The Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the $ B_{Z} $ Component of Interplanetary Magnetic Field
Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ...
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| Autor*in: |
Timoçin, Erdinç [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media, LLC, part of Springer Nature 2020 |
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| Übergeordnetes Werk: |
Enthalten in: Wireless personal communications - Springer US, 1994, 114(2020), 4 vom: 31. Mai, Seite 2923-2932 |
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| Übergeordnetes Werk: |
volume:114 ; year:2020 ; number:4 ; day:31 ; month:05 ; pages:2923-2932 |
| Links: |
|---|
| DOI / URN: |
10.1007/s11277-020-07510-z |
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| Katalog-ID: |
OLC2120510601 |
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| 520 | |a Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ_{1} $), Hall conductivity ($ σ_{2} $) data calculated for Rome (41.8° N, 12.5° E); Juliusruh (54.6° N, 13.4° E); Uppsala (59.8° N, 17.6° E); Lycksele (64.7° N, 18.8° E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the $ B_{Z} $ component. From the analysis results it is observed that the turnings in the $ B_{Z} $ component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the $ B_{Z} $ component increases all conductivities while the northward turnings of the $ B_{Z} $ component decreases all conductivities. The effect on the conductivities of the changes in the $ B_{Z} $ component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the $ B_{Z} $ component as latitude increase. | ||
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| 700 | 1 | |a Yeşil, Ali |4 aut | |
| 700 | 1 | |a Ünal, İbrahim |4 aut | |
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10.1007/s11277-020-07510-z doi (DE-627)OLC2120510601 (DE-He213)s11277-020-07510-z-p DE-627 ger DE-627 rakwb eng 620 VZ Timoçin, Erdinç verfasserin aut The Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the $ B_{Z} $ Component of Interplanetary Magnetic Field 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ_{1} $), Hall conductivity ($ σ_{2} $) data calculated for Rome (41.8° N, 12.5° E); Juliusruh (54.6° N, 13.4° E); Uppsala (59.8° N, 17.6° E); Lycksele (64.7° N, 18.8° E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the $ B_{Z} $ component. From the analysis results it is observed that the turnings in the $ B_{Z} $ component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the $ B_{Z} $ component increases all conductivities while the northward turnings of the $ B_{Z} $ component decreases all conductivities. The effect on the conductivities of the changes in the $ B_{Z} $ component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the $ B_{Z} $ component as latitude increase. Ionosphere Ionospheric conductivities Interplanetary magnetic field Superposed epoch analysis Yeşil, Ali aut Ünal, İbrahim aut Enthalten in Wireless personal communications Springer US, 1994 114(2020), 4 vom: 31. Mai, Seite 2923-2932 (DE-627)188950273 (DE-600)1287489-9 (DE-576)049958909 0929-6212 nnns volume:114 year:2020 number:4 day:31 month:05 pages:2923-2932 https://doi.org/10.1007/s11277-020-07510-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MKW AR 114 2020 4 31 05 2923-2932 |
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10.1007/s11277-020-07510-z doi (DE-627)OLC2120510601 (DE-He213)s11277-020-07510-z-p DE-627 ger DE-627 rakwb eng 620 VZ Timoçin, Erdinç verfasserin aut The Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the $ B_{Z} $ Component of Interplanetary Magnetic Field 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ_{1} $), Hall conductivity ($ σ_{2} $) data calculated for Rome (41.8° N, 12.5° E); Juliusruh (54.6° N, 13.4° E); Uppsala (59.8° N, 17.6° E); Lycksele (64.7° N, 18.8° E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the $ B_{Z} $ component. From the analysis results it is observed that the turnings in the $ B_{Z} $ component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the $ B_{Z} $ component increases all conductivities while the northward turnings of the $ B_{Z} $ component decreases all conductivities. The effect on the conductivities of the changes in the $ B_{Z} $ component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the $ B_{Z} $ component as latitude increase. Ionosphere Ionospheric conductivities Interplanetary magnetic field Superposed epoch analysis Yeşil, Ali aut Ünal, İbrahim aut Enthalten in Wireless personal communications Springer US, 1994 114(2020), 4 vom: 31. Mai, Seite 2923-2932 (DE-627)188950273 (DE-600)1287489-9 (DE-576)049958909 0929-6212 nnns volume:114 year:2020 number:4 day:31 month:05 pages:2923-2932 https://doi.org/10.1007/s11277-020-07510-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MKW AR 114 2020 4 31 05 2923-2932 |
