The STAFF-DWP wave instrument on the DSP equatorial spacecraft:: description and first results

被引：21

作者：

Cornilieau-Wehrlin, N

Alleyne, HS

Yearby, KH

de Vaux, BD

Meyer, A

Santolík, O

Parrot, M

Belmont, G

Rezeau, L

Le Contel, O

Roux, A

Attié, D

Robert, P

Bouzid, V

Herment, D

Cao, J

机构：

[1] CETP, IPSL, F-78140 Velizy Villacoublay, France

[2] Univ Sheffield, Sheffield S1 3JD, S Yorkshire, England

[3] Fac Math & Phys, CZ-18000 Prague, Czech Republic

[4] LPCE, F-45071 Orleans, France

[5] CETP, IPSL, UPMC, F-78140 Velizy Villacoublay, France

[6] Chinese Acad Sci, CSSAR, Beijing 100080, Peoples R China

来源：

ANNALES GEOPHYSICAE | 2005年 / 23卷 / 08期

关键词：

space plasma physics; instruments and techniques; waves and instabilities; magnetospheric physics; Solar wind-magnetosphere interactions;

D O I：

10.5194/angeo-23-2785-2005

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The STAFF-DWP wave instrument on board the equatorial spacecraft (TC1) of the Double Star Project consists of a combination of 2 instruments which are a heritage of the Cluster mission: the Spatio-Temporal Analysis of Field Fluctuations (STAFF) experiment and the Digital Wave-Processing experiment (DWP). On DSP-TC1 STAFF consists of a three-axis search coil magnetometer, used to measure magnetic fluctuations at frequencies up to 4 kHz and a waveform unit, up to 10 Hz, plus snapshots up to 180 Hz. DWP provides several onboard analysis tools: a complex FFT to fully characterise electromagnetic waves in the frequency range 10 Hz-4 kHz, a particle correlator linked to the PEACE electron experiment, and compression of the STAFF waveform data. The complementary Cluster and TC1 orbits, together with the similarity of the instruments, permits new multi-point studies. The first results show the capabilities of the experiment, with examples in the different regions of the magnetos phere-solar wind system that have been encountered by DSP-TC1 at the beginning of its operational phase. An overview of the different kinds of electromagnetic waves observed on the dayside from perigee to apogee is given, including the different whistler mode waves (hiss, chorus, lion roars) and broad-band ULF emissions. The polarisation and propagation characteristics of intense waves in the vicinity of a bow shock crossing are analysed using the dedicated PRASSADCO tool, giving results compatible with previous studies: the broad-band ULF waves consist of a superimposition of different wave modes, whereas the magnetosheath lion roars are right-handed and propagate close to the magnetic field. An example of a combined Cluster DSP-TC1 magnetopause crossing, is given. This first case study shows that the ULF wave power intensity is higher at low latitude (DSP) than at high latitude (Cluster). On the nightside in the tail, a first wave event comparison - in a rather quiet time interval - is shown. It opens the doors to future studies, such as event timing during substorms, to possibly determine their onset location.

引用

页码：2785 / 2801

页数：17

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