Swarm in situ observations of F region polar cap patches created by cusp precipitation

被引:64
作者
Goodwin, L. V. [1 ]
Iserhienrhien, B. [1 ]
Miles, D. M. [2 ]
Patra, S. [3 ]
van der Meeren, C. [4 ]
Buchert, S. C. [5 ]
Burchill, J. K. [6 ]
Clausen, L. B. N. [3 ]
Knudsen, D. J. [6 ]
McWilliams, K. A. [1 ]
Moen, J. [3 ]
机构
[1] Univ Saskatchewan, Dept Phys & Engn Phys, Inst Space & Atmospher Studies, Saskatoon, SK, Canada
[2] Univ Alberta, Dept Phys, Edmonton, AB, Canada
[3] Univ Oslo, Dept Phys, Oslo, Norway
[4] Univ Bergen, Dept Phys & Technol, Birkeland Ctr Space Sci, Bergen, Norway
[5] Swedish Inst Space Phys, Uppsala, Sweden
[6] Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
HIGH-LATITUDE IONOSPHERE; HF RADAR BACKSCATTER; MAGNETOPAUSE RECONNECTION; ELECTRON-DENSITY; MAGNETIC-FIELD; PLASMA; CONVECTION; ORIGIN; IRREGULARITIES; SCINTILLATION;
D O I
10.1002/2014GL062610
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
High-resolution in situ measurements from the three Swarm spacecraft, in a string-of-pearls configuration, provide new insights about the combined role of flow channel events and particle impact ionization in creating F region electron density structures in the northern Scandinavian dayside cusp. We present a case of polar cap patch formation where a reconnection-driven low-density relative westward flow channel is eroding the dayside solar-ionized plasma but where particle impact ionization in the cusp dominates the initial plasma structuring. In the cusp, density features are observed which are twice as dense as the solar-ionized background. These features then follow the polar cap convection and become less structured and lower in amplitude. These are the first in situ observations tracking polar cap patch evolution from creation by plasma transport and enhancement by cusp precipitation, through entrainment in the polar cap flow and relaxation into smooth patches as they approach the nightside auroral oval.
引用
收藏
页码:996 / 1003
页数:8
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