Raising awareness of Asperger’s Syndrome amongst coaches and athletes: the power of virtual support networks

The Virtual Alliance for sport technology (V.A.S.T) is an online tool utilised by a community of experts and practitioners to facilitate the generation and sharing of knowledge in order to promote inclusion in sport. The principal aim of the present study was to utilise this platform to create and evaluate an online teaching resource to provide support for coaches working with athletes with Asperger’s Syndrome. At present little information is provided by National governing bodies about Asperger’s, and as a consequence many athletes can be marginalised in sports provision. A methods-driven evaluative framework was adopted in order to assess the impact of the web-tool. Gantt timelines and a programme theory were produced prior to the project, and programme processes were evaluated throughout. Website impact was assessed via triangulation of statistical analysis regarding website usage with interviews conducted with network users. Results were interpreted using a figurational framework to investigate how information about the web-tool was disseminated and transformed through virtual networks of interdependencies which linked participants diagnosed with Asperger syndrome, their coaches and the online community. Results gained from this project are expected to highlight how web-based platforms have the capability to bring together otherwise marginalised groups with virtual networks of sports experts, athletes and practitioners. The implications of these results will increase awareness of participants with Asperger’s syndrome within sport and provide coaches, athletes and policy makers with information that will enable them to effectively teach and support sports participants with Asperger’s syndrome in an athlete-centric manner

Swahili translation and validation of the Warwick Edinburgh Mental Wellbeing Scale (WEMWBS) in adolescents and adults taking part in the girls’ education challenge fund project in Tanzania

Background: The Warwick Edinburgh Mental Wellbeing Scale (WEMWBS) is validated for measuring mental wellbeing in populations aged 11 + and has been translated into 30 + languages. The aims of this study were a) to translate and validate WEMWBS for use in Swahili-speaking populations to facilitate measurement and understanding of wellbeing, evaluation of policy and practice, and enable international comparisons; and b) to examine sociodemographic characteristics associated with higher and lower mental wellbeing in participants in the Girls’ Education Challenge (GEC) project in Tanzania. Methods: A short questionnaire including WEMWBS and similar scales for comparison, socio-demographic information, and self-reported health was translated into Swahili using gold standard methodology. This questionnaire was used to collect data from secondary school students, learner guides, teacher mentors and teachers taking part in the GEC project in Tanzania. Focus groups were used to assess acceptability and comprehensibility of WEMWBS and conceptual understanding of mental wellbeing. These were audio-taped, transcribed and analysed thematically. Internal consistency of WEMWBS, correlation with comparator scales and confirmatory factor analysis were completed as quantitative validation. Finally, multivariable logistic regression was used to explore associations between individual characteristics and ‘high’ and ‘low’ mental wellbeing, defined as the highest and lowest quartile of WEMWBS scores. Results: 3052 students and 574 adults were recruited into the study. Participants reported that WEMWBS was understandable and relevant to their lives. Both WEMWBS and its short form met quantitative standards of reliability and validity, were correlated with comparator scales and met the criteria to determine a single factor structure. For students in the GEC supported government schools: mental wellbeing was higher in students in the final two ‘forms’ of school compared with the first two. In addition: being male, urban residence, the absence of markers of social marginality and better self-reported health were all significantly associated with better mental wellbeing. For adults, urban residence and better self-reported health were associated with better mental wellbeing. Conclusions: The Swahili translation of WEMWBS is available for use. Further work to explore how to intervene to increase mental wellbeing in vulnerable GEC participants is needed

An insight into ancient aeolian processes and post‐Noachian aqueous alteration in Gale crater, Mars, using ChemCam geochemical data from the Greenheugh capping unit

Aeolian processes have shaped and contributed to the geological record in Gale crater, Mars, long after the fluviolacustrine system existed ∼3 Ga ago. Understanding these aeolian deposits, particularly those which have been lithified and show evidence for aqueous alteration, can help to constrain the environment at their time of deposition and the role of liquid water later in Mars’ history. The NASA Curiosity rover investigated a prominent outcrop of aeolian sandstone within the Stimson formation at the Greenheugh pediment as part of its investigation of the Glen Torridon area. In this study, we use geochemical data from ChemCam to constrain the effects of aeolian sedimentary processes, sediment provenance, and diagenesis of the sandstone at the Greenheugh pediment, comparing the Greenheugh data to the results from previous Stimson localities situated 2.5 km north and >200 m lower in elevation. Our results, supported by mineralogical data from CheMin, show that the Stimson formation at the Greenheugh pediment was likely sourced from an olivine-rich unit that may be present farther up the slopes of Gale crater’s central mound. Our results also suggest that the Greenheugh pediment Stimson formation was cemented by surface water runoff such as that which may have formed Gediz Vallis. The lack of alteration features in the Stimson formation at the Greenheugh pediment relative to those of the Emerson and Naukluft plateaus suggests that groundwater was not as available at this locality compared to the others. However, all sites share diagenesis at the unconformity

