Pitch angle distribution of suprathermal electrons behind dipolarization fronts: A statistical overview

被引:166
作者
Fu, H. S. [1 ]
Khotyaintsev, Y. V. [1 ]
Vaivads, A. [1 ]
Andre, M. [1 ]
Sergeev, V. A. [2 ]
Huang, S. Y. [1 ]
Kronberg, E. A. [3 ]
Daly, P. W. [3 ]
机构
[1] Swedish Inst Space Phys, SE-75121 Uppsala, Sweden
[2] St Petersburg State Univ, Earth Phys Dept, St Petersburg, Russia
[3] Max Planck Inst Solar Syst Res, Katlenburg Lindau, Germany
基金
瑞典研究理事会;
关键词
PLASMA SHEET; CLUSTER; ACCELERATION; SUBSTORM; ONSET; EVENT; IMF;
D O I
10.1029/2012JA018141
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine the pitch angle distribution (PAD) of suprathermal electrons (> 40 keV) inside the flux pileup regions (FPRs) that are located behind the dipolarization fronts (DFs), in order to better understand the particle energization mechanisms operating therein. The 303 earthward-propagating DFs observed during 9 years (2001-2009) by Cluster 1 have been analyzed and divided into two groups according to the differential fluxes of the > 40 keV electrons inside the FPR. One group, characterized by the low flux (F < 500/cm(2) , s . sr . keV), consists of 153 events and corresponds to a broad distribution of IMF Bz components. The other group, characterized by the high flux (F >= 500/cm(2) . s . sr . keV), consists of 150 events and corresponds to southward IMF Bz components. Only the high-flux group is considered to investigate the PAD of the > 40 keV electrons as the low-flux situation may lead to large uncertainties in computing the anisotropy factor that is defined as A = F-perpendicular to/F-parallel to - 1 for F-perpendicular to > F-parallel to, and A = -F-parallel to/F-perpendicular to + 1 for F-perpendicular to < F-parallel to. We find that, among the 150 events, 46 events have isotropic distribution (vertical bar A vertical bar <= 0.5); 60 events have perpendicular distribution (A > 0.5), and 44 events have field-aligned distribution inside the FPR (A < -0.5). The perpendicular distribution appears mainly inside the growing FPR, where the flow velocity is increasing and the local flux tube is compressed. The field-aligned distribution occurs mainly inside the decaying FPR, where the flow velocity is decreasing and the local flux tube is expanding. Inside the steady FPR, we observed primarily the isotropic distribution of suprathermal electrons. This statistical result confirms the previous case study and gives an overview of the PAD of suprathermal electrons behind DFs. Citation: Fu, H. S., Y. V. Khotyaintsev, A. Vaivads, M. Andre, V. A. Sergeev, S. Y. Huang, E. A. Kronberg, and P. W. Daly (2012), Pitch angle distribution of suprathermal electrons behind dipolarization fronts: A statistical overview, J. Geophys. Res., 117, A12221, doi:10.1029/2012JA018141.
引用
收藏
页数:9
相关论文
共 47 条
[1]   BURSTY BULK FLOWS IN THE INNER CENTRAL PLASMA SHEET [J].
ANGELOPOULOS, V ;
BAUMJOHANN, W ;
KENNEL, CF ;
CORONITI, FV ;
KIVELSON, MG ;
PELLAT, R ;
WALKER, RJ ;
LUHR, H ;
PASCHMANN, G .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1992, 97 (A4) :4027-4039
[2]   Multi-spacecraft observation of plasma dipolarization/injection in the inner magnetosphere [J].
Apatenkov, S. V. ;
Sergeev, V. A. ;
Kubyshkina, M. V. ;
Nakamura, R. ;
Baumjohann, W. ;
Runov, A. ;
Alexeev, I. ;
Fazakerley, A. ;
Frey, H. ;
Muhlbachler, S. ;
Daly, P. W. ;
Sauvaud, J.-A. ;
Ganushkina, N. ;
Pulkkinen, T. ;
Reeves, G. D. ;
Khotyaintsev, Y. .
ANNALES GEOPHYSICAE, 2007, 25 (03) :801-814
[3]   Adiabatic electron heating in the magnetotail current sheet: Cluster observations and analytical models [J].
Artemyev, A. V. ;
Petrukovich, A. A. ;
Nakamura, R. ;
Zelenyi, L. M. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2012, 117
[4]   Electron acceleration signatures in the magnetotail associated with substorms [J].
Asano, Y. ;
Shinohara, I. ;
Retino, A. ;
Daly, P. W. ;
Kronberg, E. A. ;
Takada, T. ;
Nakamura, R. ;
Khotyaintsev, Y. V. ;
Vaivads, A. ;
Nagai, T. ;
Baumjohann, W. ;
Fazakerley, A. N. ;
Owen, C. J. ;
Miyashita, Y. ;
Lucek, E. A. ;
Reme, H. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2010, 115
[5]   Observations and simulations of non-local acceleration of electrons in magnetotail magnetic reconnection events [J].
Ashour-Abdalla, Maha ;
El-Alaoui, Mostafa ;
Goldstein, Melvyn L. ;
Zhou, Meng ;
Schriver, David ;
Richard, Robert ;
Walker, Raymond ;
Kivelson, Margaret G. ;
Hwang, Kyoung-Joo .
NATURE PHYSICS, 2011, 7 (04) :360-365
[6]   Statistical properties of tail plasma sheet electrons above 40 keV [J].
Asnes, A. ;
Friedel, R. W. H. ;
Lavraud, B. ;
Reeves, G. D. ;
Taylor, M. G. G. T. ;
Daly, P. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2008, 113 (A3)
[7]   AVERAGE PLASMA PROPERTIES IN THE CENTRAL PLASMA SHEET [J].
BAUMJOHANN, W ;
PASCHMANN, G ;
CATTELL, CA .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1989, 94 (A6) :6597-6606
[8]   Particle Acceleration in the Magnetotail and Aurora [J].
Birn, J. ;
Artemyev, A. V. ;
Baker, D. N. ;
Echim, M. ;
Hoshino, M. ;
Zelenyi, L. M. .
SPACE SCIENCE REVIEWS, 2012, 173 (1-4) :49-102
[9]   Bursty bulk flows and dipolarization in MHD simulations of magnetotail reconnection [J].
Birn, J. ;
Nakamura, R. ;
Panov, E. V. ;
Hesse, M. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2011, 116
[10]   The superdense plasma sheet: Plasmaspheric origin, solar wind origin, or ionospheric origin? [J].
Borovsky, JE ;
Thomsen, MF ;
McComas, DJ .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1997, 102 (A10) :22089-22097