Abstract:An unseasonal equatorial plasma bubble (EPB) event over South‐East Asia was observed on July 22, 2014 that has not been studied before. An investigation into this event is presented with the 26th July, 2014 as a comparison, non‐bubble day. The 22nd July EPB event occurred in the late post‐sunset sector and was associated with a small upward plasma drift. This event was highlighted using a new filter on the SCINDA S4 data. Ionosonde data show that sporadic E was present during the growth period for the EPB even… Show more
“…Many papers have employed the use of GPS ground station data, UHF ground station data, ionosonde data, and/or Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) Radio Occultation (RO) data. The results in Currie et al (2021) showed a clear example of an EPB that was missed in GPS ground data in previous studies. Further analysis of the data to include low elevation angles highlighted the event, and other data sets were used to verify the presence of other EPB indicators, confirming that the enhanced scintillation was not contamination from multipath effects.…”
Section: Introductionmentioning
confidence: 68%
“…The results in Currie et al. (2021) showed a clear example of an EPB that was missed in GPS ground data in previous studies. Further analysis of the data to include low elevation angles highlighted the event, and other data sets were used to verify the presence of other EPB indicators, confirming that the enhanced scintillation was not contamination from multipath effects.…”
Section: Introductionmentioning
confidence: 88%
“…The scintillation data are provided as an S4 index. These S4 data have been used for EPB detection in the post sunset ionosphere (e.g., Carter et al, 2013Carter et al, , 2018Currie et al, 2021). The global coverage of S4 data provided in the "scnLv1" profiles extends ground-based measurements to provide a global scintillation database.…”
Section: Methodsmentioning
confidence: 99%
“…The best-case scenario for calculating occurrence comes from having data every day that clearly and reliably shows an event or no event. Currie et al (2021) highlights the importance of detecting events that may be missed in standard data processing techniques but applies the concept to identifying case studies of unseasonal events. However, the same is true if a complete understanding of climatology and the factors affecting climatology are to be understood.…”
The Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) Radio Occultation data has been previously used as a way of investigating the climatology of Equatorial Plasma Bubbles (EPB). These low‐density regions can cause random phase and amplitude scintillation of satellite signals and forecasting these is an important priority in the space physics community. The ability to build useful forecasting models depends on the underlying data sets used in testing and validating these models. Correctly identifying days of EPB activity is important, but statistical studies using large data sets require the use of automated detection methods. Many of these detection methods heavily reduce data sets by removing unfavorable data, such as COSMIC profiles where the maximum scintillation occurs in the E region. This study presents a new F region s4max9sec index that can be used to study the presence of F region scintillation without excluding profiles that exhibit E region scintillation. The new index is shown to decrease EPB occurrence through the increase in available data, and is also shown to detect EPB events previously excluded from climatological studies. Calculation of the climatology using the new index is shown to resolve some differences that exist in the EPB climatology literature, particularly the location of the maximum scintillation occurrence during the equinox seasons. The use of this index is highlighted as a potential for studying F region scintillation in the presence of E region scintillation; an area of research that needs to be expanded for a complete understanding of EPBs.
“…Many papers have employed the use of GPS ground station data, UHF ground station data, ionosonde data, and/or Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) Radio Occultation (RO) data. The results in Currie et al (2021) showed a clear example of an EPB that was missed in GPS ground data in previous studies. Further analysis of the data to include low elevation angles highlighted the event, and other data sets were used to verify the presence of other EPB indicators, confirming that the enhanced scintillation was not contamination from multipath effects.…”
Section: Introductionmentioning
confidence: 68%
“…The results in Currie et al. (2021) showed a clear example of an EPB that was missed in GPS ground data in previous studies. Further analysis of the data to include low elevation angles highlighted the event, and other data sets were used to verify the presence of other EPB indicators, confirming that the enhanced scintillation was not contamination from multipath effects.…”
Section: Introductionmentioning
confidence: 88%
“…The scintillation data are provided as an S4 index. These S4 data have been used for EPB detection in the post sunset ionosphere (e.g., Carter et al, 2013Carter et al, , 2018Currie et al, 2021). The global coverage of S4 data provided in the "scnLv1" profiles extends ground-based measurements to provide a global scintillation database.…”
Section: Methodsmentioning
confidence: 99%
“…The best-case scenario for calculating occurrence comes from having data every day that clearly and reliably shows an event or no event. Currie et al (2021) highlights the importance of detecting events that may be missed in standard data processing techniques but applies the concept to identifying case studies of unseasonal events. However, the same is true if a complete understanding of climatology and the factors affecting climatology are to be understood.…”
The Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) Radio Occultation data has been previously used as a way of investigating the climatology of Equatorial Plasma Bubbles (EPB). These low‐density regions can cause random phase and amplitude scintillation of satellite signals and forecasting these is an important priority in the space physics community. The ability to build useful forecasting models depends on the underlying data sets used in testing and validating these models. Correctly identifying days of EPB activity is important, but statistical studies using large data sets require the use of automated detection methods. Many of these detection methods heavily reduce data sets by removing unfavorable data, such as COSMIC profiles where the maximum scintillation occurs in the E region. This study presents a new F region s4max9sec index that can be used to study the presence of F region scintillation without excluding profiles that exhibit E region scintillation. The new index is shown to decrease EPB occurrence through the increase in available data, and is also shown to detect EPB events previously excluded from climatological studies. Calculation of the climatology using the new index is shown to resolve some differences that exist in the EPB climatology literature, particularly the location of the maximum scintillation occurrence during the equinox seasons. The use of this index is highlighted as a potential for studying F region scintillation in the presence of E region scintillation; an area of research that needs to be expanded for a complete understanding of EPBs.