The high-resolution map of Oxia Planum, Mars; the landing site of the ExoMars Rosalind Franklin rover mission

This 1:30,000 scale geological map describes Oxia Planum, Mars, the landing site for the ExoMars Rosalind Franklin rover mission. The map represents our current understanding of bedrock units and their relationships prior to Rosalind Franklin’s exploration of this location. The map details 15 bedrock units organised into 6 groups and 7 textural and surficial units. The bedrock units were identified using visible and near-infrared remote sensing datasets. The objectives of this map are (i) to identify where the most astrobiologically relevant rocks are likely to be found, (ii) to show where hypotheses about their geological context (within Oxia Planum and in the wider geological history of Mars) can be tested, (iii) to inform both the long-term (hundreds of metres to ∼1 km) and the short-term (tens of metres) activity planning for rover exploration, and (iv) to allow the samples analysed by the rover to be interpreted within their regional geological context.The ExoMars Rosalind Franklin Mission is a partnership between ESA and NASA. The Rosalind Franklin Rover has eight instruments in its ‘Pasteur’ Payload, with Principal Investigators from seven countries all of whom we would like to thank for there support of this project. We would like to acknowledge the following funding bodies, people and institutions supporting the lead authors of this work. We thank the UK Space Agency (UK SA) for funding P. Fawdon, on grants; ST/W002736/1, ST/L00643X/1 and ST/R001413/1, MRB on grants; ST/T002913/1, ST/V001965/1, ST/R001383/1, ST/R001413/1, P. Grindrod on grants; ST/L006456/1, ST/R002355/1, ST/V002678/1 and J. Davis on grants ST/K502388/1, ST/R002355/1, ST/V002678/1 through the ongoing Aurora space exploration programme. C. Orgel was supported by the ESA Research Fellowship Program. Alessandro Frigeri: was funded by the Italian Space Agency (ASI) grant ASI-INAF number 2017-412-H.0 (ExoMars/Ma_MISS) and D. Loizeau was funded by the H2020-COMPET-2015 programme (grant 687302), C. Quantin-Nataf was supported by the French space agency CNES, I. Torres was supported by an ESA Young Graduate Traineeship, A. Nass was supported by Helmholtz Metadata Projects (#ZT-I-PF-3-008). We thank NASA and the HiRISE camera team for data collection support throughout the ExoMars landing site selection and charectorisation process. The USGS for the HiRISE DTM data and maintaining the ISIS and SOCET SET DEM workflows. The authors wish to thank the CaSSIS spacecraft and instrument engineering teams. CaSSIS is a project of the University of Bern and funded through the Swiss Space Office via ESA's PRODEX programme. The instrument hardware development was also supported by the Italian Space Agency (ASI) (ASI-INAF agreement no. I/2020-17-HH.0), INAF/Astronomical Observatory of Padova, and the Space Research Center (CBK) in Warsaw. Support from SGF (Budapest), the University of Arizona (Lunar and Planetary Lab.) and NASA are also gratefully acknowledged. Operations support from the UK Space Agency under grant ST/R003025/1 is also acknowledged. This research has made use of the USGS Integrated Software for Imagers and Spectrometers (ISIS) Technical support for setup of the Multi-Mission Geographic Information System for concurrent team mapping was provided by F. Calef (III) and T. Soliman at NASA JPL and S. de Witte at ESA-ESTEC.This work was supported by Agencia Estatal de Investigación [grant number ID2019-107442RB-C32, MDM-2017-0737]; Agenzia Spaziale Italiana [grant number 2017-412-H.0]; Bundesministerium für Wirtschaft und Technologie [grant number 50 QX 2002]; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Euskal Herriko Unibertsitatea [grant number PES21/88]; Istituto Nazionale di Astrofisica [grant number I/ 060/10/0]; Ministerio de Economía y Competitividad [grant number PID2019-104205GB-C21]; Ministry of Science and Higher Education of the Russian Federation [grant number AAAA-A18-118012290370-6]; National Aeronautics and Space Administration [grant number NNX15AH46G]; Norges Forskningsråd [grant number 223272]; European Union's Horizon 2020 (H2020-COMPET-2015) [grant number 687302 (PTAL)]; Sofja Kovalevskaja Award of the Alexander von Humboldt Foundation; MINECO [grant number PID2019-107442RB-C32]; The Open University [grant number Space Strategic Research Area]; European Union's Horizon 2020 research and innovation programme [grant number 776276]; H2020-COMPET-2015 [grant number 687302]; The Research Council of Norway, Centres of Excellence funding scheme [grant number 223272]; Helmholtz Metadata Projects [grant number ZT-I-PF-3-008]; The Research Council of Norway [grant number 223272]; Swiss Space Office via ESA's PRODEX programme; Ines Torres was supported by an ESA Young Graduate Traineeship; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung [grant number 200021_197293]; Science and Technology Facilities Council [grant number 1967420]; UK Space Agency [grant number ST/K502388/1, ST/R002355/1, ST/V002678/1]. The ExoMars Rosalind Franklin Mission is a partnership between ESA and NASA. The Rosalind Franklin Rover has eight instruments in its ‘Pasteur’ Payload, with Principal Investigators from seven countries all of whom we would like to thank for there support of this project. We would like to acknowledge the following funding bodies, people and institutions supporting the lead authors of this work. We thank the UK Space Agency (UK SA) for funding P. Fawdon, on grants; ST/W002736/1, ST/L00643X/1 and ST/R001413/1, MRB on grants; ST/T002913/1, ST/V001965/1, ST/R001383/1, ST/R001413/1, P. Grindrod on grants; ST/L006456/1, ST/R002355/1, ST/V002678/1 and J. Davis on grants ST/K502388/1, ST/R002355/1, ST/V002678/1 through the ongoing Aurora space exploration programme. C. Orgel was supported by the ESA Research Fellowship Program. Alessandro Frigeri: was funded by the Italian Space Agency (ASI) grant ASI-INAF number 2017-412-H.0 (ExoMars/Ma_MISS) and D. Loizeau was funded by the H2020-COMPET-2015 programme (grant 687302), C. Quantin-Nataf was supported by the French space agency CNES, I. Torres was supported by an ESA Young Graduate Traineeship, A. Nass was supported by Helmholtz Metadata Projects (#ZT-I-PF-3-008). We thank NASA and the HiRISE camera team for data collection support throughout the ExoMars landing site selection and charectorisation process. The USGS for the HiRISE DTM data and maintaining the ISIS and SOCET SET DEM workflows. The authors wish to thank the CaSSIS spacecraft and instrument engineering teams. CaSSIS is a project of the University of Bern and funded through the Swiss Space Office via ESA's PRODEX programme. The instrument hardware development was also supported by the Italian Space Agency (ASI) (ASI-INAF agreement no. I/2020-17-HH.0), INAF/Astronomical Observatory of Padova, and the Space Research Center (CBK) in Warsaw. Support from SGF (Budapest), the University of Arizona (Lunar and Planetary Lab.) and NASA are also gratefully acknowledged. Operations support from the UK Space Agency under grant ST/R003025/1 is also acknowledged. This research has made use of the USGS Integrated Software for Imagers and Spectrometers (ISIS) Technical support for setup of the Multi-Mission Geographic Information System for concurrent team mapping was provided by F. Calef (III) and T. Soliman at NASA JPL and S. de Witte at ESA-ESTEC.Peer reviewe

