The Macro-Social Benefits of Education, Training and Skills in Comparative Perspective [Wider Benefits of Learning Research Report No. 9]

This report, the second from the Centre's strand of comparative research, complements an earlier WBL research report (Education, Equity and Social Cohesion: A Distributional Model) in exploring further themes of societal comparison and the distributional effects of education systems. Despite generally high levels of educational attainment there is huge diversity amongst Western Societies in terms of crime, tolerance, trust and social cohesion. In this report, we take a comparative approach to investigating relationships between education and these outcomes at a societal level. Through an interdisciplinary review of literatures from sociology, history, economics and psychology we examine the role of education systems from a number of countries in influencing trends in, and levels of, these variables. Whilst the importance of country and historical context is stressed throughout we arrive at some general conclusions concerning the role of education systems in the development of various forms of social cohesion. This report will be of interest to policy makers, researchers and practitioners who are interested in the social impact of education systems. In particular, we examine implications for current UK policy targeted at increasing national educational attainment

Education and Social Cohesion: Re-Centering the Debate

Social Capital theory has tended to treat social cohesion as a mere aggregation of individual and community level characteristics, ignoring the long tradition of theory on social solidarity and social cohesion at the societal level. However, the key indicators of social capital – associational membership and social trust – do not co-vary cross nationally and societies rich in community level social capital are not always cohesive societies. Social capital and societal cohesion are not necessarily the same thing and education may have different effects on each. This article seeks to put the analysis of education and societal cohesion back in the centre of the picture. We do this firstly through a critical review of some of the existing literature on education and social capital which points to the limitations of individual level analysis of what are fundamentally societal issues. Secondly, we outline some alternative models for understanding how education impacts on social cohesion in different societies, drawing on an analysis of some of the aggregated cross-national data on skills, income distribution and various indicators of social cohesion. The argument suggests some causal mechanisms for the social impacts of education that are quite different from those which normally underpin arguments about human and social capital

The chimera of competitiveness: varieties of capitalism and the economic crisis

In this paper we assess the different definitions and theories of economic competitiveness at the firm and national levels. First we contrast the theories of classical liberal economists with those of the German historical school of national economics, noting the importance of the historical school for theories of national economic competitiveness. Drawing on the comparative political economy literature on ‘varieties of capitalism’, we hen discuss the factors underlying competitiveness in social market economies, social democratic economies, and liberal economies. These models f capitalism are compared under six headings: labour markets and labour market institutions; financial markets; corporate funding and governance; inter-firm relations; the role of the state; and economic culture and history. In the penultimate section of the paper we discuss how the different odels of capitalism have responded to the economic crisis and the impact of the crisis on their economic competitiveness. The paper concludes with a summary of the key points to emerge from the analysis and looks to how the scene may evolve as national economies begin to adapt

Education, Equity and Social Cohesion : A Distributional Model [Wider Benefits of Learning Research Report No. 7]

This report - the first from the Centre’s comparative strand of research - focuses on the effects of education on social cohesion at the societal level. The research involved two elements. The first was a theoretical analysis and critique of models in the existing international and comparative literature on education, social capital and social cohesion. This led to the development of a new hypothetical model relating skills distribution to social cohesion. The second part of the research used cross-national, quantitative techniques to test the model on aggregated data for 15 countries. The analysis suggests that educational distribution may be a very significant influence on societal cohesion in certain contexts. Improving levels of education alone may not foster social solidarity if inequalities of skill and income persist. The findings here have important policy implications. Existing policies focus on developing the individual resources and competences which will help to build social capital and community cohesion. However, these will not necessarily impact on cohesion at the societal level. Creating a more cohesive society is likely to require policies that are also designed to increase equality through narrowing educational outcomes

Learning, Continuity and Change in Adult Life [Wider Benefits of Learning Research Report No. 3]

