Mineral Weathering in a Semiarid Mountain River: Its assessment through PHREEQC inverse modeling

By means of PHREEQC inverse modeling, we have simulated the weathering reactions in Los Reartes River, a mountainous (2400–670 m a.s.l.) drainage basin from the Sierras Pampeanas of Córdoba, Argentina, analyzing the effect of lithology, relief, and climate. The steep upper half of the basin (slopes > 20) is occupied by exposed granite; the remaining area is mostly metamorphic, with cropping out gneisses and progressively decreasing slopes (< 6). Climate is semihumid to semiarid; rainfall mainly occurs in summer and decreases with decreasing height. PHREEQC inverse models developed using water chemical data showed that (a) oligoclase was the major supplier of solutes, while the main precipitated phase was kaolinite in the granite domain; (b) muscovite is the chief supplier of solutes and illite is the main precipitated phase in the gneissic realm; (c) the steeper portions of the metamorphic reach are less crucial in supplying solutes than the lower ones, thus highlighting the importance of the water residence time in the kinetics of dissolution; (d) in the driest time of the year (winter, 20 mm/month) we registered the highest production of dissolved and precipitated phases; fluxes (mmol/month), however, are higher at the end of the rainy season; (e) CO₂ consumption is important all along the Los Reartes drainage basin and, in terms of mmol/kg H₂O, the lowermost portion of the basin is the most significant supplier; (f) CO₂ accounts for over 50 of all the species involved in the weathering reactions occurring at the Los Reartes drainage basin.     

Spatial variation in pore water geochemistry in a mangrove system (Pai Matos island, Cananeia-Brazil)

Spatial variation in salinity, pH, redox potential, and in the concentrations of dissolved Mn, Fe²⁺ and sulphides in pore water were investigated in a mangrove system in the state of São Paulo (Brazil). Total organic C (TOC), S, Fe and Mn were analyzed in the solid phase, along with acid volatile sulphide (AVS), density of roots and percentage of sand. Five zones, situated along the length of a 180 m transect were considered in the study. Four of these were colonized by different species of vascular plants (Spartina, Laguncularia, Avicennia and Rhizophora) and were denominated soils; the other was not colonized by vegetation, and was denominated sediment. The results indicated important differences between the physicochemical conditions of the pore water in the vegetated zones and the sediment. In the former, two geochemical environments were identified, based on soil depths. The upper 20 cm contained the largest quantity of roots, and the conditions were oxic (Eh > 350 mV) or suboxic (Eh: 100–350 mV), acidic, and with high concentrations of Fe and Mn in the pore water. Below this depth, the soil became anoxic, the concentration of sulphides (HS⁻) increased significantly and the concentrations of dissolved Fe and Mn decreased significantly. The total S and the AVS fraction increased with depth, while TOC concentrations decreased, indicating that the decreases in Fe and Mn were due to the precipitation of metal sulphides. However, clear differences among the vegetated zones were not observed. The sediment was always anoxic, but with low concentrations of sulphide in the interstitial water, and was neutral or slightly alkaline. As in the soils, the concentrations of sulphides and total S increased significantly with depth, indicating that the conditions favoured the synthesis and stability of metal sulphides.     

Experimental data on the speciation of sulfur as a function of oxygen fugacity in basaltic melts

The speciation of sulfur as a function of oxygen fugacity was calculated in glasses of basaltic composition saturated experimentally with either sulfide or sulfate phases. The experiments were conducted on mixtures of synthetic and natural materials equilibrated at 1300 °C and 1 GPa in a piston-cylinder apparatus. Sulfur speciation was calculated by measuring the peak shift of the sulfur Kα radiation relative to a sulfide standard, whereas oxygen fugacity was calculated from the composition of olivine and spinel present in the assemblages. The results are consistent with sulfur being present as sulfite (S⁴⁺) in addition to sulfate (S⁶⁺) in oxidized melts. Therefore, sulfur speciation derived from SKα peak shifts should be seen as ”sulfate mole fraction equivalents“ (X(S⁶⁺)_eq.). Using the data available, an empiric function:

X(S6+)_eq.=0.86/(1+exp(2.89−2.23ΔFMQ))     

