Review of Geotechnical Investigations Resulting from the Roermond April 13, 1992 Earthquake

In 1987 the Engineering Geology section of the Delft University of Technology carried out a survey of the SE Netherlands to determine which areas were susceptible to liquefaction based on soil profile, groundwater levels and a Richter scale magnitude 6 earthquake along the principal rift fault through the Netherlands, the Peelrand fault system. The fault system has been active since the Triassic and forms part of the Rhine-North Sea rift system. The last major earthquake along the Peelrand fault was in 1933. Recently, in 1992, A 5.8 magnitude earthquake occurred at Roermond, near to the Dutch-German border. Though damage resulting from the earthquake was limited, remedial works to structures amounted to US$ 50 million in the Netherlands. The paper reviews geotechnical investigations associated with the earthquake carried out in the Netherlands. Much of the damage is attributed to liquefaction; excess pore pressures resulting from the earthquake caused sand vent eruptions, river-dyke failures and slope failures. Comparisons are made between the predictions of 1987 and that which occurred in 1992. Site investigation works are recording geotechnical and building data so as to allow for correlations between extents of damage, ground geotechnical profiles and building design. Models for liquefaction are reviewed to describe the slope failure as well as the sand vent phenomena. Densification of subsoil has been inferred from CPTs taken before and after the earthquake for some sites. Pile foundation damage has been investigated for buildings in Roermond for which their susceptibility to earthquake lateral forces in terms of stiffness and pile head working load is given

Hourly resolved cloud modification factors in the ultraviolet

Cloud impacts on the transfer of ultraviolet (UV) radiation through the atmosphere can be assessed by using a cloud modification factor (CMF). CMF, which is based on total global solar irradiation (SOL<sub>CMF</sub>), has proved to be a solid basis to derive CMFs for the UV radiation (UV<sub>CMF</sub>). This is an advantage, because total global irradiance, the basis for SOL<sub>CMF</sub>, is frequently measured and forecasted by numerical weather prediction systems and includes all relevant effects for radiation transmission, such as cloud optical depth, different cloud layers, multiple reflection, as well as the distinct difference as to whether the solar disc is obscured by clouds or not. In the UV range clouds decrease the irradiance to a lesser extent than in the visible and infrared spectral range. Thus the relationship between CMFs for solar radiation and for UV-radiation is not straight forward, but will depend on whether, for example, the solar zenith angle (SZA) and wavelength band or action spectrum in the UV have been taken into consideration. Den Outer et al. provide a UV<sub>CMF</sub> algorithm on a daily basis, which accounts for these influences. It requires as input a daily SOL<sub>CMF</sub> and the SZA at noon. The calculation of SOL<sub>CMF</sub> uses the clear-sky algorithm of the European Solar Radiation Atlas to account for varying turbidity impacts. The algorithm's capability to derive hourly UV<sub>CMFs</sub> based on the SZA at the corresponding hour and its worldwide applicability is validated for erythemal UV using observational data retrieved from the databases of the COST-Action 726 on "Long-term changes and climatology of UV radiation over Europe" and the USDA UV-B Monitoring Program. The clear-sky part of the models has proved to be of good quality. Accumulated to daily doses it forms a tight cluster of points to the highest measured daily sums. All sky model performances for hourly resolution are shown to be comparable in accuracy with the well performing daily models of the COST-726 model intercomparison

