Merlin and Puschino Observations of H2o Masers in Outer Galactic SFR S128N

We have imaged H₂O maser emission from the star-forming region S128 at milli-arcsec resolution using MERLIN, to complement 20 years of monitoring data from the Puschino radio telescope. The drift velocities of the masers and the velocity and location of a new maser region add depth to the model of two colliding CO clouds triggering collapse. Some H₂O masers appear to originate directly from this shock front. The brightest maser appears typical of a YSO jet and remains unsaturated close to peak intensity. The distribution of maser clumps has a fractal dimension 0.4; combined with analysis of drift velocity variations this suggests that the masers trace the dissipation of supersonic turbulence. The spatial distribution of velocities shows that this is in parts more structured than the Kolmogorov cascade.     

Spatial and temporal mapping of water in soil by magnetic resonance imaging

Experiments on model and real soil blocks designed to assess the feasibility of using magnetic resonance imaging for three-dimensional mapping of the time-varying spatial distribution of water in structured soils are reported. The results show that, notwithstanding inherent problems in imaging natural soils with a significant iron content, experimental parameters can be identified which allow satisfactory images to be obtained. Magnetic resonance imaging may therefore provide important information on soil structure and water movement in dual porosity soils, with attendant benefits for the calibration of models of non-Darcian flow in such soils.     

Isotopic remobilization in the Mount Isa tuff beds

The water-laid tuff beds in the mine sequence at Mount Isa, Queensland, yield anomalous whole-rock isochron results. The RbSr “age” is significantly younger than expected, the apparent initial ratio is high, and the scatter about the regression line is significantly greater than experimental. In the UThPb system, the scatter is greater, the “age” is even lower, and the initial ratios approximate to the ore values. The results are interpreted in terms of continued mobility of minor elements in the water-rich sediments while deep-burial conditions persist.