Magnetic field turbulence studies aboard the China Seismo-Electromagnetic Satellite and related ground based phenomena

Konrad Schwingenschuh; Werner Magnes; Xuhui Shen; Jindong Wang; Bingjun Cheng; Bin Zhou; Andreas Pollinger; Christian Hagen; Roland Lammegger; Michaela Ellmeier; Christoph Schirninger; Hans U. Eichelberger; Mohammed Y. Boudjada; Bruno P. Besser; Magda Delva; Irmgard Jernej; Özer Aydogar

doi:https://doi.org/10.5194/egusphere-egu21-14321

[Back] [Session NH4.2]

EGU21-14321

https://doi.org/10.5194/egusphere-egu21-14321

EGU General Assembly 2021

© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Magnetic field turbulence studies aboard the China Seismo-Electromagnetic Satellite and related ground based phenomena

Konrad Schwingenschuh¹, Werner Magnes¹, Xuhui Shen², Jindong Wang³, Bingjun Cheng³, Bin Zhou³, Andreas Pollinger¹, Christian Hagen¹, Roland Lammegger⁴, Michaela Ellmeier⁴, Christoph Schirninger¹, Hans U. Eichelberger¹, Mohammed Y. Boudjada¹, Bruno P. Besser¹, Magda Delva¹, Irmgard Jernej¹, and Özer Aydogar¹

Konrad Schwingenschuh et al.

¹Space Research Institute, Austrian Academy of Sciences, Graz, Austria (konrad.schwingenschuh@oeaw.ac.at)
²National Institute of Natural Hazards, MEMC, Beijing, China
³National Space Science Center, CAS, Beijing, China
⁴Institute of Experimental Physics, Graz University of Technology, Graz, Austria

With a new type of a scalar magnetometer, the Coupled Dark State Magnetometer (CDSM) aboard the China Seismo-Electromagnetic Satellite (CSES) mission, we observed magnetic field fluctuations in the period mid July 2018 until mid November 2018.
The measurement range of the CDSM is from 1000 nT up to 100000 nT and the accuracy 0.19 nT (1), the operational performance is discussed in (2). We are using 1 Hz data in the latitude range -65 degree to +65 degree, CSES has an altitude of approx. 507 km in Sun synchronous polar configuration with 97.4 degree inclination.
We analyzed the total magnetic field turbulence by converting the time series into thermodynamic parameters, e.g. entropy, finally these results have been compared with ground based seismic and volcanic events.

Ref:
(1) Pollinger, A., et al.: Coupled dark state magnetometer for the China Seismo-Electromagnetic Satellite, Measurement Science and Technology, 29, 9, 2018. https://doi.org/10.1088/1361-6501/aacde4
(2) Pollinger, A., et al.: In-orbit results of the Coupled Dark State Magnetometer aboard the China Seismo-Electromagnetic Satellite, Geosci. Instrum. Method. Data Syst., 9, 275–291, 2020. https://doi.org/10.5194/gi-9-275-2020

How to cite: Schwingenschuh, K., Magnes, W., Shen, X., Wang, J., Cheng, B., Zhou, B., Pollinger, A., Hagen, C., Lammegger, R., Ellmeier, M., Schirninger, C., Eichelberger, H. U., Boudjada, M. Y., Besser, B. P., Delva, M., Jernej, I., and Aydogar, Ö.: Magnetic field turbulence studies aboard the China Seismo-Electromagnetic Satellite and related ground based phenomena, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-14321, https://doi.org/10.5194/egusphere-egu21-14321, 2021.

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