UV-radiation and health

Jaarlijks krijgen meer dan 51.000 mensen in Nederland te horen dat ze huidkanker hebben en overlijden ruim 900 mensen aan de gevolgen ervan. Sinds 1990 is het aantal gevallen verviervoudigd. Deze stijging is veel sterker dan bij andere vormen van kanker, en een verdere stijging dreigt (met een factor 2 tot 5). De gevaarlijkste vorm van huidkanker komt in Nederland relatief vaak voor, en binnen Europa behoort Nederland tot de koplopers. Blootstelling van de huid aan UV-straling is de voornaamste oorzaak van het ontstaan van huidkanker, en dan vooral door onverstandig zongedrag. De vergrijzing en de aantasting van de ozonlaag blijken slechts een deel van de toename aan huidkanker te verklaren. Het blootstellingsgedrag lijkt de hoofdrol te spelen en daarbij zijn het dragen van minder bedekkende kleding, meer vrije tijd en langere (zon/strand) vakanties van belang, maar ook klimaatverandering en het gebruik van kunstmatige UV-bronnen voor bruining dragen mogelijk bij. De belangrijkste manier om huidkanker te voorkomen is dan ook ervoor te zorgen dat de huid niet verbrandt door de zon of zonnebank. Maar ook zonder te verbranden kan de huid beschadigd raken. Daarom is het verstandig om de huiddelen die veelvuldig worden blootgesteld extra te beschermen en om daarbij rekening te houden met de zonkracht en de duur van het verblijf in de zon. Bij een hoogstaande (zomer)zon tussen 11 en 16 uur is meer bescherming nodig dan 's morgens vroeg en in de namiddag. Behalve aan huidkanker draagt UV-straling bij aan de vorming van staar en veroorzaakt het huidveroudering en sneeuwblindheid. Het is niet wenselijk om de zonblootstelling volledig te vermijden, omdat UV-blootstelling van de huid ook de voornaamste bron is van vitamine D. Deze vitamine is essentieel voor gezonde botten en spieren. Bovendien zijn er aanwijzingen dat vitamine D de kans op darmkanker kan verkleinen. Momenteel is er een felle wetenschappelijke discussie gaande welke hoeveelheid vitamine D de meeste gezondheidswinst oplevert. De kosten van de medische behandeling van huidkanker bedragen naar schatting circa 325 (250-400) miljoen euro per jaar. De kosten voor de behandeling van door UV veroorzaakte staar, worden geschat op 75-150 miljoen euro per jaar. De kosten zijn grotendeels vermijdbaar door verstandiger (zon)gedrag. De actuele zonkrachtmetingen (www.rivm.nl/zonkracht) en betere kennis over (ontwikkelingen in) blootstellingsgedrag en gezondheidseffecten dragen bij aan een goede voorlichting en preventie. Er is alle reden de kennisopbouw met betrekking tot UV-stralingsbescherming te versterken.Every year more than 51,000 new cases of skin cancer are diagnosed in the Netherlands and over 900 fatalities are reported. The number of new skin cancer cases is rising rapidly and since 1990 a fourfold increase has been observed. This increase is much stronger than for other types of cancer, and a further increase is expected (with a factor of 2-5). The incidence of melanoma of the skin in the Netherlands is among the highest in Europe. Exposure of the skin to UV-radiation is the primary cause of skin cancer, and sun-exposure is the primary source of UV-exposure. The increase in skin cancer incidence that has been observed is only partly explained by the ageing of the Dutch population and the depletion of the ozone layer. A change in exposure behaviour is probably the most dominant factor that could explain a major part of the increased skin cancer incidence. Changes in fashion, with more of the body exposed, shorter working hours and longer vacations, including an increase in summer holidays spent in southern Europe are likely causes. Climate change and the use of artificial tanning devices may also contribute. Skin cancer prevention should be focused on the avoidance of UV-induced erythema (sunburn) in solar and artificial exposures. Limiting the chronic exposure of the most exposed skin parts is also very important, because damage to the skin also occurs below the threshold of erythemal doses. It is, therefore, important to provide additional protection for the parts of the skin that are chronically exposed. Solar exposure is the most important UV-source and protection is most needed when the sun is high in the sky, in the summer months between 11:00 am and 16:00 (4 pm). The UV-index is a good indicator; it is much lower in the early morning or late afternoon/early evening. UV-exposure also contributes to the incidence of cataract and causes skin ageing and snow blindness (photokeratitis). Exposure of the skin to solar UV from the sun should not be completely avoided, however, as it is an important source of vitamin D. Vitamin D is essential for healthy bones and muscles, and there are indications that a high vitamin D status lowers the risk of developing colon cancer, and may also be a factor in the development of a number of other cancers and chronic diseases. At present, a scientific debate is ongoing regarding the minimally required and optimal levels of vitamin D, and how to best achieve them. In the Netherlands the estimated costs for medical treatments of skin cancer and precancerous skin lesions amount to 325 million Euro (250-400). Estimated medical costs for the UV-contribution to cataract formation are 75-150 million Euro per year. These costs can be substantially reduced if (solar) UV-exposure is restricted. Prevention is supported by Solar UV-index measurements (www.rivm.nl/zonkracht), and improved knowledge on UV-radiation exposure and associated health effects. Strengthening the knowledge building and dissemination of information about UV-radiation protection is vitally important.Ministerie van VW

