Erratum to J. M. Adelson, G. R. Helz, and C. V. Miller (2001) Reconstructing the rise of recent coastal anoxia; molybdenum in Chesapeake Bay sediments. Geochimica et Cosmochimica Acta65, 237-252.     

J.M AdelsonG.R Helz  C.V Miller 《Geochimica et cosmochimica acta》2002,66(24):4367

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An overview and general results of the Lopez island OBS experiment     

G. H. Sutton  F. K. Duennebier  B. Iwatake  J. D. Tuthill  B. T. R. Lewis  J. Ewing 《Marine Geophysical Researches》1981,5(1):3-34

The purpose of the experiment was to determine the effects of coupling and bottom currents on ocean bottom seismometers. Twelve operational OBSs, three specially designed three-component systems, and a hydrophone were compared with each other. Unlike seismometers placed on hard rock at land stations, ocean bottom seismometers can be affected by soft sediments (which act as lossy mechanical springs) and by buoyancy. Coupling through soft sediments can modify the response to ground motion much as a low pass filter does, and high buoyancy tends to counteract this effect. These effects are observed in the Lopez data, which consist of signals from mechanical transient tests, cap shots, airgun pulses, and general background noise. The modification of response is pronounced for some instruments and barely noticeable in others. Instruments that stand high in the water relative to their base width tend to be susceptible to rocking motion that shows up as a mechanical cross coupling between horizontal and vertical motion. Correlation of Lopez results with coupling theory suggests that it is possible to design ocean bottom seismometers that will couple well to any sediment. Current levels at the Lopez site (<5 cm s^-1) were too small to produce noticeable effect on any of the instruments; however, the same design criteria that will minimize coupling problems will also lessen problems caused by ocean currents.Hawaii Institute of Geophysics Contribution No. 1171.  相似文献   

Episode 49 of the Pu'u 'O'o-Kupaianaha eruption of Kilauea volcano-breakdown of a steady-state eruptive era     

M. T. Mangan  C. C. Heliker  T. N. Mattox  J. P. Kauahikaua  R. T. Helz 《Bulletin of Volcanology》1995,57(2):127-135

The Pu'u 'O'o-Kupaianaha eruption (1983-present) is the longest lived rift eruption of either Kilauea or neighboring Mauna Loa in recorded history. The initial fissure opening in January 1983 was followed by three years of episodic fire fountaining at the Pu'u 'O'o vent on Kilauea's east rift zone 19km from the summit (episodes 4–47). These spectacular events gave way in July 1986 to five and a half years of nearcontinuous, low-level effusion from the Kupaianaha vent, 3km to the cast (episode 48). A 49th episode began in November 1991 with the opening of a new fissure between Pu'u 'O'o and Kupaianaha. this three week long outburst heralded an era of more erratic eruptive behavior characterized by the shut down of Kupaianaha in February 1992 and subsequent intermittent eruption from vents on the west flank of Pu'u 'O'o (episodes 50 and 51). The events occurring over this period are due to progressive shrinkage of the rift-zone reservoir beneath the eruption site, and had limited impact on eruption temperatures and lava composition.  相似文献   

Balancing deformation in NW Borneo: Quantifying plate-scale vs. gravitational tectonics in a delta and deepwater fold-thrust belt system     

Rosalind C. King  Guillaume Backé  Christopher K. Morley  Richard R. Hillis  Mark R.P. Tingay 《Marine and Petroleum Geology》2010

Recent GPS measurements demonstrate that NW Borneo undergoes 4–6 mm of plate-scale shortening a year, which is not accommodated by plate-scale structures. The only geological structure in NW Borneo described to accommodate on-going shortening is the Baram Delta System located on the outer shelf to basin floor. Delta toe fold-thrust belts are commonly thought to be caused by margin-normal compressional stresses generated by margin-parallel upslope gravitational extension.  相似文献   

Social capital,individual responses to heat waves and climate change adaptation: An empirical study of two UK cities     

Johanna Wolf  W. Neil Adger  Irene Lorenzoni  Vanessa Abrahamson  Rosalind Raine 《Global Environmental Change》2010,20(1):44-52

It has been claimed that high social capital contributes to both positive public health outcomes and to climate change adaptation. Strong social networks have been said to support individuals and collective initiatives of adaptation and enhance resilience. As a result, there is an expectation that social capital could reduce vulnerability to risks from the impacts of climate change in the health sector. This paper examines evidence on the role social networks play in individuals’ responses to heat wave risk in a case study in the UK. Based on interviews with independently living elderly people and their primary social contacts in London and Norwich, we suggest that strong bonding networks could potentially exacerbate rather than reduce the vulnerability of elderly people to the effects of heat waves. Most respondents interviewed did not feel that heat waves posed a significant risk to them personally, and most said that they would be able to cope with hot weather. Bonding networks could perpetuate rather than challenge these narratives and therefore contribute to vulnerability rather than ameliorating it. These results suggest a complex rather than uniformly positive relationship between social capital, health and adaptation to climate change.  相似文献   

Crystallization history of Kilauea Iki lava lake as seen in drill core recovered in 1967–1979     

