Preprints
https://doi.org/10.5194/egusphere-2025-46
https://doi.org/10.5194/egusphere-2025-46
28 Feb 2025
 | 28 Feb 2025

A new magnetic observatory in La Réunion Island

Benoit Heumez, Frédérick Pesquiera, Abdelkader Telali, and Vincent Lesur

Abstract. A new magnetic observatory has been set on La Réunion island in the Indian Ocean through a collaboration between the "Institut de physique du globe de Paris" (IPGP) local volcano observatory (OVPF) and its magnetic observatory service. This observatory is isolated and serves for monitoring the evolution of the magnetic field in that region. It is also particularly useful for large scale modelling of the core field and other contributions to the geomagnetic field. Three-component vector magnetic field data are continuously collected at 1 Hz using a fluxgate, while scalar data are collected at 0.2 Hz with a proton magnetometer. The data are transmitted every 5 minutes to IPGP main site and made immediately available to the scientific community (see www.bcmt.fr). Due to the strong magnetic field generated by the surrounding volcanic rocks, the differences between the magnetic field strengths as recorded by the proton magnetometer and the strengths calculated from the recorded vector field values vary during a day. To circumvent this difficulty, constant offset values of -2400 nT, 280 nT and -20 nT are systematically added to the X, Y and Z magnetic field components prior to the data distribution. We show that this efficiently reduces the differences between measured and calculated magnetic field strengths inside a day. Definitive observatory data have been calculated over the year 2023 and, although the baseline values present strong variations throughout that year, the derived data meet the quality required for an INTERMAGNET observatory. A Fourier analysis of the data shows that these are not contaminated by a significant noise even if peaks at 0.2 Hz indicate a small cross-talk between vector and scalar instruments.

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Journal article(s) based on this preprint

22 Sep 2025
A new magnetic observatory in La Réunion Island – meeting data quality requirements in a volcanic island setting
Benoit Heumez, Frédérick Pesquiera, Abdelkader Telali, and Vincent Lesur
Geosci. Instrum. Method. Data Syst., 14, 225–235, https://doi.org/10.5194/gi-14-225-2025,https://doi.org/10.5194/gi-14-225-2025, 2025
Short summary
Benoit Heumez, Frédérick Pesquiera, Abdelkader Telali, and Vincent Lesur

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse

Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Vincent Lesur on behalf of the Authors (02 May 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Publish subject to minor revisions (review by editor) (30 May 2025) by Seiki Asari
AR by Vincent Lesur on behalf of the Authors (09 Jun 2025)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (11 Jun 2025) by Seiki Asari
AR by Vincent Lesur on behalf of the Authors (18 Jun 2025)  Manuscript 

Journal article(s) based on this preprint

22 Sep 2025
A new magnetic observatory in La Réunion Island – meeting data quality requirements in a volcanic island setting
Benoit Heumez, Frédérick Pesquiera, Abdelkader Telali, and Vincent Lesur
Geosci. Instrum. Method. Data Syst., 14, 225–235, https://doi.org/10.5194/gi-14-225-2025,https://doi.org/10.5194/gi-14-225-2025, 2025
Short summary
Benoit Heumez, Frédérick Pesquiera, Abdelkader Telali, and Vincent Lesur
Benoit Heumez, Frédérick Pesquiera, Abdelkader Telali, and Vincent Lesur

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Short summary
A new magnetic observatory has been set on La Réunion island in the Indian Ocean. This observatory is isolated and serves for monitoring the evolution of the magnetic field in that region. It is also particularly useful for large scale modelling of the core field and other contributions to the geomagnetic field. The magnetic field strength and direction are measured every second, transmitted every 5 minutes to IPGP main site and made immediately available to users (see www.bcmt.fr).
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