Anisotropic multiple scattering in diffuse media

The multiple scattering of scalar waves in diffusive media is investigated by means of the radiative transfer equation. This approach amounts to a resummation of the ladder diagrams of the Born series; it does not rely on the diffusion approximation. Quantitative predictions are obtained, concerning various observables pertaining to optically thick slabs, such as the mean angle-resolved reflected and transmitted intensities, and the shape of the enhanced backscattering cone. Special emphasis is put on the dependence of these quantities on the anisotropy of the cross-section of the individual scatterers, and on the internal reflections due to the optical index mismatch at the boundaries of the sample. The regime of very anisotropic scattering, where the transport mean free path $\ell^*$ is much larger than the scattering mean free path $\ell$, is studied in full detail. For the first time the relevant Schwarzschild-Milne equation is solved exactly in the absence of internal reflections, and asymptotically in the regime of a large index mismatch. An unexpected outcome concerns the angular width of the enhanced backscattering cone, which is predicted to scale as $\Delta\theta\sim\lambda/\sqrt{\ell\ell^*}$, in contrast with the generally accepted $\lambda/\ell^*$ law, derived within the diffusion approximation.Comment: 53 pages TEX, including 2 tables. The 4 figures are sent at reques

Probing helium interfaces with light scattering : from fluid mechanics to statistical physics

We have investigated the formation of helium droplets in two physical situations. In the first one, droplets are atomised from superfluid or normal liquid by a fast helium vapour flow. In the second, droplets of normal liquid are formed inside porous glasses during the process of helium condensation. The context, aims, and results of these experiments are reviewed, with focus on the specificity of light scattering by helium. In particular, we discuss how, for different reasons, the closeness to unity of the index of refraction of helium allows in both cases to minimise the problem of multiple scattering and obtain results which it would not be possible to get using other fluids.Comment: 21 page

Genetic analysis of the vitamin D receptor gene in two epithelial cancers: melanoma and breast cancer case-control studies

<p>Abstract</p> <p>Background</p> <p>Vitamin D serum levels have been found to be related to sun exposure and diet, together with cell differentiation, growth control and consequently, cancer risk. Vitamin D receptor (<it>VDR</it>) genotypes may influence cancer risk; however, no epidemiological studies in sporadic breast cancer (BC) or malignant melanoma (MM) have been performed in a southern European population. In this study, the <it>VDR </it>gene has been evaluated in two epithelial cancers BC and MM.</p> <p>Methods</p> <p>We have conducted an analysis in 549 consecutive and non-related sporadic BC cases and 556 controls, all from the Spanish population, and 283 MM cases and 245 controls. Genotyping analyses were carried out on four putatively functional SNPs within the <it>VDR </it>gene.</p> <p>Results</p> <p>An association with the minor allele A of the non-synonymous SNP rs2228570 (rs10735810, <it>Fok</it>I, Met1Thr) was observed for BC, with an estimated odds ratio (OR) of 1.26 (95% CI = 1.02–1.57; p = 0.036). The synonymous variant rs731236 (<it>Taq</it>I) appeared to be associated with protection from BC (OR = 0.80, 95%CI = 0.64–0.99; p = 0.047). No statistically significant associations with MM were observed for any SNP. Nevertheless, sub-group analyses revealed an association between rs2228570 (<it>FokI</it>) and absence of childhood sunburns (OR = 0.65, p = 0.003), between the 3'utr SNP rs739837 (<it>Bgl</it>I) and fair skin (OR = 1.31, p = 0.048), and between the promoter SNP rs4516035 and the more aggressive tumour location in head-neck and trunk (OR = 1.54, p = 0.020).</p> <p>Conclusion</p> <p>In summary, we observed associations between SNPs in the <it>VDR </it>gene and BC risk, and a comprehensive analysis using clinical and tumour characteristics as outcome variables has revealed potential associations with MM. These associations required confirmation in independent studies.</p