The high-resolution map of Oxia Planum, Mars; the landing site of the ExoMars Rosalind Franklin rover mission

This 1:30,000 scale geological map describes Oxia Planum, Mars, the landing site for the ExoMars Rosalind Franklin rover mission. The map represents our current understanding of bedrock units and their relationships prior to Rosalind Franklin’s exploration of this location. The map details 15 bedrock units organised into 6 groups and 7 textural and surficial units. The bedrock units were identified using visible and near-infrared remote sensing datasets. The objectives of this map are (i) to identify where the most astrobiologically relevant rocks are likely to be found, (ii) to show where hypotheses about their geological context (within Oxia Planum and in the wider geological history of Mars) can be tested, (iii) to inform both the long-term (hundreds of metres to ∼1 km) and the short-term (tens of metres) activity planning for rover exploration, and (iv) to allow the samples analysed by the rover to be interpreted within their regional geological context

Religious diversity in Australia:Rethinking social cohesion

This paper argues for a reconsideration of social cohesion as an analytical concept and a policy goal in response to increasing levels of religious diversity in contemporary Australia. In recent decades, Australian has seen a revitalization of religion, increasing numbers of those who do not identify with a religion (the ”nones”), and the growth of religious minorities, including Islam, Buddhism, Hinduism, and Sikhism. These changes are often understood as problematic for social cohesion. In this paper, we review some conceptualizations of social cohesion and religious diversity in Australia, arguing that the concept of social cohesion, despite its initial promise, is ultimately problematic, particularly when it is used to defend privilege. We survey Australian policy responses to religious diversity, noting that these are varied, often piecemeal, and that the hyperdiverse state of Victoria generally has the most sophisticated set of public policies. We conclude with a call for more nuanced and contextualized analyses of religious diversity and social cohesion in Australia. Religious diversity presents both opportunities as well as challenges to social cohesion. Both these aspects need to be considered in the formation of policy responses

