Mineralisation at the Carrock Fell Tungsten Mine,N. England: Paragenetic,fluid inclusion and geochemical study

Tungsten ore at Carrock Fell Mine comprises wolframite and scheelite in polyminerallic quartz veins which traverse the Grainsgill Granite cupola and surrounding country rocks. In the veins, a wolframite-scheelite-apatite assemblage pre-dates a scheelite-arsenopyrite-pyrite (plus other sulphides) assemblages. Temperatures of mineralisation declined from a peak near 350°C to 170°C, and the hydrothermal fluid contained about 6 weight% NaCl and 3 wt% NaHCO₃. Contemporaneous greisenisation involved loss of Na, Cr, Ca and Ba from granite, but Si and K were retained while B, Be and Al increased slightly. Sn also increased but is always a trace constituent, and F appears to have decreased. Zones of intense alteration contain high concentrations of quartzhosted fluid inclusions resulting from penetration of the granite by fluid chemically similar to that in the vein quartz. The W-rich, Sn-poor nature of the mineralisation may relate to the weakly saline, F-deficient but CO₂-rich fluid chemistry. The alteration and mineralisation processes took place during late cooling of the Lower-Devonian Skiddaw Granite. Cross-cutting quartz-ankerite veins and argillitic zones which may be considerably younger than those producing the tungsten ore, have a distinct mineral suite lacking W and As and including major Pb and Zn. Temperatures at this late stage were below 150°C, and the fluid is estimated to have contained approximately 12 wt% NaCl and 15 wt% CaCl₂.     

Seismicity and seismic intensities in Jamaica,West Indies: A problem in risk assessment

A review of the history of earthquake observations in Jamaica is presented; there have been several high-intensity earthquakes in the last 300 years. The observed seismicity of the Jamaica region is discussed in the context of what is known of regional tectonics, and possible source regions of earthquakes are identified but a comparison between instrumentally determined seismicity and macroseismicity shows that the instrumental data are of insufficient quantity or quality to permit direct assessment of earthquake risk by conventional techniques. An alternative approach has been adopted; consideration of the macroseismic record suggests that the peak acceleration in rock with 90 per cent probability of not being exceeded in any 50-year period is of order 0.3 g but that there are very significant local variations caused by near-surface geology. Especially this applies to the capital, Kingston, and envelope response spectra are derived for shallow, intermediate and deep thickness of sediments under the city to demonstate the possibility that localized amplification may occur. A current apparent decline in the seismicity of the Jamaica region is noted but it is shown that the decline in the number of earthquakes of engineering interest is not yet statistically significant.     

Amphibole-bearing basalts from the submarine volcano Kick’em-Jenny in the lesser antilles Island arc

An oceanographic survey by H.M.S. Hecla of the 1974 active submarine volcano (12°18′N and 61°38′W) revealed a crater at 190 m below sea level and bottom-sampling yielded fresh olivine basalt pyroclastics with phenocrysts of olivine, plagioclase and clinopyroxene. Megacrysts of amphilbole, up to 16 modal percent, are subsilicic and nepheline-normative ferroan pargasites. The mineral assemblage Ol+Cpx+Pl+Amph appears to have been in equilibrium in the Kick’em-Jenny melt prior to eruption, although published experimental studies on hydrous (H₂O-saturated) or anhydrous alkali basaltic compositions have not yielded this mineral assemblage at any pressure. Interpolation between the experimentally determined phase relationships for dry and water-saturated alkali basaltic liquids indicates, however, that in an isobaric section at 5 kb the observed assemblage can exist in the water-undersaturated region. The Kick’em-Jenny olivine basalts belong to a suite of variably undersaturated basaltic rocks including alkali picrites and basanites, common in Grenada and the southern Grenadines, but although the available evidence indicates the importance of the presence of water in the genesis of these melts, their origin seems most likely to be associated with partial melting of upper mantle material rather than melting of amphibolite in an underthrust lithospheric slab.     

