Coasts: the high-risk areas of the world

No other region is more threatened by natural perils than coasts. Fierce winds, storm surges, large waves and tsunamis expend their destructive energy when they reach the coastline. Constituting, in many cases, the boundary between continental plates, coasts experience earthquakes and volcanic eruptions more frequently. The changing climate poses the threat of sea level rise. Most global trade crosses the oceans; ports are the entry and exit points of a nation’s trade. As a consequence, coasts attract people, businesses and industries. Some coastal regions rank among the top places in the world in terms of population and value accumulation. Enormous catastrophe loss potentials have been created and are increasing. Risk is the result of a natural hazard, the values at risk and their vulnerability. Living with and reducing the risk requires awareness at all levels of society and partnership between the public authorities, the people and enterprises concerned, and the financial sector. Great natural events are not avoidable, great disasters are. Catastrophes are not only products of chance but also the outcome of the interaction between political, financial, social, technical and natural circumstances. Effective safeguards are both achievable and indispensable, but they will never provide complete protection. In order to manage the risks faced by a society, we have to be aware of that.     

Carboniferous trilobites: the beginning of the end

It is commonly assumed that by Carboniferous times trilobites were all but extinct, represented by only a handful of species belonging to the genera Phillipsia or Griffithides and found occasionally at a few localities. In fact, there is afar greater abundance and diversity of forms than is usually realized, and in parts of the Carboniferous System trilobites can be as stratigraphically important as many other fossil groups.     

Speleogenesis: the evolution of the Castleton caves

Castleton, in North Derbyshire, is unique in Britain in having four caves open to tourists, as well as several ‘mid’ caves, most of which are only accessible to potholers and speleologists. Together, the tourist and wild caves tell a fascinating story of speleogenesis — the growth and development of a cave system. Both geologists and geomorphologists often ignore cave systems, but such systems play an important part in the evolution of the landscape as we see it today.     

Deltas: the fertile dustbins of the continents

Deltas and their associated deep-water submarine fans are the main repositories of sediment produced by continental erosion. The internal structure of prograding deltas is often complicated by changes in loci of deposition and changes in land-sea levels during their formation. The high water content and rapid deposition cause syn-sedimentary deformation. Deltas have been inhabited by man throughout history due to their rich surface resources. Ancient deltas are rich in hydrocarbons which are widely exploited. They are very sensitive to changes in the hinterland and today their existence is threatened by anthropogenic actions such as dam construction and sea-level changes.     

风险管理是干旱管理的发展趋势

对我国干旱管理现状进行了分析,指出了存在的问题,介绍了抗旱工作要从被动抗旱向主动防旱、科学防旱转变的趋势,并从应急抗旱向常规抗旱和长期抗旱转变的科学管理理念出发,提出我国的干旱管理方式应该从现行的危机管理向风险管理转变,并重点介绍了干旱风险管理的几个主要方面:干旱期的水资源管理、干旱早期预警和干旱预案.     

Climate: Is the past the key to the future?

 The climate of the Holocene is not well suited to be the baseline for the climate of the planet. It is an interglacial, a state typical of only 10% of the past few million years. It is a time of relative sea-level stability after a rapid 130-m rise from the lowstand during the last glacial maximum. Physical geologic processes are operating at unusual rates and much of the geochemical system is not in a steady state. During most of the Phanerozoic there have been no continental ice sheets on the earth, and the planet’s meridional temperature gradient has been much less than it is presently. Major factors influencing climate are insolation, greenhouse gases, paleogeography, and vegetation; the first two are discussed in this paper. Changes in the earth’s orbital parameters affect the amount of radiation received from the sun at different latitudes over the course of the year. During the last climate cycle, the waxing and waning of the northern hemisphere continental ice sheets closely followed the changes in summer insolation at the latitude of the northern hemisphere polar circle. The overall intensity of insolation in the northern hemisphere is governed by the precession of the earth’s axis of rotation, and the precession and ellipticity of the earth’s orbit. At the polar circle a meridional minimum of summer insolation becomes alternately more and less pronounced as the obliquity of the earth’s axis of rotation changes. Feedback processes amplify the insolation signal. Greenhouse gases (H₂O, CO₂, CH₄, CFCs) modulate the insolation-driven climate. The atmospheric content of CO₂ during the last glacial maximum was approximately 30% less than during the present interglacial. A variety of possible causes for this change have been postulated. The present burning of fossil fuels, deforestation, and cement manufacture since the beginning of the industrial revolution have added CO₂ to the atmosphere when its content due to glacial-interglacial variation was already at a maximum. Anthropogenic activity has increased the CO₂ content of the atmosphere to 130% of its previous Holocene level, probably higher than at any time during the past few million years. During the Late Cretaceous the atmospheric CO₂ content was probably about four times that of the present, the level to which it may rise at the end of the next century. The results of a Campanian (80 Ma) climate simulation suggest that the positive feedback between CO₂ and another important greenhouse gas, H₂O, raised the earth’s temperature to a level where latent heat transport became much more significant than it is presently, and operated efficiently at all latitudes. Atmospheric high- and low-pressure systems were as much the result of variations in the vapor content of the air as of temperature differences. In our present state of knowledge, future climate change is unpredictable because by adding CO₂ to the atmosphere we are forcing the climate toward a “greenhouse” mode when it is accustomed to moving between the glacial–interglacial “icehouse” states that reflect the waxing and waning of ice sheets. At the same time we are replacing freely transpiring C3 plants with water-conserving C4 plants, producing a global vegetation complex that has no past analog. The past climates of the earth cannot be used as a direct guide to what may occur in the future. To understand what may happen in the future we must learn about the first principles of physics and chemistry related to the earth’s system. The fundamental mechanisms of the climate system are best explored in simulations of the earth’s ancient extreme climates. Received: 7 November 1996/Accepted: 23 January 1997     

