First results of low frequency electromagnetic wave detector of TC-2/Double Star program (2024)

Articles | Volume 23, issue 8

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Articles | Volume 23, issue 8

https://doi.org/10.5194/angeo-23-2803-2005

© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.

Special issue:

  • Double Star - First Results

https://doi.org/10.5194/angeo-23-2803-2005

© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.

Articles | Volume 23, issue 8

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First results of low frequency electromagnetic wave detector of TC-2/Double Star program (1)

08 Nov 2005

First results of low frequency electromagnetic wave detector of TC-2/Double Star program (2)|08 Nov 2005

J. B. Cao, Z. X. Liu, J. Y. Yang, C. X. Yian, Z. G. Wang, X. H. Zhang, S. R. Wang, S. W. Chen, W. Bian, W. Dong, Z. G. Zhang, F. L. Hua, L. Zhou, N. Cornilleau-Wehrlin, B. de Laporte, M. Parrot, H. Alleyne, K. Yearby, O. Santolík, and C. Mazelle

J. B. Cao

Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100080, China

Z. X. Liu

Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100080, China

J. Y. Yang

Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100080, China

Graduate School of the Chinese Academy of Sciences, Beijing 100039, China

C. X. Yian

Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, 100080, China

Z. G. Wang

DSP Payload Subsystem, Center for Space Science and Applied Research, Beijing, China

X. H. Zhang

DSP Payload Subsystem, Center for Space Science and Applied Research, Beijing, China

S. R. Wang

DSP Payload Subsystem, Center for Space Science and Applied Research, Beijing, China

S. W. Chen

DSP Payload Subsystem, Center for Space Science and Applied Research, Beijing, China

W. Bian

DSP Payload Subsystem, Center for Space Science and Applied Research, Beijing, China

W. Dong

DSP Payload Subsystem, Center for Space Science and Applied Research, Beijing, China

Z. G. Zhang

DSP Payload Subsystem, Center for Space Science and Applied Research, Beijing, China

F. L. Hua

DSP Payload Subsystem, Center for Space Science and Applied Research, Beijing, China

L. Zhou

DSP Payload Subsystem, Center for Space Science and Applied Research, Beijing, China

N. Cornilleau-Wehrlin

Center d’Environnement Terrestre et Planetaire, Velizy, France

B. de Laporte

Center d’Environnement Terrestre et Planetaire, Velizy, France

M. Parrot

Laboratory de Physique et Chimie de l’Environnement, Orleans, France

H. Alleyne

University of Sheffield, Automatic Control/System Engineering, Sheffield, UK

K. Yearby

University of Sheffield, Automatic Control/System Engineering, Sheffield, UK

O. Santolík

Faculty of Mathmatics and Physics, Charles University, Prague, Czech Republic

Institute of Atmospheric Physics, ASCR, Prague, Czech Republic

C. Mazelle

Centre d’Etude Spatiale des Rayonnements, 31028, Toulouse, France

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 8November 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 3November 2004. LFEW also observed the plasmaspheric hiss and mid-latitude hiss both in the Southern Hemisphere and Northern Hemisphere on 8November 2004. The hiss in the Southern Hemisphere may be the reflected waves of the hiss in the Northern Hemisphere.

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How to cite. Cao, J. B., Liu, Z. X., Yang, J. Y., Yian, C. X., Wang, Z. G., Zhang, X. H., Wang, S. R., Chen, S. W., Bian, W., Dong, W., Zhang, Z. G., Hua, F. L., Zhou, L., Cornilleau-Wehrlin, N., de Laporte, B., Parrot, M., Alleyne, H., Yearby, K., Santolík, O., and Mazelle, C.: First results of low frequency electromagnetic wave detector of TC-2/Double Star program, Ann. Geophys., 23, 2803–2811, https://doi.org/10.5194/angeo-23-2803-2005, 2005.

First results of low frequency electromagnetic wave detector of TC-2/Double Star program (2024)

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