GPS/GLONASS sensing of the neutral atmosphere: Model-independent correction of ionospheric influences

被引:29
作者
Ladreiter, HP [1 ]
Kirchengast, G [1 ]
机构
[1] GRAZ UNIV,INST METEOROL & GEOPHYS,A-8010 GRAZ,AUSTRIA
关键词
D O I
10.1029/96RS01094
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Radio occultation sensing of the terrestrial atmosphere can be performed by using signals from Global Positioning System (GPS) or Global Navigation Satellite System (GLONASS) satellites, which are received by satellites in low Earth orbit. The signal transmitted from a GPS/GLONASS satellite, when occulted, suffers propagation effects in the ionosphere and atmosphere, including carrier and group phase shifts and ray path bending. Those propagation effects give direct information on the refractivity of the medium of occultation. In order to sense the neutral atmosphere only, we have to carefully correct for the ionospheric contribution to the propagation effects whose influences are poorly known at present time. In this paper, we provide a straightforward method for model-independent correction of the ionospheric effects based on the correction of the ionospheric bending angle rather than correction of the optical path lengths, as done by previous studies. Using the presented correction, the accuracy of retrieved temperature profiles of the atmosphere is better than 1 K up to heights of some 55 km during typical ionospheric conditions. The formalism can easily be implemented in on-line analyses of phase data obtained by the radio occultation technique. This promising technique may thus in fact become an extremely valuable tool for supporting climate monitoring as well as weather and climate modeling and prediction.
引用
收藏
页码:877 / 891
页数:15
相关论文
共 17 条
[1]  
Brunner F. K., 1991, Manuscripta Geodaetica, V16, P205
[2]  
Budden K.G., 1985, The Propagation of Radio Waves: The Theory of Radio Waves of Low Power in the Ionosphere and Magnetosphere, V1st ed.
[3]   ATMOSPHERE OF MARS ANALYZED BY INTEGRAL INVERSION OF MARINER 4 OCCULTATION DATA [J].
FJELDBO, G ;
ESHLEMAN.VR .
PLANETARY AND SPACE SCIENCE, 1968, 16 (08) :1035-&
[4]   2-FREQUENCY BISTATIC RADAR-OCCULATATION METHOD FOR STUDY OF PLANETARY IONOSPHERES [J].
FJELDBO, G ;
ESHLEMAN, VR ;
GARRIOTT, OK ;
SMITH, FL .
JOURNAL OF GEOPHYSICAL RESEARCH, 1965, 70 (15) :3701-&
[5]   NEUTRAL ATMOSPHERE OF VENUS AS STUDIED WITH MARINER-V RADIO OCCULTATION EXPERIMENTS [J].
FJELDBO, G ;
KLIORE, AJ ;
ESHLEMEN, VR .
ASTRONOMICAL JOURNAL, 1971, 76 (02) :123-&
[6]   BISTATIC RADAR-OCCULTATION METHOD FOR STUDY OF PLANETARY ATMOSPHERES [J].
FJELDBO, G ;
ESHLEMAN, VR .
JOURNAL OF GEOPHYSICAL RESEARCH, 1965, 70 (13) :3217-+
[7]   Three-dimensional satellite refractive tomography of the atmosphere: Numerical simulation [J].
Gorbunov, ME .
RADIO SCIENCE, 1996, 31 (01) :95-104
[8]  
GORBUNOV ME, 1993, 119 MAXPL I MET
[9]   ACCURACIES OF ATMOSPHERIC PROFILES OBTAINED FROM GPS OCCULATIONS [J].
HARDY, KR ;
HAJJ, GA ;
KURSINSKI, ER .
INTERNATIONAL JOURNAL OF SATELLITE COMMUNICATIONS, 1994, 12 (05) :463-473
[10]  
KING RW, 1985, SURVEYING GPS, P128