Z. X. Liu

State Key Laboratory of Space Weather

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O. Santolı́k

Czech Academy of Sciences, Institute of Atmospheric Physics

K. H. Yearby

University of Sheffield

C. Mazelle

Institut de Recherche en Astrophysique et Planétologie

Junying Yang

Beihang University

Weijie Bian

Nanjing University of Aeronautics and Astronautics

B. de Laporte

Ecologie des Forêts de Guyane

Fanglin Hua

Sun Yat-sen University

H. StC. K. Alleyne

University of Sheffield

Z. G. Zhang

National Space Science Center

Zixuan Wang

Henan University of Technology

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National Space Science Center

Chinese Academy of Sciences

Charles River Laboratories (Netherlands)

Centre National de la Recherche Scientifique

State Key Laboratory of Space Weather

University of Sheffield

Laboratoire d'Informatique et d'Automatique pour les Systèmes

Centre National d'Études Spatiales

Beihang University

Ministry of Industry and Information Technology

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First results of low frequency electromagnetic wave detector of TC-2/Double Star program

Annales Geophysicae (2005)

Jinbin Cao Z. X. Liu Junying Yang C. X. Yian Zixuan Wang

Abstract. LFEW is a low frequency electromagnetic wave detector mounted on TC-2, which can measure the magnetic fluctuation of low frequency electromagnetic waves. The frequency range is 8 Hz to 10 kHz. LFEW comprises a boom-mounted, three-axis search coil magnetometer, a preamplifier and an electronics box that houses a Digital Spectrum Analyzer. LFEW was calibrated at Chambon-la-Forêt in France. The ground calibration results show that the performance of LFEW is similar to that of STAFF on TC-1. The first results of LFEW show that it works normally on board, and that the AC magnetic interference of the satellite platform is very small. In the plasmasphere, LFEW observed the ion cyclotron waves. During the geomagnetic storm on 8 November 2004, LFEW observed a wave burst associated with the oxygen ion cyclotron waves. This observation shows that during geomagnetic storms, the oxygen ions are very active in the inner magnetosphere. Outside the plasmasphere, LFEW observed the chorus on 3 November 2004. LFEW also observed the plasmaspheric hiss and mid-latitude hiss both in the Southern Hemisphere and Northern Hemisphere on 8 November 2004. The hiss in the Southern Hemisphere may be the reflected waves of the hiss in the Northern Hemisphere.

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10.5194/angeo-23-2803-2005

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