Measurement of a Peak in the Cosmic Microwave Background Power Spectrum from the North American Test Flight of Boomerang

We describe a measurement of the angular power spectrum of anisotropies in the cosmic microwave background (CMB) at scales of 0&fdg;3 to 5 degrees from the North American test flight of the Boomerang experiment. Boomerang is a balloon-borne telescope with a bolometric receiver designed to map CMB anisotropies on a long-duration balloon flight. During a 6 hr test flight of a prototype system in 1997, we mapped more than 200 deg(2) at high Galactic latitudes in two bands centered at 90 and 150 GHz with a resolution of 26&arcmin; and 16&farcm;5 FWHM, respectively. Analysis of the maps gives a power spectrum with a peak at angular scales of 1 degrees with an amplitude 70 μK(CMB).     

Low‐frequency modulation and trend of the relationship between ENSO and precipitation along the northern to centre Peruvian Pacific coast

The relationship between El Niño Southern Oscillation (ENSO) and precipitation along the Peruvian Pacific coast is investigated over 1964–2011 on the basis of a variety of indices accounting for the different types of El Niño events and atmospheric and oceanographic manifestations of the interannual variability in the tropical Pacific. We show the existence of fluctuations in the ENSO/precipitation relationship at decadal timescales that are associated with the ENSO property changes over the recent decades. Several indices are considered in order to discriminate the influence of the two types of El Niño, namely, the eastern Pacific El Niño and the central Pacific El Niño, as well as the influence of large‐scale atmospheric variability associated to the Madden and Julian Oscillation, and of regional oceanic conditions. Three main periods are identified that correspond to the interleave periods between the main climatic transitions over 1964–2011, i.e. the shifts of the 1970s and the 2000s, over which ENSO experiences significant changes in its characteristics. We show that the relationship between ENSO and precipitation along the western coast of Peru has experienced significant decadal change. Whereas El Niño events before 2000 lead to increased precipitation, in the 2000s, ENSO is associated to drier conditions. This is due to the change in the main ENSO pattern after 2000 that is associated to cooler oceanic conditions off Peru during warm events (i.e. central Pacific El Niño). Our analysis also indicates that the two extreme El Niño events of 1982/1983 and 1997/1998 have overshadowed actual trends in the relationship between interannual variability in the tropical Pacific and precipitation along the coast of Peru. Overall, our study stresses on the complexity of the hydrological cycle on the western side of the Andes with regard to its relationship with the interannual to decadal variability in the tropical Pacific. Copyright © 2014 John Wiley & Sons, Ltd.     

Exploring the time geography of public transport networks with the gtfs2gps package

Journal of Geographical Systems - The creation of the General Transit Feed Specification (GTFS) in the mid-2000s provided a new data format for cities to organize and share digital information on...     

The ocean’s role in setting the mean position of the Inter-Tropical Convergence Zone

Through study of observations and coupled climate simulations, it is argued that the mean position of the Inter-Tropical Convergence Zone (ITCZ) north of the equator is a consequence of a northwards heat transport across the equator by ocean circulation. Observations suggest that the hemispheric net radiative forcing of climate at the top of the atmosphere is almost perfectly symmetric about the equator, and so the total (atmosphere plus ocean) heat transport across the equator is small (order 0.2 PW northwards). Due to the Atlantic ocean’s meridional overturning circulation, however, the ocean carries significantly more heat northwards across the equator (order 0.4 PW) than does the coupled system. There are two primary consequences. First, atmospheric heat transport is southwards across the equator to compensate (0.2 PW southwards), resulting in the ITCZ being displaced north of the equator. Second, the atmosphere, and indeed the ocean, is slightly warmer (by perhaps 2 °C) in the northern hemisphere than in the southern hemisphere. This leads to the northern hemisphere emitting slightly more outgoing longwave radiation than the southern hemisphere by virtue of its relative warmth, supporting the small northward heat transport by the coupled system across the equator. To conclude, the coupled nature of the problem is illustrated through study of atmosphere–ocean–ice simulations in the idealized setting of an aquaplanet, resolving the key processes at work.