Conjugate observations of the day-side reconnection electric field: A GEM boundary layer campaign

被引:34
作者
Pinnock, M [1 ]
Rodger, AS
Baker, KB
Lu, G
Hairston, M
机构
[1] British Antarctic Survey, NERC, Cambridge CB3 0ET, England
[2] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[3] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[4] Univ Texas, Ctr Space Sci, Richardson, TX 75083 USA
来源
ANNALES GEOPHYSICAE-ATMOSPHERES HYDROSPHERES AND SPACE SCIENCES | 1999年 / 17卷 / 04期
基金
美国国家科学基金会; 美国国家航空航天局; 英国自然环境研究理事会;
关键词
ionosphere (plasma convection; polar; ionosphere); magnetospheric physics (magnetosphere-ionosphere interactions);
D O I
10.1007/s00585-999-0443-4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Data from HF-radars are used to make the first simultaneous conjugate measurements of the dayside reconnection electric field. A period of 4 h around local magnetic noon are studied during a geospace environment modeling (GEM) boundary layer campaign. The interplanetary magnetic field (IMF) was southward whilst the eastward component (By) was variable. The flow patterns derived from the radar data show the expected conjugate asymmetries associated with IMF \By\ > 0. High-time resolution data (50 and 100 s) enable the flow of plasma across the open/closed field line boundary (the separatrix) to be studied in greater detail than in previous work. The latitude of the separatrix follows the same general trend in both hemispheres but shows a hemispherical difference of 4 degrees, with the summer cusp at higher latitude, as expected from dipole tilt considerations. However, the short-time scale motion of the separatrix cannot be satisfactorily resolved within the best resolution (300 m s(-1)) of the experiment. The orientation of the separatrix with respect to magnetic latitude is found to follow the same trend in both hemispheres and qualitatively fits that predicted by a model auroral oval. It shows no correlation with IMF By. However, the degree of tilt in the Northern (summer) Hemisphere is found to be significantly greater than that given by the model oval. The convection pattern data show that the meridian at which throat flow occurs is different in the two hemispheres and is controlled by IMF By, in agreement with empirically derived convection patterns and theoretical models. The day-side reconnection electric field values are largest when the radar's meridian is in the throat flow or Parry afternoon flow regions. In the morning or afternoon convection cells, the reconnection electric field tends to zero away from the throat flow region. The reconnection electric field observed in the throat flow region is bursty in nature.
引用
收藏
页码:443 / 454
页数:12
相关论文
共 40 条
[1]   HF radars: Multifrequency study of refraction effects and localization of scattering [J].
Andre, R ;
Hanuise, C ;
Villain, JP ;
Cerisier, JC .
RADIO SCIENCE, 1997, 32 (01) :153-168
[2]  
Baker K.B., 1989, EOS T AM GEOPHYS UNI, 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]   HF RADAR SIGNATURES OF THE CUSP AND LOW-LATITUDE BOUNDARY-LAYER [J].
BAKER, KB ;
DUDENEY, JR ;
GREENWALD, RA ;
PINNOCK, M ;
NEWELL, PT ;
RODGER, AS ;
MATTIN, N ;
MENG, CI .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1995, 100 (A5) :7671-7695
[5]   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
[6]   HF-radar observations of the dayside magnetic merging rate: A Geospace Environment Modeling boundary layer campaign study [J].
Baker, KB ;
Rodger, AS ;
Lu, G .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1997, 102 (A5) :9603-9617
[7]   COMPRESSED GEOMAGNETIC-FIELD AS A FUNCTION OF DIPOLE TILT [J].
CHOE, JY ;
BEARD, DB .
PLANETARY AND SPACE SCIENCE, 1974, 22 (04) :595-608
[8]   CAN IONOSPHERE REGULATE MAGNETOSPHERIC CONVECTION [J].
CORONITI, FV ;
KENNEL, CF .
JOURNAL OF GEOPHYSICAL RESEARCH, 1973, 78 (16) :2837-2851
[9]  
COWLEY SWH, 1992, ANN GEOPHYS, V10, P103
[10]   DEPENDENCE OF CONVECTIVE FLOWS AND PARTICLE-PRECIPITATION IN THE HIGH-LATITUDE DAYSIDE IONOSPHERE ON THE X AND Y COMPONENTS OF THE INTERPLANETARY MAGNETIC-FIELD [J].
COWLEY, SWH ;
MORELLI, JP ;
LOCKWOOD, M .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1991, 96 (A4) :5557-5564