Udo Barckhausen und Bernd Schreckenberger hauling in the magnetometer array
Source: BGR
Udo Barckhausen, Ingo Heyde, Bernd Schreckenberger:
What can we find out about polymetallic sulfides on the seafloor using magnetic measurements?
The seafloor consists most predominantly of basaltic rock which has a relatively high content of magnetic minerals and therefore also a pronounced magnetic signature. In places where, for a longer time, hot water has been flowing through the rock (the so-called hydrothermalism), the basalt is chemically altered, and especially the magnetic minerals are changed in a way that they lose their ferromagnetic properties. Magnetic measurements can identify the hydrothermally altered rock parts, because they are usually revealed by a weakened magnetic field. As the formation of polymetallic sulfides at the seafloor takes place in direct connection with hydrothermalism, the magnetic anomalies of the altered basalts are an indirect hint to possible deposits.
Which measurements can by carried out especially well with the 'Pourquoi Pas?'?
The 'Pourquoi Pas?' is outstandingly well equipped for the use of the ROV Victor 6000. It can not only be used for the sampling of rocks, fluids etc. but can alternatively be equipped with a so-called bathymetry module. This consists for the main part of a multibeam echo sounding system for high-resolution seafloor mapping. This module, we enhanced with our Fluxgate gradiometer system for a high-resolution magnetic survey of the seafloor. Thus, we obtained data from a surface of 1.5 km x 3.3 km in the extended area of the Kairei hydrothermal field in a constant distance of 50 m above ground. In combination with the bathymetry, this is a unique data set furnishing a high-precision map of the magnetic field in this ridge area. The interpretation of the measured magnetic minima and maxima regarding volcanic structures, but especially active and inactive sulfide occurrences will be extremely exciting. First of all, however, the magnetic field data will have to be processed, in order, for example, to eliminate the magnetic disturbance of the ROV itself.
At a water depth of 2,500 to 3,000 meters, this resolution cannot be achieved with sensors towed close to the ocean surface. It must be noted as well that the magnetic field of a mass anomaly decays, with increasing distance, very quickly at 1/d³. This shows the possibilities of measurements, that are carried out close the magnetic sources.
What kind of magnetometer is used on the cruise INDEX 2016?
Altogether, we use four magnetometer systems, sometimes at the same time. Traditional standard for geophysical measurements is the gradient magnetometer that is towed about 600 m behind the ship. It consists of two high-precision scalar magnetometers that are 150 m apart and measure only the strength of the magnetic field. The difference between the readings allows to eliminate the frequent disturbances of the magnetic field that have their origin in streams caused by the sun in the earth’s higher atmosphere.
Also integrated into the towed system is a magnetometer, that additionally measures the vector components of the field, that means, how strong the field is in driving direction, horizontally to it respectively in the northern and eastern direction and in the Z-direction, i. e. upwards and downwards. Thus, we gain additional information on magnetic bodies under the seafloor, as, for example, their orientation.
Of course there is a reason for the fact that these systems are towed with considerable effort at a distance of some ship’s lengths behind the vessel: it is important to get away from the big iron mass of the ship that disturbs the magnetic measurements significantly.
Quite in contrast to this principle, two identically constructed vector magnetometers are mounted on the compass deck of the ship which perform non-stop recordings throughout the whole cruise. The interpretation is more difficult and not that exact but not impossible and offers also advantages towards the towed system.
Last but not least we still have two vector magnetometers incorporated into a titanium casing which is pressure-resistant down to 6,000 meters water depth. On the cruise INDEX 2016, this system is attached to the ROV Victor and measures the magnetic field about 50 m above ground. So far, this technology has not often been applied, but it offers great possibilities and is the only way to survey small-scale magnetic bodies like, for example, sulfide fields, in greater water depths.
Gravimetry
What can we find out on polymetallic sulfides on the seafloor using gravimetric measurements?
Ship-based gravity data allow, especially by means of density modeling, statements on variations in the structural build-up of the oceanic crust. Thus, areas can be identified where the oceanic crust is especially thick or also especially thin. This allows conclusions on the possible formation of polymetallic sulfides in the respective area. In water-depths of more than 4,000 m, however, the spatial resolution is very limited and statements on single fields is not possible. For that purpose, gravimetric measurements would have to be carried out directly at the seafloor or closely above ground, for example with an AUV (Autonomous Underwater Vehicle).
Which gravimeters were used on the cruise INDEX 2016?
We have installed BGR’s sea gravimeter system KSS32M, built by the firm BGGS in Meersburg, close to the ship’s center on a pedestal especially designed for this purpose. It is a scalar gravimeter, which means, we only measure the vertical component of the gravity acceleration. For that purpose, the gravity sensor is installed on a gyro stabilized platform, which ensures the dynamic levelling. The ship’s own, older KSS31 system is set up very close-by, it includes not only a gyro table and a gravity sensor but also a well-equipped electronic rack for supply and steering of the system. The parallel measurements enlarge the database and allow the comparison of both systems regarding data quality.