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10.1007/s11277-020-07510-z doi (DE-627)OLC2120510601 (DE-He213)s11277-020-07510-z-p DE-627 ger DE-627 rakwb eng 620 VZ Timoçin, Erdinç verfasserin aut The Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the $ B_{Z} $ Component of Interplanetary Magnetic Field 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ_{1} $), Hall conductivity ($ σ_{2} $) data calculated for Rome (41.8° N, 12.5° E); Juliusruh (54.6° N, 13.4° E); Uppsala (59.8° N, 17.6° E); Lycksele (64.7° N, 18.8° E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the $ B_{Z} $ component. From the analysis results it is observed that the turnings in the $ B_{Z} $ component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the $ B_{Z} $ component increases all conductivities while the northward turnings of the $ B_{Z} $ component decreases all conductivities. The effect on the conductivities of the changes in the $ B_{Z} $ component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the $ B_{Z} $ component as latitude increase. Ionosphere Ionospheric conductivities Interplanetary magnetic field Superposed epoch analysis Yeşil, Ali aut Ünal, İbrahim aut Enthalten in Wireless personal communications Springer US, 1994 114(2020), 4 vom: 31. Mai, Seite 2923-2932 (DE-627)188950273 (DE-600)1287489-9 (DE-576)049958909 0929-6212 nnns volume:114 year:2020 number:4 day:31 month:05 pages:2923-2932 https://doi.org/10.1007/s11277-020-07510-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MKW AR 114 2020 4 31 05 2923-2932 |
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10.1007/s11277-020-07510-z doi (DE-627)OLC2120510601 (DE-He213)s11277-020-07510-z-p DE-627 ger DE-627 rakwb eng 620 VZ Timoçin, Erdinç verfasserin aut The Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the $ B_{Z} $ Component of Interplanetary Magnetic Field 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ_{1} $), Hall conductivity ($ σ_{2} $) data calculated for Rome (41.8° N, 12.5° E); Juliusruh (54.6° N, 13.4° E); Uppsala (59.8° N, 17.6° E); Lycksele (64.7° N, 18.8° E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the $ B_{Z} $ component. From the analysis results it is observed that the turnings in the $ B_{Z} $ component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the $ B_{Z} $ component increases all conductivities while the northward turnings of the $ B_{Z} $ component decreases all conductivities. The effect on the conductivities of the changes in the $ B_{Z} $ component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the $ B_{Z} $ component as latitude increase. Ionosphere Ionospheric conductivities Interplanetary magnetic field Superposed epoch analysis Yeşil, Ali aut Ünal, İbrahim aut Enthalten in Wireless personal communications Springer US, 1994 114(2020), 4 vom: 31. Mai, Seite 2923-2932 (DE-627)188950273 (DE-600)1287489-9 (DE-576)049958909 0929-6212 nnns volume:114 year:2020 number:4 day:31 month:05 pages:2923-2932 https://doi.org/10.1007/s11277-020-07510-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MKW AR 114 2020 4 31 05 2923-2932 |
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10.1007/s11277-020-07510-z doi (DE-627)OLC2120510601 (DE-He213)s11277-020-07510-z-p DE-627 ger DE-627 rakwb eng 620 VZ Timoçin, Erdinç verfasserin aut The Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the $ B_{Z} $ Component of Interplanetary Magnetic Field 2020 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, LLC, part of Springer Nature 2020 Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ_{1} $), Hall conductivity ($ σ_{2} $) data calculated for Rome (41.8° N, 12.5° E); Juliusruh (54.6° N, 13.4° E); Uppsala (59.8° N, 17.6° E); Lycksele (64.7° N, 18.8° E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the $ B_{Z} $ component. From the analysis results it is observed that the turnings in the $ B_{Z} $ component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the $ B_{Z} $ component increases all conductivities while the northward turnings of the $ B_{Z} $ component decreases all conductivities. The effect on the conductivities of the changes in the $ B_{Z} $ component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the $ B_{Z} $ component as latitude increase. Ionosphere Ionospheric conductivities Interplanetary magnetic field Superposed epoch analysis Yeşil, Ali aut Ünal, İbrahim aut Enthalten in Wireless personal communications Springer US, 1994 114(2020), 4 vom: 31. Mai, Seite 2923-2932 (DE-627)188950273 (DE-600)1287489-9 (DE-576)049958909 0929-6212 nnns volume:114 year:2020 number:4 day:31 month:05 pages:2923-2932 https://doi.org/10.1007/s11277-020-07510-z lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MKW AR 114 2020 4 31 05 2923-2932 |
