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Amplitude scintillation index derived from C/N0 measurements released by common geodetic GNSS receivers operating at 1 Hz
https://orcid.org/0000-0001-6004-5938
Abstract Two widely used scintillation indexes $$ S_{4} $$ and $$ \sigma_{\varphi } $$ are generated by dedicated ionospheric scintillation monitoring receivers (ISMRs), which typically have 50-Hz temporal resolution and thus require substantial memory capabilities. Taking into consideration the huge number of common Global Navigation Satellite System (GNSS) receivers, the derivation of a GNSS receiver-based scintillation index as a supplement to the ISMR indexes is expected to improve the study of ionospheric scintillation. We developed an amplitude scintillation index, $$ S_{{4{\text{c}}}} $$, which is derived from the carrier-to-noise density ratio ($$ C/N_{0} $$) data released by common geodetic GNSS receivers operating at 1-Hz. The reliability of the $$ S_{{4{\text{c}}}} $$ index is compared with the typical scintillation index $$ S_{4} $$ of three ISMRs located in Hong Kong and Brazil. The statistics indicate that during scintillation activity, the correlation coefficient between $$ S_{{4{\text{c}}}} $$ (derived from common receivers) and $$ S_{4} $$ (generated by ISMRs) is generally higher than 0.9. The reliability of $$ S_{{4{\text{c}}}} $$ was also verified based on 1-year observations from two adjacent stations in Hong Kong, which are equipped with Leica GR50 and Septentrio PolaRxS Pro receivers, respectively. Long-term scintillation occurrence ($$ S_{{4{\text{c}}}} $$ > 0.2 vs. $$ S_{4} $$ > 0.2) rates show good agreement between $$ S_{{4{\text{c}}}} $$ and $$ S_{4} $$. In addition, two-dimensional $$ S_{{4{\text{c}}}} $$ maps (1° × 1°) generated by GPS L1 and BDS B1 signals data collected at 117 continuous operation tracking stations in China clearly show post-sunset super plasma bubbles as the source of ionospheric scintillation during the main phase of the intense storm that occurred on September 8, 2017. These results demonstrate the feasibility of using the $$ S_{{4{\text{c}}}} $$ index derived from the large volume of GNSS observations recorded by non-scintillation GNSS receivers for the study and monitoring of ionospheric scintillation.
Amplitude scintillation index derived from C/N0 measurements released by common geodetic GNSS receivers operating at 1 Hz
https://orcid.org/0000-0001-6004-5938
Abstract Two widely used scintillation indexes $$ S_{4} $$ and $$ \sigma_{\varphi } $$ are generated by dedicated ionospheric scintillation monitoring receivers (ISMRs), which typically have 50-Hz temporal resolution and thus require substantial memory capabilities. Taking into consideration the huge number of common Global Navigation Satellite System (GNSS) receivers, the derivation of a GNSS receiver-based scintillation index as a supplement to the ISMR indexes is expected to improve the study of ionospheric scintillation. We developed an amplitude scintillation index, $$ S_{{4{\text{c}}}} $$, which is derived from the carrier-to-noise density ratio ($$ C/N_{0} $$) data released by common geodetic GNSS receivers operating at 1-Hz. The reliability of the $$ S_{{4{\text{c}}}} $$ index is compared with the typical scintillation index $$ S_{4} $$ of three ISMRs located in Hong Kong and Brazil. The statistics indicate that during scintillation activity, the correlation coefficient between $$ S_{{4{\text{c}}}} $$ (derived from common receivers) and $$ S_{4} $$ (generated by ISMRs) is generally higher than 0.9. The reliability of $$ S_{{4{\text{c}}}} $$ was also verified based on 1-year observations from two adjacent stations in Hong Kong, which are equipped with Leica GR50 and Septentrio PolaRxS Pro receivers, respectively. Long-term scintillation occurrence ($$ S_{{4{\text{c}}}} $$ > 0.2 vs. $$ S_{4} $$ > 0.2) rates show good agreement between $$ S_{{4{\text{c}}}} $$ and $$ S_{4} $$. In addition, two-dimensional $$ S_{{4{\text{c}}}} $$ maps (1° × 1°) generated by GPS L1 and BDS B1 signals data collected at 117 continuous operation tracking stations in China clearly show post-sunset super plasma bubbles as the source of ionospheric scintillation during the main phase of the intense storm that occurred on September 8, 2017. These results demonstrate the feasibility of using the $$ S_{{4{\text{c}}}} $$ index derived from the large volume of GNSS observations recorded by non-scintillation GNSS receivers for the study and monitoring of ionospheric scintillation.
Amplitude scintillation index derived from C/N0 measurements released by common geodetic GNSS receivers operating at 1 Hz
https://orcid.org/0000-0001-6004-5938
Abstract Two widely used scintillation indexes $$ S_{4} $$ and $$ \sigma_{\varphi } $$ are generated by dedicated ionospheric scintillation monitoring receivers (ISMRs), which typically have 50-Hz temporal resolution and thus require substantial memory capabilities. Taking into consideration the huge number of common Global Navigation Satellite System (GNSS) receivers, the derivation of a GNSS receiver-based scintillation index as a supplement to the ISMR indexes is expected to improve the study of ionospheric scintillation. We developed an amplitude scintillation index, $$ S_{{4{\text{c}}}} $$, which is derived from the carrier-to-noise density ratio ($$ C/N_{0} $$) data released by common geodetic GNSS receivers operating at 1-Hz. The reliability of the $$ S_{{4{\text{c}}}} $$ index is compared with the typical scintillation index $$ S_{4} $$ of three ISMRs located in Hong Kong and Brazil. The statistics indicate that during scintillation activity, the correlation coefficient between $$ S_{{4{\text{c}}}} $$ (derived from common receivers) and $$ S_{4} $$ (generated by ISMRs) is generally higher than 0.9. The reliability of $$ S_{{4{\text{c}}}} $$ was also verified based on 1-year observations from two adjacent stations in Hong Kong, which are equipped with Leica GR50 and Septentrio PolaRxS Pro receivers, respectively. Long-term scintillation occurrence ($$ S_{{4{\text{c}}}} $$ > 0.2 vs. $$ S_{4} $$ > 0.2) rates show good agreement between $$ S_{{4{\text{c}}}} $$ and $$ S_{4} $$. In addition, two-dimensional $$ S_{{4{\text{c}}}} $$ maps (1° × 1°) generated by GPS L1 and BDS B1 signals data collected at 117 continuous operation tracking stations in China clearly show post-sunset super plasma bubbles as the source of ionospheric scintillation during the main phase of the intense storm that occurred on September 8, 2017. These results demonstrate the feasibility of using the $$ S_{{4{\text{c}}}} $$ index derived from the large volume of GNSS observations recorded by non-scintillation GNSS receivers for the study and monitoring of ionospheric scintillation.
Amplitude scintillation index derived from C/N0 measurements released by common geodetic GNSS receivers operating at 1 Hz
Luo, Xiaomin (author) / Gu, Shengfeng (author) / Lou, Yidong (author) / Cai, Lei (author) / Liu, Zhizhao (author)
Journal of Geodesy ; 94
2020
Article (Journal)
Electronic Resource
English
A method for scintillation characterization using geodetic receivers operating at 1 Hz
| Online Contents | 2017
A method for scintillation characterization using geodetic receivers operating at 1 Hz
| Online Contents | 2017
| Online Contents | 2019