DEPENDENCE OF CONVECTIVE FLOWS AND PARTICLE-PRECIPITATION IN THE HIGH-LATITUDE DAYSIDE IONOSPHERE ON THE X AND Y COMPONENTS OF THE INTERPLANETARY MAGNETIC-FIELD

被引:268
作者
COWLEY, SWH [1 ]
MORELLI, JP [1 ]
LOCKWOOD, M [1 ]
机构
[1] RUTHERFORD APPLETON LAB, DIDCOT OX11 0QX, OXON, ENGLAND
关键词
D O I
10.1029/90JA02063
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The asymmetries in the convective flows, current systems, and particle precipitation in the high-latitude dayside ionosphere which are related to the equatorial plane components of the interplanetary magnetic field (IMF) are discussed in relation to the results of several recent observational studies. It is argued that all of the effects reported to date which are ascribed to the y component of the IMF can be understood, at least qualitatively, in terms of a simple theoretical picture in which the effects result from the stresses exerted on the magnetosphere consequent on the interconnection of terrestrial and interplanetary fields. In particular, relaxation under the action of these stresses allows, in effect, a partial penetration of the IMF into the magnetospheric cavity, such that the sense of the expected asymmetry effects on closed field lines can be understood, to zeroth order, in terms of the "dipole plus uniform field" model. In particular, in response to IMF By, the dayside cusp should be displaced in longitude about noon in the same sense as By in the northern hemisphere, and in the opposite sense to By in the southern hemisphere, while simultaneously the auroral oval as a whole should be shifted in the dawn-dusk direction in the opposite sense with respect to By. These expected displacements are found to be consistent with recently published observations. Similar considerations lead to the suggestion that the auroral oval may also undergo displacements in the noon-midnight direction which are associated with the x component of the IMF. We show that a previously published study of the position of the auroral oval contains strong initial evidence for the existence of this effect. However, recent results on variations in the latitude of the cusp are more ambiguous. This topic therefore requires further study before definitive conclusions can be drawn.
引用
收藏
页码:5557 / 5564
页数:8
相关论文
共 39 条
[1]  
ATKINSON G, 1972, MAGNETOSPHERE IONOSP, P203
[2]   IMF BY-DEPENDENT PLASMA-FLOW AND BIRKELAND CURRENTS IN THE DAYSIDE MAGNETOSPHERE .1. DYNAMICS EXPLORER OBSERVATIONS [J].
BURCH, JL ;
REIFF, PH ;
MENIETTI, JD ;
HEELIS, RA ;
HANSON, WB ;
SHAWHAN, SD ;
SHELLEY, EG ;
SUGIURA, M ;
WEIMER, DR ;
WINNINGHAM, JD .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1985, 90 (NA2) :1577-+
[3]   INTENSITY DISTRIBUTION OF DAYSIDE POLAR SOFT ELECTRON-PRECIPITATION AND THE IMF [J].
CANDIDI, M ;
KROEHL, HW ;
MENG, CI .
PLANETARY AND SPACE SCIENCE, 1983, 31 (05) :489-498
[4]   EVIDENCE OF THE INFLUENCE OF THE INTERPLANETARY MAGNETIC-FIELD AZIMUTHAL COMPONENT ON POLAR CUSP CONFIGURATION [J].
CANDIDI, M ;
MASTRANTONIO, G ;
ORSINI, S ;
MENG, CI .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1989, 94 (A10) :13585-13591
[5]   QUALITATIVE STUDY OF RECONNECTION BETWEEN EARTHS MAGNETIC-FIELD AND AN INTERPLANETARY FIELD OF ARBITRARY ORIENTATION [J].
COWLEY, SWH .
RADIO SCIENCE, 1973, 8 (11) :903-913
[6]   MAGNETOSPHERIC ASYMMETRIES ASSOCIATED WITH THE Y-COMPONENT OF THE IMF [J].
COWLEY, SWH .
PLANETARY AND SPACE SCIENCE, 1981, 29 (01) :79-96
[7]   OBSERVATION OF AN IMF SECTOR EFFECT IN THE Y-MAGNETIC FIELD COMPONENT AT GEOSTATIONARY ORBIT [J].
COWLEY, SWH ;
HUGHES, WJ .
PLANETARY AND SPACE SCIENCE, 1983, 31 (01) :73-90
[8]   THE IMPACT OF RECENT OBSERVATIONS ON THEORETICAL UNDERSTANDING OF SOLAR-WIND - MAGNETOSPHERE INTERACTIONS [J].
COWLEY, SWH .
JOURNAL OF GEOMAGNETISM AND GEOELECTRICITY, 1986, 38 (11) :1223-1256
[10]  
COWLEY SWH, 1984, ACHIEVEMENTS IMS ESA, V217, P483