THE DETERMINATION OF TIME-STATIONARY 2-DIMENSIONAL CONVECTION PATTERNS WITH SINGLE-STATION RADARS

被引:53
作者
FREEMAN, MP [1 ]
RUOHONIEMI, JM [1 ]
GREENWALD, RA [1 ]
机构
[1] JOHNS HOPKINS UNIV, APPL PHYS LAB, LAUREL, MD 20723 USA
关键词
D O I
10.1029/91JA00445
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
At the present time, most ground-based radar estimations of ionospheric convection use observations from single-station facilities. This approach requires certain assumptions as to the spatial and/or temporal uniformity of the convection. In this paper we present a critical examination of the accuracy of these vector velocity determinations, using realistic modeled flow patterns that are time-stationary but not spatially uniform. We find that under certain circumstances the actual and inferred flow fields show considerable discrepancy, sometimes not even agreeing in the sense of flow direction! Specifically, we show that the natural curvature present in ionospheric convection on varying spatial scales can introduce significant error in the velocity estimate, particularly when the radius of curvature of the flow structure is less than or equal to the radar range to the scattering volume. The presence of flow curvature cannot be detected by radars which determine velocities from measurements in two viewing directions, and it might not be detected by radars using azimuth scanning techniques. Thus we argue that every effort should be made to measure the ionospheric convection by bidirectional or multidirectional observations of a common ionospheric volume and that a synthesis of coherent and incoherent radar observations from different sites is preferable to multidirectional single-station observations using either radar alone. These conclusions are applicable to any Doppler measurement technique and are equally valid for high-latitude wind patterns using Fabry-Perot interferometer techniques.
引用
收藏
页码:15735 / 15749
页数:15
相关论文
共 43 条
[1]   DIURNAL RADIO AURORA VARIATIONS AT 50 MHZ MEASURED BY THE BISTATIC AURORAL RADAR SYSTEM RADARS [J].
ANDRE, D ;
MCNAMARA, AG ;
WALLIS, DD ;
MCINTOSH, BA ;
HUGHES, TJ ;
SOFKO, GJ ;
KOEHLER, JA ;
MCDIARMID, DR ;
PRIKRYL, P ;
WATERMANN, J .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1988, 93 (A8) :8651-8661
[2]  
Baker K. B., 1989, EOS T AGU, V70, P785, DOI DOI 10.1029/89EO00253
[3]   SIMULTANEOUS HF-RADAR AND DMSP OBSERVATIONS OF THE CUSP [J].
BAKER, KB ;
GREENWALD, RA ;
RUOHONIEMI, JM ;
DUDENEY, JR ;
PINNOCK, M ;
NEWELL, PT ;
GREENSPAN, ME ;
MENG, CI .
GEOPHYSICAL RESEARCH LETTERS, 1990, 17 (11) :1869-1872
[4]   A NEW MAGNETIC COORDINATE SYSTEM FOR CONJUGATE STUDIES AT HIGH-LATITUDES [J].
BAKER, KB ;
WING, S .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1989, 94 (A7) :9139-9143
[5]  
BREKKE A, 1977, RADIO SCI, V12, P141, DOI 10.1029/RS012i001p00141
[6]   DIRECT MEASUREMENTS OF PLASMA DRIFT VELOCITIES AT HIGH MAGNETIC LATITUDES [J].
DOUPNIK, JR ;
BANKS, PM ;
BARON, MJ ;
RINO, CL ;
PETRICEKS, J .
JOURNAL OF GEOPHYSICAL RESEARCH, 1972, 77 (22) :4268-+
[7]   STUDIES OF CONJUGATE PLASMA CONVECTION IN THE VICINITY OF THE HARANG DISCONTINUITY [J].
DUDENEY, JR ;
RODGER, AS ;
PINNOCK, M ;
RUOHONIEMI, JM ;
BAKER, KB ;
GREENWALD, RA .
JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS, 1991, 53 (3-4) :249-263
[8]   INTERPLANETARY MAGNETIC FIELD AND AURORAL ZONES [J].
DUNGEY, JW .
PHYSICAL REVIEW LETTERS, 1961, 6 (02) :47-&
[9]   MILLSTONE HILL INCOHERENT-SCATTER OBSERVATIONS OF AURORAL CONVECTION OVER 60-DEGREES LESS-THAN-OR-EQUAL-TO-LAMBDA-LESS-THAN-OR-EQUAL-TO 75-DEGREES .1. OBSERVING AND DATA REDUCTION PROCEDURES [J].
EVANS, JV ;
HOLT, JM ;
WAND, RH .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1979, 84 (NA12) :7059-7074
[10]   LARGE-SCALE PATTERNS OF AURORAL IONOSPHERIC CONVECTION OBSERVED WITH THE CHATANIKA RADAR [J].
FOSTER, JC ;
DOUPNIK, JR ;
STILES, GS .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1981, 86 (NA13) :1357-1371