“…First, it is worth mentioning that a moderate geomagnetic storm occurred in the late hours of 14 January, with Dst reaching −91 nT and Kp reaching 6- (Le et al, 2022). A useful way to analyze temporal changes in ionograms is by representing the data in a format similar to a "range-time-intensity" plot (Carter et al, 2018;Currie et al, 2021;Pradipta et al, 2015). Instead of using total power, Pradipta et al (2015) integrated over the dBm amplitudes across all sounding frequencies, effectively creating a sum of digitized echoes.…”
The Hunga Tonga Volcano eruption launched a myriad of atmospheric waves that have been observed to travel around the world several times. These waves generated traveling ionospheric disturbances (TIDs) in the ionosphere, which are known to adversely impact radio applications such as Global Navigation Satellite Systems (GNSS). One such GNSS application is Precise Point Positioning (PPP), which can achieve cm‐level accuracy using a single receiver, following a typical convergence time of 30 min to 1 hr. A network of ionosondes located throughout the Australian region were used in combination with GNSS receivers to explore the impacts of the Hunga Tonga Volcano eruption on the ionosphere and what subsequent impacts they had on PPP. It is shown that PPP accuracy was not significantly impacted by the arrival of the TIDs and Spread‐F, provided that PPP convergence had already been achieved. However, when the PPP algorithm was initiated from a cold start either shortly before or after the TID arrivals, the convergence times were significantly longer. GNSS stations in northeastern Australia experienced increases in convergence time of more than 5 hr. Further analysis reveals increased convergence times to be caused by a super equatorial plasma bubble (EPB), the largest observed over Australia to date. The EPB structure was found to be ∼42 TECU deep and ∼300 km across, traveling eastwards at 30 m/s. The Hunga Tonga Volcano eruption serves as an excellent example of how ionospheric variability can impact real‐world applications and the challenges associated with modeling the ionosphere to support GNSS.
Equatorial plasma bubbles (EPBs) occur frequently in low-latitude areas and have a non-negligible impact on navigation satellite signals. To systematically analyze the effects of a single EPB event on multi-frequency signals of GPS, Galileo, GLONASS, and BDS, all-sky airglow images over South China are jointly used to visually determine the EPB structure and depletion degree. The results reveal that scintillations, or GNSS signal fluctuations, are directly linked to EPBs and that the intensity of scintillation is positively correlated with the airglow depletion intensity. The center of the airglow depletion often corresponds to stronger GNSS scintillation, while the edge of the bubble, which is considered to have the largest density gradient, corresponds to relatively smaller scintillation instead. This work also systematically analyzes the responses of multi-constellation and multi-frequency signals to EPBs. The results show that the L2 and L5 frequencies are more susceptible than the L1 frequency is. For different constellations, Galileo’s signal has the best tracking stability during an EPB event compared with GPS, GLONASS, and BDS. The results provide a reference for dual-frequency signal selection in precise positioning or TEC calculation, that is, L1C and L2L for GPS, L1C and L5Q for Galileo, L1P and L2C for GLONASS, and L1P and L5P for BDS. Notably, BDS-2 is significantly weaker than BDS-3. And inclined geosynchronous orbit (IGSO) satellites have abnormal data error rates, which should be related to the special signal path trajectory of the IGSO satellite.
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