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SIGMA SIGNED

Investigating Internal Magnetic Field Sources on the Moon and Mars

Total Cost €

0

EC-Contrib. €

0

Partnership

0

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Project "SIGMA" data sheet

The following table provides information about the project.

Coordinator
INSTITUTO NACIONAL DE TECNICA AEROESPACIAL ESTEBAN TERRADAS 

Organization address
address: CR TORREJON AJALVIR KM 4 2
city: TORREJON DE ARDOZ MADRID
postcode: 28850
website: www.inta.es

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Spain [ES]
 Total cost 160˙932 €
 EC max contribution 160˙932 € (100%)
 Programme 1. H2020-EU.1.3.2. (Nurturing excellence by means of cross-border and cross-sector mobility)
 Code Call H2020-MSCA-IF-2019
 Funding Scheme MSCA-IF-EF-ST
 Starting year 2021
 Duration (year-month-day) from 2021-01-01   to  2022-12-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    INSTITUTO NACIONAL DE TECNICA AEROESPACIAL ESTEBAN TERRADAS ES (TORREJON DE ARDOZ MADRID) coordinator 160˙932.00

Map

 Project objective

The Earth possesses an internal magnetic field produced by convection movements occurring in the outer liquid metallic core of the planet, called dynamo. In order to understand how the Earth dynamo mechanisms work, it is required to understand how a planetary dynamo operates as a whole, from its birth to its demise. For this purpose, our inner Solar System provides a natural laboratory. Today, amongst all our companion telluric planets, only Mercury possesses a core magnetic field. Venus has no observable internal magnetic field, which is enigmatic. Crustal magnetic fields are observed at the surface of Mars and the Moon, which is indicative that these bodies likely had a dynamo in their history, but is no longer active. More importantly, these crustal fields hold fundamental information about the ancient core field, such as its morphology, intensity and temporal variation. By studying the crustal magnetic fields of other planetary bodies, such as Mercury, the Moon or Mars, where different dynamos might have operated, the dynamo processes themselves can be better understood. The SIGMA project targets to unveil crucial unanswered questions of the Earth global magnetic field evolution through an investigation of different planetary crustal anomalies using a novel methodology of surveys (developed by the host) and the generation of advanced models (expertise of the fellow candidate). The results will have an innovative impact in the imminent planetary exploration, where the candidate would be positioned as a senior and independent researcher with a profile comprising theoretical and experimental pioneering techniques.

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The information about "SIGMA" are provided by the European Opendata Portal: CORDIS opendata.

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