R. T. Helz 《Bulletin of Volcanology》1980,43(4):675-701

Kilauea Iki lava lake formed during the 1959 summit eruption, one of the most picritic eruptions of Kilauea Volcano in the twentieth century. Since 1959 the 110 to 122 m thick lake has cooled slowly, developing steadily thickening upper and lower crusts, with a lens of more molten lava in between. Recent coring dates, with maximum depths reached in the center of the lake, are: 1967 (26.5 m). 1975 (44.2 m), 1976 (46.0 m) and 1979 (52.7 m). These depths define the base of the upper crust at the time of drilling. The bulk of the core consists of a gray, olivine-phyric basalt matrix, which locally contains coarser-grained diabasic segregation veins. The most important megascopic variation in the matrix rock is its variation in olivine content. The upper 15 m of crust is very olivine-rich. Abundance and average size of olivine decrease irregularly downward to 23 m; between 23 and 40 m the rock contains 5–10% of small olivine phenocrysts. Below 40 m. olivine content and average grainsize rise sharply. Olivine contents remain high (20–45%, by volume) throughout the lower crust, except for a narrow (< 6 m) olivine depleted zone near the basalt contact. Petrographically the olivine phenocrysts in Kilauea Iki can be divided into two types. Type 1 phenocrysts are large (1–12 mm long), with irregular blocky outlines, and often contain kink bands. Type 2 crystals are relatively small (0.5–2 mm in length), euhedral and undeformed. The variations in olivine content of the matrix rock are almost entirely variations in the amount of type 1 olivines. Sharp mineral layering of any sort is rare in Kilauea Iki. However, the depth range 41–52 m is marked by the frequent occurrence of steeply dipping (70°–90°) bands or bodies of slightly vuggy olivine-rich rock locally capped with a small cupola of segregation-vein material. In thin section there is clear evidence for relative movement of melt and crystals within these structures. The segregation veins occur only in the upper crust. The most widely distributed (occurring from 4.5–59.4 m) are thin veins (most < 5 cm thick), which cut the core at moderate angles and appear to have been derived from the immediately adjacent wall-rock by filter pressing. There is also a series of thicker (0.1–1.5 m) segregation veins, which recur every 2–3 m, between 20 and 52 m. These have subhorizontal contacts and appear, from similarities in thickness and spacing, to correlate between drill holes as much as 100 m apart. These large veins are not derived from the adjacent wallrock: their mechanism of formation is still problematical. The total thickness of segregation veins in Kilauea Iki is 3–6 m in the central part of the lake, corresponding to 6–11% of the upper crust. Whole-rock compositions for Kilauea Iki fall into two groups: the matrix rock ranges from 20-7.5% MgO, while the segregation veins all contain between 6.0 and 4.5% MgO. There are no whole-rock compositions of intermediate MgO content. Samples from < 12 m show eruption-controlled chemistry. Below that depth, matrix rock compositions have higher Al₂O₃, TiO₂ and alkalies, and lower CaO and FeO, at a given MgO content than do the eruption pumices. The probable causes of this are assimilation of low-melting components from foundered crust, plus removal of olivine, plus removal of minor augite, for rocks with MgO contents of < 8.0%. Given the observed rate of growth of the upper crust, one can infer that significant removal of the type 1 olivine phenocrysts from the upper part of the lake began in 1963 and ceased sometime prior to 1972. The process. probably gravitative settling, appears to have been inhibited earlier by gas streaming from the lower part of the lens of melt. The olivine cumulate zone, which extends into the upper crust, contains relatively few (25–40%) olivine crystals, few of which actually touch each other. The diffuseness of the cumulate zone raises the possibility that the crystals were coated with a relatively visous boundary layer of melt which moved with them. Calculations of the Stokes’ law settling rates of the largest olivine crystals found at the base of the crust in 1975–76 suggest that the «melt» had a viscosity of > 10⁶ poises, and probably had the properties of a Bingham body, rather than a Newtonian fluid, by that date, which was several years after olivine removal ceased.  相似文献   

Trace element inventory for the northern Chesapeake Bay with emphasis on the influence of man     

G.R Helz 《Geochimica et cosmochimica acta》1976,40(6):573-580

For the northern half of the Chesapeake Bay. Maryland, an evaluation has been made of the relative importance of various human and natural sources of Cr, Mn, Fe, Co, Ni, Cu, Cd, Zn, and Pb. For rive of these (Mn, Fe, Co, Ni, and Zn) river discharge, shore erosion and salt water advection from the oceans account for more than half of the total input. On the other hand, the principal source for Cr and Cu is direct industrial discharge, for Cd is municipal wastewater, and for Pb is atmospheric dust and rain. In the subestuary of Baltimore Harbor, industry is the major contributor of all the elements except Cd and Pb, which again come mostly from wastewater and the atmosphere, respectively. Estimates of the removal of these elements by sedimentation suggest that less than $\text{1}\text{3}$ of the annual input of each metal is removed, except in the case of Cr and Fe where more than $\text{2}\text{3}$ is removed. These results suggest that human enhancement of normal input rates for these elements has the potential to produce a regional rather than merely a local biologic impact. It is of interest that for most of the elements, the percentage of the total input that is retained in the sediments is similar for heavily stressed Baltimore Harbor as it is for the northern Bay system as a whole.  相似文献   

Orbital elements, masses and distance of λ Scorpii A and B determined with the Sydney University Stellar Interferometer and high-resolution spectroscopy     

W. J. Tango  J. Davis  M. J. Ireland  C. Aerts  K. Uytterhoeven  A. P. Jacob  A. Mendez  J. R. North  E. B. Seneta  P. G. Tuthill 《Monthly notices of the Royal Astronomical Society》2006,370(2):884-890

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Dust scattering in the Miras R Car and RR Sco resolved by optical interferometric polarimetry     

M. J. Ireland  P. G. Tuthill  J. Davis  W. Tango 《Monthly notices of the Royal Astronomical Society》2005,361(1):337-344

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Multiwavelength diameters of nearby Miras and semiregular variables     

M. J. Ireland  P. G. Tuthill  T. R. Bedding  J. G. Robertson  A. P. Jacob 《Monthly notices of the Royal Astronomical Society》2004,350(1):365-374

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