Onset of magmatic accretion within a magma-poor rifted margin: a case study from the Platta ocean-continent transition, eastern Switzerland

Exhumation of subcontinental mantle rocks and its exposure at the seafloor is known from different magma-poor passive continental margins. However, the transition from largely amagmatic passive rifting to seafloor spreading is still poorly documented. In this contribution we use MOR-type gabbroic and basaltic rocks to characterize the magmatism associated with the formation of an ancient ocean-continent transition preserved in the Platta nappe, eastern Switzerland. Gabbros form individual small intrusions into exhumed serpentinized subcontinental mantle rocks. Mineral and bulk-rock chemistry and simple modeling indicate that each gabbro body records different magmatic processes ranging from predominantly fractional crystallization to solidification without fractionation. Mg numbers and Ni contents of equilibrium olivine calculated from basalts and gabbros indicate that few mafic rocks are primary melts but most represent fractionated compositions ranging from T- to N-MORB. Whereas most mafic rocks may be explained by low to moderate degrees of melting of an N-MORB-type mantle, the source of some basalt is enriched in incompatible elements. This compositional variation seems to correlate with the spatial distribution of the mafic rocks within the ocean-continent transition whereby mafic rocks with T-MORB signatures occur close to the continental margin whereas N-MORB signatures are predominantly found oceanwards. As in an opening system time and space are closely linked, the chemical evolution of the mafic rocks along the ocean-continent transitions suggests continuous thinning of the subcontinental mantle and associated uplift of the underlying asthenosphere during the time between the crustal and the lithospheric breakup.     

The Starzach site in Southern Germany: a site with naturally occurring CO<Subscript>2</Subscript> emissions recovering from century-long gas mining as a natural analog for a leaking CCS reservoir

In this paper, we present the Starzach site, a region featuring numerous natural CO₂ emission spots, such as mofettes, that reappeared after a longer period of extensive industrial CO₂ mining. We discuss the results of a detailed literature study on the geological setting and the activities related to the gas mining in combination with own measurements to introduce the site as an example on how gas leakage from an insecure CCS reservoir could manifest at the surface. The site is in particular interesting for such investigations as the CO₂ emissions started to replenish after the end of the CO₂ mining and offers the unique possibility to investigate an increase in degassing activity as it might be expected for an active CCS site where leakage is suspected. Based on the geological setting and soil, gas emission, and isotope investigations, we further discuss the source of the CO₂ emission and the gas ascent to the ground surface via deep-reaching faults, latter being so far excluded by previous work. The combination of our extensive literature review and recent field investigations allowed us to draw new geological conclusions for the site that were under discussion for a long time and to give insight into the site’s potential for CCS-related analog studies in the future.     

Neuordnung der Schriftleitung

Ohne Zusammenfassung     

On the height scale of magnetic fields above sunspots derived from RATAN-600 observations

Model calculations of the S-component are compared with observations of the RATAN-600 telescope at five discrete microwave frequencies referring to active region McMath No. 15974 on May 1, 1979. The spectral variations of source diameter, flux density, and degree of polarization are used to derive the height scale of the magnetic field in accordance with a magnetic dipole distribution under the assumption of advanced temperature and electron density distributions according to most recent EUV observations.