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Timoçin, Erdinç |
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10.1007/s11277-020-07510-z |
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620 |
| title_sort |
the responses of ionospheric conductivities on the mid-latitudes to changes in the $ b_{z} $ component of interplanetary magnetic field |
| title_auth |
The Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the $ B_{Z} $ Component of Interplanetary Magnetic Field |
| abstract |
Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ_{1} $), Hall conductivity ($ σ_{2} $) data calculated for Rome (41.8° N, 12.5° E); Juliusruh (54.6° N, 13.4° E); Uppsala (59.8° N, 17.6° E); Lycksele (64.7° N, 18.8° E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the $ B_{Z} $ component. From the analysis results it is observed that the turnings in the $ B_{Z} $ component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the $ B_{Z} $ component increases all conductivities while the northward turnings of the $ B_{Z} $ component decreases all conductivities. The effect on the conductivities of the changes in the $ B_{Z} $ component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the $ B_{Z} $ component as latitude increase. © Springer Science+Business Media, LLC, part of Springer Nature 2020 |
| abstractGer |
Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ_{1} $), Hall conductivity ($ σ_{2} $) data calculated for Rome (41.8° N, 12.5° E); Juliusruh (54.6° N, 13.4° E); Uppsala (59.8° N, 17.6° E); Lycksele (64.7° N, 18.8° E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the $ B_{Z} $ component. From the analysis results it is observed that the turnings in the $ B_{Z} $ component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the $ B_{Z} $ component increases all conductivities while the northward turnings of the $ B_{Z} $ component decreases all conductivities. The effect on the conductivities of the changes in the $ B_{Z} $ component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the $ B_{Z} $ component as latitude increase. © Springer Science+Business Media, LLC, part of Springer Nature 2020 |
| abstract_unstemmed |
Abstract In this study, we investigate the response of the ionospheric conductivities on the middle latitudes to the southward and northward turnings of the $ B_{Z} $ component of the interplanetary magnetic field (IMF). For this purpose, parallel conductivity ($ σ_{0} $), Pedersen conductivity ($ σ_{1} $), Hall conductivity ($ σ_{2} $) data calculated for Rome (41.8° N, 12.5° E); Juliusruh (54.6° N, 13.4° E); Uppsala (59.8° N, 17.6° E); Lycksele (64.7° N, 18.8° E) during the 22nd solar cycle are examined. The superposed epoch analysis method is used to investigate the response of the conductivities to the southward and northward turnings of the $ B_{Z} $ component. From the analysis results it is observed that the turnings in the $ B_{Z} $ component of the IMF have significant effect on all conductivities. At the event moment (zero time), the southward turnings of the $ B_{Z} $ component increases all conductivities while the northward turnings of the $ B_{Z} $ component decreases all conductivities. The effect on the conductivities of the changes in the $ B_{Z} $ component occurs before about 18 h from the event moment, and this effect disappears after about 24 h from the event moment. Furthermore, all of ionospheric conductivities shows or does less reaction to changes in the $ B_{Z} $ component as latitude increase. © Springer Science+Business Media, LLC, part of Springer Nature 2020 |
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The Responses of Ionospheric Conductivities on the Mid-Latitudes to Changes in the $ B_{Z} $ Component of Interplanetary Magnetic Field |
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Yeşil, Ali Ünal, İbrahim |
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