TY - JOUR
T1 - Worst-Case GPS Scintillations on the Ground Estimated from Radio Occultation Observations of FORMOSAT-3/COSMIC During 2007–2014
AU - Liu, J. Y.
AU - Chen, S. P.
AU - Yeh, W. H.
AU - Tsai, H. F.
AU - Rajesh, P. K.
N1 - Publisher Copyright:
© 2015, Springer Science+Business Media Dordrecht.
PY - 2016/7/1
Y1 - 2016/7/1
N2 - The FORMOSAT-3/COSMIC (F3/C) satellite probes the S4 scintillation index profile of GPS signals by using the radio occultation (RO) technique. In this study, for practical use on the Earth’s surface, a method is developed to convert and integrate the probed RO S4 index, so obtaining the scintillation on the ground. To estimate the worst case, the maximum value on each profile probed by F3/C, which is termed S4max, is isolated. The isolated data are further used to construct the global three-dimensional distributions of S4max for various local times, seasons, solar activities, and locations. The converted S4max for the first time estimates the global distribution of ionospheric scintillations in the GPS L1 band C/A code signal on the ground. The results show that the worst-case scintillations appear within the low-latitude region of ±30°N, peaking around ±20°N magnetic latitude; they begin at 1900 MLT, reach their maximum at 2100 MLT, and vanish by about 0200–0300 MLT. The most pronounced low-latitude scintillation occurs over the South American and African sectors.
AB - The FORMOSAT-3/COSMIC (F3/C) satellite probes the S4 scintillation index profile of GPS signals by using the radio occultation (RO) technique. In this study, for practical use on the Earth’s surface, a method is developed to convert and integrate the probed RO S4 index, so obtaining the scintillation on the ground. To estimate the worst case, the maximum value on each profile probed by F3/C, which is termed S4max, is isolated. The isolated data are further used to construct the global three-dimensional distributions of S4max for various local times, seasons, solar activities, and locations. The converted S4max for the first time estimates the global distribution of ionospheric scintillations in the GPS L1 band C/A code signal on the ground. The results show that the worst-case scintillations appear within the low-latitude region of ±30°N, peaking around ±20°N magnetic latitude; they begin at 1900 MLT, reach their maximum at 2100 MLT, and vanish by about 0200–0300 MLT. The most pronounced low-latitude scintillation occurs over the South American and African sectors.
KW - FORMOSAT-3/COSMIC satellite
KW - Ionospheric scintillation
KW - Radio occultation
KW - S4 index
UR - http://www.scopus.com/inward/record.url?scp=84952944655&partnerID=8YFLogxK
U2 - 10.1007/s10712-015-9355-x
DO - 10.1007/s10712-015-9355-x
M3 - 回顧評介論文
AN - SCOPUS:84952944655
SN - 0169-3298
VL - 37
SP - 791
EP - 809
JO - Surveys in Geophysics
JF - Surveys in Geophysics
IS - 4
ER -