over Hungary
title_short Impact of ICME- and SIR/CIR-Driven Geomagnetic Storms on the Ionosphere over Hungary
title_sort impact of icme and sir cir driven geomagnetic storms on the ionosphere over hungary
topic ionosphere
ionospheric storms
geomagnetic storms
geomagnetic indices
space weather
solar eruptions
url https://www.mdpi.com/2073-4433/14/9/1377
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AT andreaopitz impactoficmeandsircirdrivengeomagneticstormsontheionosphereoverhungary
AT zsuzsannadalya impactoficmeandsircirdrivengeomagneticstormsontheionosphereoverhungary
AT arpadkis impactoficmeandsircirdrivengeomagneticstormsontheionosphereoverhungary
AT veronikabarta impactoficmeandsircirdrivengeomagneticstormsontheionosphereoverhungary