This report presents results from extensive fieldwork carried out by the Wider Benefits of Learning research team. It presents an original analytical framework developed specifically for this study, combined with empirical results from 140 in-depth biographical interviews in three different areas of England. The interviews explore the way learning affects people’s health and well-being; their family lives; and their engagement in civic activity. The report addresses these effects at both an individual and collective level. It concludes with a set of significant policy implications

The relevance of aerosol in the retrieval of tropospheric NO2 from satellite - a study of model data applicability

Nitrogen dioxide (NO2) is a key pollutant in the troposphere, being one of the main precursors of tropospheric ozone, and source of nitric acid, as well as contributing to global climate change. Tropospheric NO2 vertical columns can be determined from satellite observations, although some uncertainties are still associated with the retrieval process. The conversion from measured slant columns to vertical columns is accomplished with airmass factors (AMF) that are determined by radiative transfer (RT) models. While the measurement (instrumental) conditions are well assessed, improvement is still needed regarding the a priori information of atmospheric characteristics required for the estimation of AMFs (e.g., vertical distribution of the gas, aerosol loading and clouds). This thesis presents a sensitivity study focused on the impact of aerosol on the tropospheric NO2 AMF. Optical properties, size distribution, and vertical distribution of the aerosol were varied within several scenarios. Overall, the results show a tendency for two main opposite effects. On the one hand, enhancement of the measurement sensitivity occurs by means of multiple scattering, when aerosol is mixed with the trace gas. On the other hand, a shielding effect by an aerosol layer located above the NO2 is also verified. The identified pivotal factors for the AMF calculations were the relative vertical distribution of aerosol and NO2, the aerosol optical depth and the single scattering albedo, as well as the surface reflectance. A case study was developed, focusing on the impact on the NO2 measurements of volcanic ash emitted from Eyjafjallajökull during the spring of 2010. Aerosol and NO2 data from the EURAD chemical transport model (CTM) were used to design scenarios for the RT calculations. A small variation of AMFs was found, revealing that, in the days and region analysed, the satellite observations of NO2 were not significantly affected by the mentioned eruption. Nonetheless, it was verified that the conclusions of the study are dependent on the accuracy of the CTM data, and on the approach employed to account for (and determine) aerosol optical properties. Such findings highlight the potential challenges that can be faced in the future if model data are used in satellite retrievals. In addition, a model evaluation performed within the GEMS project is described, where global stratospheric and tropospheric NO2 columns predicted by two chemical transport models MOZART and TM5 are compared with SCIAMACHY observations. The evaluation exercise allowed for the identification of flaws in the model systems, showing problems with the prediction of high levels of pollution in some regions (e.g., East-Asia), and with the simulation of NO2 concentrations during biomass burning events

Enabling the Participation of People with Parkinson's and Their Caregivers in Co-Inquiry around Collectivist Health Technologies

While user participation is central to HCI, co-inquiry takes this further by having participants direct and control research from conceptualisation to completion. We describe a co-inquiry, conducted over 16 months with a Parkinson's support group. We explored how the participation of members might be enabled across multiple stages of a research project, from the generation of research questions to the development of a prototype. Participants directed the research into developing alternative modes of information provision, resulting in ‘Parkinson’s Radio’ — a collectivist health information service produced and edited by members of the support group. We reflect on how we supported participation at different stages of the project and the successes and challenges faced by the team. We contribute insights into the design of collectivist health technologies for this group, and discuss opportunities and tensions for conducting co-inquiry in HCI research

MarcoPolo-R: Near Earth Asteroid Sample Return Mission candidate as ESA-M3 class mission

