Abstract

Abstract. The China Seismo-Electromagnetic Satellite (CSES) was launched in February 2018 into a polar, sun-synchronous, low Earth orbit. It provides the first demonstration of the Coupled Dark State Magnetometer (CDSM) measurement principle in space. The CDSM is an optical scalar magnetometer based on the coherent population trapping (CPT) effect and measures the scalar field with the lowest absolute error aboard CSES. Therefore, it serves as the reference instrument for the measurements done by the fluxgate sensors within the High Precision Magnetometer instrument package. In this paper several correction steps are discussed in order to improve the accuracy of the CDSM data. This includes the extraction of valid 1 Hz data, the application of the sensor heading characteristic, the handling of discontinuities, which occur when switching between the CPT resonance superpositions, and the removal of fluxgate and satellite interferences. The in-orbit performance is compared to the Absolute Scalar Magnetometer aboard the Swarm satellite Bravo via the CHAOS magnetic field model. Additionally, an uncertainty of the magnetic field measurement is derived from unexpected parametric changes of the CDSM in orbit in combination with performance measurements on the ground.

Highlights

  • The China Seismo-Electromagnetic Satellite (CSES), known as Zhangheng-1, investigates natural electromagnetic phenomena and possible applications for earthquake monitoring from space (Shen et al, 2018)

  • The China Seismo-Electromagnetic Satellite (CSES) mission provides the first demonstration of the Coupled Dark State Magnetometer (CDSM) measurement principle in space

  • This includes the extraction of valid 1 Hz data, the application of the sensor heading characteristic, the handling of discontinuities, which occur when switching between the coherent population trapping (CPT) resonance superpositions, and the removal of fluxgate and satellite interferences

Read more

Summary

Introduction

The China Seismo-Electromagnetic Satellite (CSES), known as Zhangheng-1, investigates natural electromagnetic phenomena and possible applications for earthquake monitoring from space (Shen et al, 2018). The CPT resonance n = 0 is excited by the two light fields denoted by the black dashed arrowed lines in Fig. 1 and occurs under certain conditions when the frequency difference of both first-order sidebands of this FM spectrum fits the energy difference of the 52S1/2 ground states F = 1, mF = 0 and F = 2, mF = 0. This resonance is used to adjust the microwave oscillator frequency to changes in νHFS and to compensate for a temperature-dependent drift of the electronics. 44270 is the identifier for the daytime ascending segment of orbit 4427

Correction of in-orbit data
Extraction of valid 1 Hz data
Application of sensor heading characteristic
Removal of fluxgate interferences
Removal of satellite interferences
In-orbit performance
Comparison to CHAOS model and Swarm data
Discussion of data integrity
Discontinuity jumps when switching CPT resonance superpositions
Microwave oscillator detuning sensitivity of the magnetic field measurement
Optical power
Sensor temperature
PCB temperature and noise of the microwave oscillator control loop
Findings
Angular-dependent microwave oscillator adjustment during ground tests
Conclusions
Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.