First results from the RAPID imaging energetic particle spectrometer on board Cluster

被引:142
作者
Wilken, B
Daly, PW
Mall, U [1 ]
Aarsnes, K
Baker, DN
Belian, RD
Blake, JB
Borg, H
Büchner, J
Carter, M
Fennell, JF
Friedel, R
Fritz, TA
Gliem, F
Grande, M
Kecskemety, K
Kettmann, G
Korth, A
Livi, S
McKenna-Lawlor, S
Mursula, K
Nikutowski, B
Perry, CH
Pu, ZY
Roeder, J
Reeves, GD
Sarris, ET
Sandahl, I
Soraas, F
Woch, J
Zong, QG
机构
[1] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany
[2] Univ Bergen, N-5007 Bergen, Norway
[3] LASP, Boulder, CO 80309 USA
[4] LANL, Los Alamos, NM 87545 USA
[5] Aerosp Corp, Los Angeles, CA 90009 USA
[6] IRF, S-90187 Umea, Sweden
[7] RAL, Didcot OX1 10QX, Oxon, England
[8] Boston Univ, Boston, MA 02215 USA
[9] IDA, D-38106 Braunschweig, Germany
[10] KFKI, H-1525 Budapest 114, Hungary
[11] NUI, Maynooth, Kildare, Ireland
[12] Univ Oulu, Oulu 90571, Finland
[13] Peking Univ, Beijing 100871, Peoples R China
[14] Univ Thrace, Xanthi, Greece
[15] IRF, S-98128 Kiruna C, Sweden
关键词
magnetospheric physics; energetic particles; trapped; magnetopause; cusp and boundary layers; magnetosheath;
D O I
10.5194/angeo-19-1355-2001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The advanced energetic particle spectrometer RAPID on board Cluster can provide a complete description of the relevant particle parameters velocity, V, and atomic mass, A, over an energy range from 30 keV up to 1.5 MeV. We present the first measurements taken by RAPID during the commissioning and the early operating phases. The orbit on 14 January 2001, when Cluster was travelling from a perigee near dawn northward across the pole towards an apogee in the solar wind, is used to demonstrate the capabilities of RAPID in investigating a wide variety of particle populations. RAPID, with its unique capability of measuring the complete angular distribution of energetic particles, allows for the simultaneous measurements of local density gradients, as reflected in the anisotropies of 90degrees particles and the remote sensing of changes in the distant field line topology, as manifested in the variations of loss cone properties. A detailed discussion of angle-angle plots shows considerable differences in the structure of the boundaries between the open and closed field lines on the nightside fraction of the pass and the magnetopause crossing. The 3 March 2001 encounter of Cluster with an FTE just outside the magnetosphere is used to show the first structural plasma investigations of an FTE by energetic multi-spacecraft observations.
引用
收藏
页码:1355 / 1366
页数:12
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