Worldwide variations in artificial skyglow

Open access journalDespite constituting a widespread and significant environmental change, understanding of artificial nighttime skyglow is extremely limited. Until now, published monitoring studies have been local or regional in scope, and typically of short duration. In this first major international compilation of monitoring data we answer several key questions about skyglow properties. Skyglow is observed to vary over four orders of magnitude, a range hundreds of times larger than was the case before artificial light. Nearly all of the study sites were polluted by artificial light. A non-linear relationship is observed between the sky brightness on clear and overcast nights, with a change in behavior near the rural to urban landuse transition. Overcast skies ranged from a third darker to almost 18 times brighter than clear. Clear sky radiances estimated by the World Atlas of Artificial Night Sky Brightness were found to be overestimated by ~25%; our dataset will play an important role in the calibration and ground truthing of future skyglow models. Most of the brightly lit sites darkened as the night progressed, typically by ~5% per hour. The great variation in skyglow radiance observed from site-to-site and with changing meteorological conditions underlines the need for a long-term international monitoring program.MILIEU (FU Berlin)Federal Ministry of Education and Research, GermanyEU COST Action ES1204 (Loss of the Night Network)European Research Council (ERC) under the EU's Seventh Framework Program (FP7/2007-2013)panish Network for Light Pollution StudiesNational Aeronautics and Space Administration (Goddard Space Flight Center)Ohio State UniversityUniversity of IowaThe Adam Mickiewicz Universit

Performance of the LHCb outer tracker

The LHCb Outer Tracker is a gaseous detector covering an area of 5 × 6 m2 with 12 double layers of straw tubes. The detector with its services are described together with the commissioning and calibration procedures. Based on data of the first LHC running period from 2010 to 2012, the performance of the readout electronics and the single hit resolution and efficiency are presented. The efficiency to detect a hit in the central half of the straw is estimated to be 99.2%, and the position resolution is determined to be approximately 200 μm. The Outer Tracker received a dose in the hottest region corresponding to 0.12 C/cm, and no signs of gain deterioration or other ageing effects are observed

Successive Cambia: A Developmental Oddity or an Adaptive Structure?

BackgroundSecondary growth by successive cambia is a rare phenomenon in woody plant species. Only few plant species, within different phylogenetic clades, have secondary growth by more than one vascular cambium. Often, these successive cambia are organised concentrically. In the mangrove genus Avicennia however, the successive cambia seem to have a more complex organisation. This study aimed (i) at understanding the development of successive cambia by giving a three-dimensional description of the hydraulic architecture of Avicennia and (ii) at unveiling the possible adaptive nature of growth by successive cambia through a study of the ecological distribution of plant species with concentric internal phloem.ResultsAvicennia had a complex network of non-cylindrical wood patches, the complexity of which increased with more stressful ecological conditions. As internal phloem has been suggested to play a role in water storage and embolism repair, the spatial organisation of Avicennia wood could provide advantages in the ecologically stressful conditions species of this mangrove genus are growing in. Furthermore, we could observe that 84.9% of the woody shrub and tree species with concentric internal phloem occurred in either dry or saline environments strengthening the hypothesis that successive cambia provide the necessary advantages for survival in harsh environmental conditions.ConclusionsSuccessive cambia are an ecologically important characteristic, which seems strongly related with water-limited environments