The electromagnetic wave experiment for CSES mission: Search coil magnetometer

Cao, Jinbin; Zeng, Li; Zhao, Feng; Wang, ZuoGui; Wang, Yan; Yu, Chen; Meng, Qingsong; Ji, ZhanQiang; Wang, Pengfei; Liu, Zhongwei; Ma, Lily

doi:10.1007/s11431-018-9241-7

Cited by 54 publications

(34 citation statements)

References 46 publications

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“…The SCM on the CSES was manufactured by Beihang University, China; it is designed to measure the magnetic field fluctuation or electromagnetic waves in the low frequency range of 10 Hz–20 kHz (Cao JB et al, ). The SCM is comprised of a three‐axis search coil sensor mounted on a 4.5 m boom.…”

Section: Initial Results From Scientific Payloadsmentioning

confidence: 99%

Introduction to special section on the China Seismo-Electromagnetic Satellite and initial results

Shen

Zong

Zhang

2018

Earth and Planetary Physics

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Section: Initial Results From Scientific Payloadsmentioning

confidence: 99%

Introduction to special section on the China Seismo-Electromagnetic Satellite and initial results

Shen

Zong

Zhang

2018

Earth and Planetary Physics

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“…Then the digital processing unit processes the digitized signals and outputs the waveform and spectral data. The performance of the SCM, including its sensitivity, transfer functions, and calibration results, were checked in the paper of Cao JB et al ().…”

Section: Scm Data Descriptionmentioning

confidence: 99%

“…It aims to measure the magnetic field fluctuation of low‐frequency EM waves in the frequency range of 10 Hz to 20 kHz. Ground calibration results have indicated that SCM is advanced compared the current SCMs in other international space missions, particularly in terms of the –3 dB measurement bandwidth, frequency resolution, and sensitivity (Cao JB et al, ). In this paper, the definitions of each level of the SCM data product are presented in Section 2.…”

Section: Introductionmentioning

confidence: 99%

China Seismo-Electromagnetic Satellite search coil magnetometer data and initial results

Wang¹,

Huang²,

Zhang³

et al. 2018

Earth and Planetary Physics

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Four levels of the data from the search coil magnetometer (SCM) onboard the China Seismo‐Electromagnetic Satellite (CSES) are defined and described. The data in different levels all contain three components of the waveform and/or spectrum of the induced magnetic field around the orbit in the frequency range of 10 Hz to 20 kHz; these are divided into an ultra‐low‐frequency band (ULF, 10–200 Hz), an extremely low frequency band (ELF, 200–2200 Hz), and a very low frequency band (VLF, 1.8–20 kHz). Examples of data products for Level‐2, Level‐3, and Level‐4 are presented. The initial results obtained in the commission test phase demonstrated that the SCM was in a normal operational status and that the data are of high enough quality to reliably capture most space weather events related to low‐frequency geomagnetic disturbances.

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“…It is the first satellite in China to measure geophysical fields. It carries eight instruments, including a search‐coil magnetometer (SCM) (Cao JB et al, ), electric field detector (EFD), high precision magnetometer (HPM) (Cheng BJ et al, ), GNSS occultation receiver (GOR), plasma analyzer package (PAP), Langmuir probe (LAP), high energetic particle package (HEPP) and detector (HEPD) (Ambrosi et al, ), and tri‐band beacon (TBB). The satellite has a sun‐synchronous orbit at an altitude of 507 km and a descending node time of 14:00 LT.…”

Section: Introductionmentioning

confidence: 99%

Preliminary results of the High Energetic Particle Package on-board the China Seismo-Electromagnetic Satellite

Chu

Huang

Shen

et al. 2018

Earth and Planetary Physics

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The high energetic particle package (HEPP) on‐board the China Seismo‐Electromagnetic Satellite (CSES) was launched on February 2, 2018. This package includes three independent detectors: HEPP‐H, HEPP‐L, and HEPP‐X. HEPP‐H and HEPP‐L can detect energetic electrons from 100 keV to approximately 50 MeV and protons from 2 MeV to approximately 200 MeV. HEPP‐X can measure solar X‐rays in the energy range from 1 keV to approximately 20 keV. The objective of the HEPP payload was to provide a survey of energetic particles with high energy, pitch angle, and time resolutions in order to gain new insight into the space radiation environments of the near‐Earth system. Particularly, the HEPP can provide new measurements of the magnetic storm related precipitation of electrons in the slot region, and the dynamics of radiation belts. In this paper, the HEPP scientific data sets are described and initial results are provided. The scientific data can show variations in the flux of energetic particles during magnetic storms.

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The electromagnetic wave experiment for CSES mission: Search coil magnetometer

Cited by 54 publications

References 46 publications

Introduction to special section on the China Seismo-Electromagnetic Satellite and initial results

Introduction to special section on the China Seismo-Electromagnetic Satellite and initial results

China Seismo-Electromagnetic Satellite search coil magnetometer data and initial results

Preliminary results of the High Energetic Particle Package on-board the China Seismo-Electromagnetic Satellite

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