Abstract
Benefiting from the special design of BeiDou Navigation Satellite System (BDS) constellation, its Geostationary Earth Orbit (GEO) satellites observations can provide favorable conditions to investigate the ionospheric plasma bubble at low latitudes. This study proposes using BDS GEO Rate of Total Electron Content Index observations to analyze the equatorial plasma bubble characteristics. We use GEO satellites instead of ground-based GNSS stations as a reference and compare the onset time of plasma bubbles observed by different GEO satellites, i.e., the reference GEO, the west and east GEO satellites, during geomagnetically quiet days, and determine plasma bubbles that are generated locally or drifted from elsewhere. According to this strategy, it is found that there is a significant difference in the occurrence rates of plasma bubbles generated locally over two closely located stations, i.e., LALX (18.19 °N, 104.98 °E; geomagnetic latitude: 11.31 °N) and YONG (16.83 °N, 112.34 °E; geomagnetic latitude: 9.96 °N) during the whole year of 2014. Statistical results indicate that during March and September equinoxes, the occurrence rates of plasma bubbles generated locally at the eastern station YONG are 52% and 34%, while at the western station LALX, they are only 34% and 25%. Further analysis reveals a close relationship between the higher bubble generation rates and the active atmospheric inter-tropical convergence zone.
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Data availability
BDS data from stations LALX and YONG can be obtained at the website of the Crustal Movement Observation Network of China (www.neis.org.cn/) or by contacting the corresponding author. BDS data from station SIN1 can be downloaded at the International GNSS Service link (ftp://cddis.gsfc.nasa.gov/). The OLR data are provided by the National Oceanic and Atmospheric Administration (www.esrl.noaa.gov/psd/data/gridded/data.interp_OLR.html#plot). The Kp and Dst data are released by the NASA’s OMNIweb (https://omniweb.gsfc.nasa.gov/form/dx1.html).
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Acknowledgements
This work is supported by the National Key Research and Development Program of China (Nos. 2018YFC1503502, 2017YFB0503401, and 2016YFB0501802), the National Natural Science Foundation of China (No. 41704032), the Fundamental Research Funds for the Central Universities, China University of Geosciences (Wuhan) (No. CUG2106354), the Fundamental Research Funds for the Central Universities (Nos. 2042019kf0222 and 2042019kf0031), and the Specialized Research Fund for Key Laboratory of Earth and Planetary Physics (DQXX2021-11). The authors are also grateful to the two reviewers for their constructive comments regarding to this paper.
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Luo, X., Lou, Y., Gu, S. et al. Local ionospheric plasma bubble revealed by BDS Geostationary Earth Orbit satellite observations. GPS Solut 25, 117 (2021). https://doi.org/10.1007/s10291-021-01155-6
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DOI: https://doi.org/10.1007/s10291-021-01155-6