MarcoPolo-R is a sample return mission to a primitive Near-Earth Asteroid (NEA) selected in February 2011 for the Assessment Study Phase at ESA in the framework of ESAfs Cosmic Vision 2 program. MarcoPolo-R is a European-led mission with a proposed NASA contribution. MarcoPolo-R takes advantage of three industrial studies completed as part of the previous Marco Polo mission (see ESA/SRE (2009)3). The aim of the new Assessment Study is to reduce the cost of the mission while maintaining its high science level, on the basis of advanced studies and technologies, as well as optimization of the mission. MarcoPolo-R will rendezvous with a unique kind of target, a primitive binary NEA, scientifically characterize it at multiple scales, and return a unique pristine sample to Earth unaltered by the atmospheric entry process or terrestrial weathering. The baseline target of MarcoPolo-R is the primitive binary NEA (175706) 1996 FG3, which offers a very efficient operational and technical mission profile. A binary target also provides enhanced science return: the choice of this target will allow new investigations to be performed more easily compared to a single object, and also enables investigations of the fascinating geology and geophysics of asteroids that are impossible to obtain from a single object. Precise measurements of the mutual orbit and rotation state of both components can be used to probe higher-level harmonics of the gravitational potential, and therefore the internal structure. A unique opportunity is offered to study the dynamical evolution driven by the YORP/Yarkovsky thermal effects. Possible migration of regolith on the primary from poles to equator allows the increasing maturity of asteroidal regolith with time to be expressed as a latitude-dependent trend, with the most-weathered material at the equator matching what is seen in the secondary. MarcoPolo-R will allow us to study the most primitive materials available to investigate early solar system formation processes. Moreover, MarcoPolo-R will provide a sample from a known target with known geological context. Direct investigation of both the regolith and fresh interior fragments is also impossible by any means other than sample return. The main goal of the MarcoPolo-R mission is to return unaltered NEA material for detailed analysis in ground-based laboratories. The limited sampling provided by meteorites does not offer the most primitive material available in near-Earth space. More primitive material, having experienced less alteration on the asteroid, will be more friable and would not survive atmospheric entry in any discernible amount. Only in the laboratory can instruments with the necessary precision and sensitivity be applied to individual components of the complex mixture of materials that forms an asteroid regolith, to determine their precise chemical and isotopic composition. Such measurements are vital for revealing the evidence of stellar, interstellar medium, pre-solar nebula and parent body processes that are retained in primitive asteroidal material, unaltered by atmospheric entry or terrestrial contamination. It is no surprise therefore that sample return missions are considered a priority by a number of the leading space agencies

STAGES: the Space Telescope A901/2 Galaxy Evolution Survey

We present an overview of the Space Telescope A901/2 Galaxy Evolution Survey (STAGES). STAGES is a multiwavelength project designed to probe physical drivers of galaxy evolution across a wide range of environments and luminosity. A complex multi-cluster system at z~0.165 has been the subject of an 80-orbit F606W HST/ACS mosaic covering the full 0.5x0.5 (~5x5 Mpc^2) span of the supercluster. Extensive multiwavelength observations with XMM-Newton, GALEX, Spitzer, 2dF, GMRT, and the 17-band COMBO-17 photometric redshift survey complement the HST imaging. Our survey goals include simultaneously linking galaxy morphology with other observables such as age, star-formation rate, nuclear activity, and stellar mass. In addition, with the multiwavelength dataset and new high resolution mass maps from gravitational lensing, we are able to disentangle the large-scale structure of the system. By examining all aspects of environment we will be able to evaluate the relative importance of the dark matter halos, the local galaxy density, and the hot X-ray gas in driving galaxy transformation. This paper describes the HST imaging, data reduction, and creation of a master catalogue. We perform Sersic fitting on the HST images and conduct associated simulations to quantify completeness. In addition, we present the COMBO-17 photometric redshift catalogue and estimates of stellar masses and star-formation rates for this field. We define galaxy and cluster sample selection criteria which will be the basis for forthcoming science analyses, and present a compilation of notable objects in the field. Finally, we describe the further multiwavelength observations and announce public access to the data and catalogues.Comment: 29 pages, 22 figures; accepted to MNRAS. Full data release available at http://www.nottingham.ac.uk/astronomy/stage