13,367 research outputs found
University of Exeter Institutional Rights Retention Policy
No full textRights Retention refers to the practice of authors retaining certain rights to their work, including the rights to share, reuse and distribute it, rather than signing these rights over to a publisher.
The University of Exeter waives ownership of, and acknowledges that members of staff own the copyright to, scholarly works they create. In exchange, authors grant the University a non-exclusive, irrevocable, worldwide, royalty-free licence to make manuscripts of their scholarly articles publicly available under a Creative Commons Attribution (CC BY) licence or a similar licence terms.
The CC BY licence is applied to the author accepted manuscript version at submission, giving precedence over any subsequent publisher's licensing agreement. This enables authors to retain sufficient rights to deposit their work in a repository and share it as open access immediately upon publication.
The policy applies to journal articles and conference proceedings with an ISSN, submitted from 1 January 2024, authored or co-authored by staff or postgraduate research students whilst they are affiliated with University of Exeter.
Authors should include a Rights Retention statement in their manuscript at submission and in any covering letter: “For the purpose of open access, the author has applied a Creative Commons Attribution (CC BY) licence to any Author Accepted Manuscript version arising from this submission".
After acceptance, authors should upload the author accepted manuscript version via Symplectic to ORE, when this is required for funder or REF compliance, in line with the Institutional Open Access Policy
Exeter cathedral and its restoration /
No full textErrata inserted.2 of the illustrations are albumen prints.History and description of Exeter catherdral. -- Transcripts of four sermons presented at the re-opening of the cathedral (October 18 & 19, 1877). -- Funeral sermon for Sir Gilbert Scott (April 7, 1878).Mode of access: Internet
Exeter Cathedral
No full textMedium: etchingprintssigned."Exeter Cathedral" [1959.3098.000.000], King, Daniel, Newcourt, RichardExtent: image (sheet trimmed to image)Extent: sheet (adhered
James Morwood, The Tragedies of Sophocles. Exeter, Bristol Phoenix Press, 2008
No full textDonnet Daniel. James Morwood, The Tragedies of Sophocles. Exeter, Bristol Phoenix Press, 2008. In: L'antiquité classique, Tome 79, 2010. pp. 366-367
Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetized molecular cloud cores (dataset)
No full textThe XZ compressed tarballs in this repository contain the binary output data from the smoothed particle radiation magnetohydrodynamics (SPRMHD) calculations presented in the paper.The tarballs are named according to the following scheme: mAAMBB[R][-rCCC].tar.xz. Here, the letters AA represent the mass-to-flux ratio used in the calculation, e.g. a ratio of 5 would imply AA=05, and so on. The letters BB represent the turbulent Mach number multiplied by ten, e.g. Mach 0.1 entails BB=01. The presence of the letter R indicates a calculation using a radiative as opposed to a barotropic equation of state. Finally, the presence of the -rCCC suffix indicates changes to the initial rotational beta, where CCC indicates the beta value multiplied by one hundred, e.g. CCC=001 implies a beta of 0.01. This nomenclature is identical to column 1 of Table 1 in the published paper, which also details any other initial conditions which are relevant.Within each tarball are a number of FORTRAN unformatted binary files in big-endian format. These files are named according to the scheme DAT????. In all the calculations without an -rCCC suffix, these are spaced at one-hundredths of a free-fall time, so that, e.g., DAT0050 corresponds to one-half of a free-fall time. In the -rCCC calculations the temporal spacing is more complex. Until one free-fall time the spacing is as before, however after that point the binary outputs are separated by 1/1600th of a free-fall time, so that DAT0101 corresponds to 1601/1600 free-fall times, and so on.The data files can be read using the open source tool SPLASH written by Daniel Price (see http://users.monash.edu.au/~dprice/splash/). This tool was also used to produce all the rendered figures in the paper. Other figures were produced from data derived from the binary files.The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/32997This is the dataset that was used to produce the paper published in MNRAS. Included are the binary dump files from all eighteen of the calculations in the paper.Science and Technology Facilities CouncilEuropean Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013)This work used the DiRAC Complexity system, operated by the University of Leicester IT Services, which forms part of the STFC DiRAC HPC Facility (www.dirac.ac.uk). This equipment is funded by BIS National E-Infrastructure capital grant ST/K000373/1 and STFC DiRAC Operations grant ST/K0003259/1. DiRAC is part of the National E-Infrastructure.Calculations were also performed on the University of Exeter Supercomputer, a DiRAC Facility jointly funded by STFC, the Large Facilities Capital Fund of BIS and the University of Exeter
Submission to Home Office Immigration Detention Consultation 2018
No full textWritten evidence to the Home Affairs Committee immigration detention inquiry 2018 submitted by Professor Nick Gill (University of Exeter), Dr Daniel
Fisher (University of Exeter), Jennifer Smith (University of Newcastle) and Andrew
Burridge (University of Exeter) (IDD0008
Media content analysis, May 2011. News Media Coverage and Information in Combined Elections (dataset)
No full textStatistical data files relating the impact of different election contexts and media coverage on the referendum vote of 2011
The censor without, the censor within: the resistance of Johnstone’s improv to the social and political pressures of 1950s Britain
No full textKeith Johnstone's improv, popularly known through the Theatresports format, was forged in the cultural and historical context of 1950s Britain. In this paper I will argue that Johnstone's incarnation of theatrical improvisation was defined by its reaction to the normalising forces exerted by the social elite upon the broader population and by civilised society upon the individual.