Preliminary investigations of the tsunami hazard of Kick'em Jenny submarine volcano

Kick'em Jenny is a submarine volcano situated 9 kilometres north of Grenada in the Lesser Antilles. A preliminary study suggests that the volcano is a prime candidate for tsunamigenic eruptions on a potentially hazardous scale, possibly affecting the whole of the Eastern Caribbean region. The uniqueness of individual volcanic eruptions means that attempts to generalise tsunamigenic mechanisms are extremely tentative. However, the theory of underwater explosion generated water waves is applicable to submarine volcanoes to model explosive eruptions. Using this theory, initial maximum ocean surface displacements are calculated for Kick'em Jenny hydroeruptions, corresponding to various event magnitudes (up to a worst-case scenario eruption on the scale of Krakatau, 1883). Wave propagation theories are then applied to the resulting tsunami wave dispersion, before beach shoaling equations are used to estimate the maximum tsunami run-up at adjacent coastal areas. Maps of the region have been prepared showing the paths of the wave-fronts (ray-tracing), travel times and maximum wave run-up amplitudes along coastlines. Finally, an attempt is made to assess how great a hazard the volcano represents, by considering the probability of each magnitude event occurring.     

Characterizing anthropic sediments in north European Neolithic settlements: An assessment from Skara Brae,Orkney

The creation of anthropic sediments, traditionally referred to under the blanket term midden, through the utilization of settlement waste materials in domestic settlement construction was first recognized during early excavations at the Orcadian Neolithic site of Skara Brae (V.G. Childe, 1931a; 1931b). Prior to the present study there has been no systematic attempt to identify the nature of these sediments at Skara Brae, whose likely occupation dates between ˜3100 and 2500 B.C., or to assess whether different materials were incorporated into construction or varied with different phases of site formation. The opportunity to begin addressing these issues arose with the location of undisturbed sediment samples held in storage since the last site excavations of 1972–1973 (D.V. Clarke, 1976). Ten thin sections were manufactured from these samples, representing earlier and later phases of Neolithic settlement at Skara Brae. Observations using thin‐section micromorphology, supported by total phosphorus and particle‐size distribution analyses, suggest that both earlier and later settlement phases show accumulation of household waste dominated by fuel residues. These wastes may have been used to help stabilize wind‐blown sand deposits during the later settlement phases. In addition, the use of clay material tempered with household waste is associated with wall construction. Animal manures are only evident in anthropic deposits on the edge of the main settlement site where composting may have been taking place, and there is no evidence for their use in site construction. The authors conclude by drawing attention to possible diverse uses of anthropic sediments in settlement construction at other Neolithic settlements in Orkney. © 2006 Wiley Periodicals, Inc.     

An observation of polar aurora and airglow from the ISIS-II spacecraft

This is a preliminary but comprehensive report on coordinated data obtained with the ISIS-II spacecraft, fourth in the ISIS series, launched 1 April 1971, into a near circular 1400 km orbit. The capabilites of the ISIS-I spacecraft have been extended in a number of ways, including the global mapping of the 3914 Å, 5577 Å and 6300 Å emissions. Data obtained during a 30-min pass over the south pole depict the nightside oval and polar cap, as well as mid-latitude airglow effects; these data are described and discussed.     

Observation of vertical E-region neutral winds in two intense auroral arcs

Vertical winds have been observed by optical Doppler measurements of the 557.7 nm emission in the aurora, using a Fabry-Perot spectrometer. Both upward and downward winds were observed, of 15 m s^?1 magnitude. The upward winds were associated with westward overhead currents, and with low altitude aurora (～ 110 km) as determined by the auroral temperature, while a high altitude aurora (～ 135 km) and eastward currents were associated with the downward wind. The Lorentz force of these currents has the wrong direction to act as a direct forcing mechanism. It is concluded that Joule heating is directly responsible for the upward winds, while the divergence of horizontal winds is responsible for the downward winds.