CLIMATE AND DIAGENETIC IMPLICATIONS OF POSSIBLE SOFT SEDIMENT DEFORMATION OF THE BASAL AEOLIAN STIMSON SEDIMENTS IN GALE CRATER

International audienceThe accumulated sediments and erosional unconformities in the deposits of Mt. Sharp of Gale Crater record multiple periods of wet and dry cycles similar to the episodic climate aridification and later brief wet periods found across Mars [1]. Early post impact (~3.6 billion), an extended period of lacustrine conditions prevailed, leading to over 300 m of lake sediments exposed at the base of Mt. Sharp [2]. This was followed by eolian sediment accumulation perhaps with fluvial deposition interludes [3]. Accumulation ceased and extensive wind erosion shaped Mt. Sharp to nearly its present topography. This erosional event is recorded as the Siccar Point unconformity, which is preserved under a “mound skirting unit”, which locally has been documented to be the remnants of an extensive, large-scale dune field – the Stimson formation [4].The Stimson formation and the Siccar Point unconformity are predominantly exposed along the Greenheugh pediment, a planar sloping topographicfeature that lies downslope of Gediz Vallis [5].Overlying the Stimson formation on the Greenheugh pediment is the remnant of a fan deposit [5] that may have advanced into transient deep lakes in Gale crater that postdated Stimson fm. deposition [6]. Investigation of the northern exposure of this pediment revealed that the sediments underlying the Siccar Point unconformity (the Carolyn Shoemaker formation) had undergone extensive diagenetic alteration. Nodular alteration was also noted in the basal sediments of the Stimson. These water-driven alterations led to hypotheses about the source and pathways of water which included the possibility that groundwater (derived from runoff from Mt. Sharp) may have developed in the overlying Stimson on the much less permeable fine-grained underlying lake sediments [7].Here we report that along a southern exposure of the pediment, 0.9 km upslope from the northern area previously investigated (Tower butte area), adiscontinuous thin massive unit lies at the boundary between the distinctive eolian dune bedding of Stimson and the underlying strongly diagenetically altered Carolyn Shoemaker formation. We propose that this unit is a result of soft-sediment deformation, a condition favored by groundwater saturation of this basal unit, and possibly driven by impact events before lithification of the Stimson

CLIMATE AND DIAGENETIC IMPLICATIONS OF POSSIBLE SOFT SEDIMENT DEFORMATION OF THE BASAL AEOLIAN STIMSON SEDIMENTS IN GALE CRATER

International audienceThe accumulated sediments and erosional unconformities in the deposits of Mt. Sharp of Gale Crater record multiple periods of wet and dry cycles similar to the episodic climate aridification and later brief wet periods found across Mars [1]. Early post impact (~3.6 billion), an extended period of lacustrine conditions prevailed, leading to over 300 m of lake sediments exposed at the base of Mt. Sharp [2]. This was followed by eolian sediment accumulation perhaps with fluvial deposition interludes [3]. Accumulation ceased and extensive wind erosion shaped Mt. Sharp to nearly its present topography. This erosional event is recorded as the Siccar Point unconformity, which is preserved under a “mound skirting unit”, which locally has been documented to be the remnants of an extensive, large-scale dune field – the Stimson formation [4].The Stimson formation and the Siccar Point unconformity are predominantly exposed along the Greenheugh pediment, a planar sloping topographicfeature that lies downslope of Gediz Vallis [5].Overlying the Stimson formation on the Greenheugh pediment is the remnant of a fan deposit [5] that may have advanced into transient deep lakes in Gale crater that postdated Stimson fm. deposition [6]. Investigation of the northern exposure of this pediment revealed that the sediments underlying the Siccar Point unconformity (the Carolyn Shoemaker formation) had undergone extensive diagenetic alteration. Nodular alteration was also noted in the basal sediments of the Stimson. These water-driven alterations led to hypotheses about the source and pathways of water which included the possibility that groundwater (derived from runoff from Mt. Sharp) may have developed in the overlying Stimson on the much less permeable fine-grained underlying lake sediments [7].Here we report that along a southern exposure of the pediment, 0.9 km upslope from the northern area previously investigated (Tower butte area), adiscontinuous thin massive unit lies at the boundary between the distinctive eolian dune bedding of Stimson and the underlying strongly diagenetically altered Carolyn Shoemaker formation. We propose that this unit is a result of soft-sediment deformation, a condition favored by groundwater saturation of this basal unit, and possibly driven by impact events before lithification of the Stimson

The Stimson formation at the Greenheugh pediment: stratigraphy, architecture, and correlation

International audienc