1National Institute of Aerospace Technology, Ctra. de Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain
2Departamento de Física de la Tierra, Astronomía y Astrofísica I, Universidad Complutense de Madrid, Pza. de las Ciencias, s/n, 28040 Madrid, Spain
*now at: CNR-IMM MATIS at Dipartimento di Fisica e Astronomia, Università di Catania, Via S. Sofia 64, 95123 Catania, Italy
Received: 17 Jan 2014 – Discussion started: 04 Aug 2014
Abstract. MOURA instrument is a three-axis magnetometer and gradiometer designed and developed for Mars MetNet Precursor mission.
Revised: 22 Dec 2014 – Accepted: 05 Jan 2015 – Published: 30 Jan 2015
The initial scientific goal of the instrument is to measure the local magnetic field in the surroundings of the lander i.e. to characterize the magnetic environment generated by the remanent magnetization of the crust and the superimposed daily variations of the field produced either by the solar wind incidence or by the thermomagnetic variations. Therefore, the qualification model (QM) will be tested in representative scenarios like magnetic surveys on terrestrial analogues of Mars and monitoring solar events, with the aim to achieve some experience prior to the arrival to Mars.
In this work, we present a practical first approach for calibration of the instrument in the laboratory; a finer correction after the comparison of MOURA data with those of a reference magnetometer located in San Pablo de los Montes (SPT) INTERMAGNET Observatory; and a comparative recording of a geomagnetic storm as a demonstration of the compliance of the instrument capabilities with the scientific objectives.
Díaz-Michelena, M., Sanz, R., Cerdán, M. F., and Fernández, A. B.: Calibration of QM-MOURA three-axis magnetometer and gradiometer, Geosci. Instrum. Method. Data Syst., 4, 1-18, doi:10.5194/gi-4-1-2015, 2015.