Nannofossils: the smoking gun for the Canarian hotspot

The origin of volcanism in the Canary Islands has been a matter of controversy for several decades. Discussions have hinged on whether the Canaries owe their origin to seafloor fractures associated with the Atlas Mountain range or to an underlying plume or hotspot of superheated mantle material. However, the debate has recently come to a conclusion following the discovery of nannofossils preserved in the products of the 2011–2012 submarine eruption at El Hierro, which tell us about the age and growth history of the western‐most island of the archipelago. Light coloured, pumice‐like ‘floating rocks’ were found on the sea surface during the first days of the eruption and have been shown to contain fragments of pre‐island sedimentary strata. These sedimentary rock fragments were picked up by ascending magma and transported to the surface during the eruption, and remarkably retained specimens of pre‐island Upper Cretaceous to Pliocene calcareous nannofossils (e.g. coccolithophores). These marine microorganisms are well known biostratigraphical markers and now provide crucial evidence that the westernmost and youngest island in the Canaries is underlain by the youngest sediment relative to the other islands in the archipelago. This finding supports an age progression for the onset of volcanism at the individual islands of the archipeligo. Importantly, as fracture‐related volcanism is known to produce non‐systematic age‐distributions within volcanic alignments, the now‐confirmed age progression corroberates to the relative motion of the African plate over an underlying mantle plume or hotspot as the cause for the present‐day Canary volcanism.     

Before the Scottish Survey: Alfred Harker the Geologist

The archival papers of the eminent petrologist Alfred Harker span his entire geological career of over 60 years. These are held by the Archive of the Sedgwick Museum of Earth Sciences (University of Cambridge). Harker was associated with the Department of Geology, the Woodwardian Museum and post-1904, the Sedgwick Memorial Museum. Importantly, his meticulously labelled notebooks provide an unprecedented insight into his development as a field and laboratory scientist. They chart Harker's beginnings as a fossil collector and observer of sedimentary stratigraphy on the North Yorkshire coast, his trips to Wales and Devon with the Sedgwick Club, and his later work in the English Lake District with his friend and colleague John. E. Marr. This paper examines in particular Harker's suite of 20 notebooks kept up until 1894, including his trip to Edinburgh in August 1892. This visit introduced the young scientist to the geology of Scotland for the first time. An overview of Harker's experience and contemporary contacts suggests some reasons why Sir Archibald Geikie later invited him to join the Scottish Survey staff in 1895.     

Mine-water chemistry: the good, the bad and the ugly

 Contaminative mine drainage waters have become one of the major hydrogeological and geochemical problems arising from mankind's intrusion into the geosphere. Mine drainage waters in Scandinavia and the United Kingdom are of three main types: (1) saline formation waters; (2) acidic, heavy-metal-containing, sulphate waters derived from pyrite oxidation, and (3) alkaline, hydrogen-sulphide-containing, heavy-metal-poor waters resulting from buffering reactions and/or sulphate reduction. Mine waters are not merely to be perceived as problems, they can be regarded as industrial or drinking water sources and have been used for sewage treatment, tanning and industrial metals extraction. Mine-water problems may be addressed by isolating the contaminant source, by suppressing the reactions releasing contaminants, or by active or passive water treatment. Innovative treatment techniques such as galvanic suppression, application of bactericides, neutralising or reducing agents (pulverised fly ash-based grouts, cattle manure, whey, brewers' yeast) require further research. Received: 13 August 1996 · Accepted: 3 January 1997     

Development and the Household: Missing the point?

Over the past two decades development has been shifting its focus toward smaller scales and particular problems. As a result, the household has become an increasingly important institution for development, and has come under increased scrunity as development practitioners and scholars seek to better understand this institution’s functions and foundations, trying to ‘get the household right’. These efforts, rather than clarifying the character and the function of the household, have contributed to its indeterminacy by reifying the very institution they seek to analyse. Arguing that these efforts fundamentally miss the point of examining the household, this paper introduces a different framework of analysis that addresses the household not as a fixed object of research, but as a local construction that embodies flows of power and knowledge both within and transcending the local. Using the example of varying constructions of the household in two villages in Ghana’s Central Region, this article illustrates how such an approach allows us to address the various functions of the household as particular embodiments of these flows, an approach that better explains the endurance or ephemerality of these functions. Such an approach provides a stronger foundation for the consideration of how particular constructions of this institution may have troubling implications for issues like gender equity and sustainability.     

Meteorite impact structures: the good and the bad

Meteorite impact structures are found on all planetary bodies in the Solar System with a solid surface. On many planets, impact craters are the dominant landform. Earth's active geology, however, tends to rapidly erase impact structures from the geological record, although we know currently of 174 confirmed impact sites. Impact events are destructive and have been linked to at least one of the 'big five' mass extinctions over the past 540 Ma. But they also provide certain economic benefits, including the formation of metalliferous ore deposits and hydrocarbon reservoirs. Impact structures can also form new biological niches, which can provide favourable conditions for the survival and evolution of life. Despite this, it was only in the past 40 years that the importance of impact cratering as a geological process was recognized and only during the past 15–20 years that the study of meteorite impact structures has moved into the geological mainstream. There is, therefore, still considerable potential for new and exciting advancements.