4 CELLS OR 2 - ARE 4 CONVECTION CELLS REALLY NECESSARY

被引:25
作者
REIFF, PH [1 ]
HEELIS, RA [1 ]
机构
[1] UNIV TEXAS, CTR SPACE SCI, RICHARDSON, TX 75083 USA
关键词
D O I
10.1029/93JA01992
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper addresses the question whether a four-cell convection pattern in the polar cap ionosphere is required by observations, or whether the data are fully explainable by a (perhaps highly distorted) two-cell convection pattern. We present convection data from Atmosphere Explorer C, which, if only the flow component in the sunward-antisunward direction were measured, could be explained either as one of two possible distorted two-cell patterns or as a full four-cell pattern. However, neither of the distorted two-cell patterns that are consistent with the sunward-antisunward flow component can be made consistent with the dawn-dusk flow component over the entire spacecraft trajectory, without postulating a severe flow kink and extra field-aligned currents sunward of the spacecraft track. In addition, the zero potential point (which in a four-cell model would mark the division between the two reverse convection cells) also exactly corresponded to the location of the reversal of the east-west component in the flow, a feature predicted from the four-cell model but more difficult to explain in a distorted two-cell model. Because the pattern was repeated on two consecutive passes, time variations can probably be ruled out as a cause of the sunward flow. Between the two northern hemisphere dayside passes, a southern hemisphere nightside pass also showed a region of sunward flow in the polar cap. The fact that in this case the sunward flow was not confined to the dayside also favors a four-cell explanation.
引用
收藏
页码:3955 / 3959
页数:5
相关论文
共 30 条
[1]   HIGH-LATITUDE CONVECTION PATTERNS FOR VARIOUS LARGE-SCALE FIELD-ALIGNED CURRENT CONFIGURATIONS [J].
BLOMBERG, LG ;
MARKLUND, GT .
GEOPHYSICAL RESEARCH LETTERS, 1991, 18 (04) :717-720
[2]   CUSP REGION PARTICLE-PRECIPITATION AND ION CONVECTION FOR NORTHWARD INTER-PLANETARY MAGNETIC-FIELD [J].
BURCH, JL ;
REIFF, PH ;
SPIRO, RW ;
HEELIS, RA ;
FIELDS, SA .
GEOPHYSICAL RESEARCH LETTERS, 1980, 7 (05) :393-396
[3]   POLAR-CAP ELECTRIC-FIELD STRUCTURES WITH A NORTHWARD INTER-PLANETARY MAGNETIC-FIELD [J].
BURKE, WJ ;
KELLEY, MC ;
SAGALYN, RC ;
SMIDDY, M ;
LAI, ST .
GEOPHYSICAL RESEARCH LETTERS, 1979, 6 (01) :21-24
[4]   IONOSPHERIC CONVECTION SIGNATURES AND MAGNETIC-FIELD TOPOLOGY [J].
COLEY, WR ;
HEELIS, RA ;
HANSON, WB ;
REIFF, PH ;
SHARBER, JR ;
WINNINGHAM, JD .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1987, 92 (A11) :12352-12364
[5]  
COWLEY SWH, 1982, PHYSICAL BASIS IONOS
[6]  
DUNGEY JW, 1963, GEOPHYSICS EARTHS EN
[7]   POLAR-CAP CURRENTS FOR DIFFERENT DIRECTIONS OF INTERPLANETARY MAGNETIC-FIELD IN Y-Z PLANE [J].
FRIISCHRISTENSEN, E ;
WILHJELM, J .
JOURNAL OF GEOPHYSICAL RESEARCH, 1975, 80 (10) :1248-1260
[8]  
HEELIS RA, 1982, J GEOPHYS RES-SPACE, V87, P6339, DOI 10.1029/JA087iA08p06339
[9]   IONOSPHERIC CONVECTION SIGNATURES OBSERVED BY DE-2 DURING NORTHWARD INTERPLANETARY MAGNETIC-FIELD [J].
HEELIS, RA ;
REIFF, PH ;
WINNINGHAM, JD ;
HANSON, WB .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1986, 91 (A5) :5817-5830
[10]   HIGH-LATITUDE ION CONVECTION IN THE NIGHTTIME F-REGION [J].
HEELIS, RA ;
HANSON, WB .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1980, 85 (NA5) :1995-2002