Johnstone's improv was a reaction against the Lord Chamberlain’s power to censor the British stage and a challenge to the internalised 'censor' British society of the time implanted in the minds of his students, stunting their creative imaginations. Johnstone borrowed elements of professional wrestling to break down the regimented conventions of the theatre space and enliven the spectator-performer relationship. As well as echoing Roland Barthes’ idealistic analysis of professional wrestling (Barthes, 1984: n.p.), Johnstone’s improv shares Barthes’ critique of the authority of the author and allows meaning to be generated out of the encounter between performers and spectators in the instant of the performance’s emergence. Through these processes, Johnstone’s improv defies the censor without (The Lord Chamberlain) by rooting out the censor within (the socially learnt inhibitions to the creative imagination).
By delineating the political and social pressures at play in the historical context of 1950s Britain and the ways that the stylistic conventions of Johnstone's improv resist and subvert these forces, I will demonstrate the emancipatory power latent in this mode of popular performance. This is a particularly timely analysis given the increasing authority of free market economics to dictate what appears on contemporary British stages, and the internalised censor that panoptical CCTV and social media is implanting within the minds of British citizens today
'Behindhand with their countrymen': Literary culture and economic decline in eighteenth-century Exeter
No full textThis is the author accepted manuscript. The final version is available from Johns Hopkins University Press via the DOI in this record.This article investigates the history of writing and printing in eighteenth-century Exeter. Writing in Exeter flourished during the same decades in which the city itself underwent a serious decline; and local authors, proud of belonging to what had, historically, been one of Britain’s greatest cities, had to operate within a marketplace dominated by a metropolitan literary culture contemptuous of provincialism. Surveying the literary works written and printed in eighteenth-century Exeter, this article explores the ways in which these authors addressed the creative and logistical challenges which confronted eighteenth-century writers who lived and worked within ‘provincial’ contexts
Smoothed particle magnetohydrodynamic simulations of protostellar outflows with misaligned magnetic field and rotation axes (dataset)
No full textThe compressed tarballs in this repository contain the binary output data from the SPMHD (smoothed particle magnetohydrodynamics) simulation presented in the paper. The data is a Fortran binary file in big-endian format. The DAT???? files are dumps of the simulation spaced every 1/100 of a free-fall time and can be read in Splash (Written by Daniel Price, see http://users.monash.edu.au/~dprice/splash/). The Atest_? and Ptest_? files contain information on accreted particles and sink particles respectively (again in big-endian format). The two Fortran programs in utils.tar.xz can read these files and output ASCII data. The tarballs themselves are named according to the following scheme: theta_*.tar.xz are the 1.5 million particle simulations presented as the main result of the paper, where theta_0.tar.xz is a fully aligned model and theta_90.tar.xz is fully misaligned (i.e. theta = 90) &c.; lowres_*.tar.xz are the two low-resolution collapse simulations earlier in the paper and disc_*.tar.xz are the two test models. For both the low-resolution and test models, `clean' denotes the result of using and unmodified code and `hav' denotes the new formalism presented in the paper. All the plots in the paper, except for Figs. 13 and 14, can be produced using Splash and the `DAT' files directly. Figs. 13 and 14 use the data extracted from the `A' and `P' files.The journal article associated with this datast was published in Monthly Notices of the Royal Astronomical Society Vol. 451 (1), pp 288-299. doi: 10.1093/mnras/stv957 and is in ORE at http://hdl.handle.net/10871/19588This is the dataset that was used to produce the paper published in MNRAS. Included are the binary dump files from each of the simulations in the paper and two utilities that can be used to produce an ASCII file detailing accreted particles.Science and Technology Facilities Council (STFC)European Research Council (ERC)Australian Research Council (ARC)University of Exeter Supercomputer: jointly funded by Science and Technology Facilities Council (STFC), Large Facilities Capital Fund of BIS, and the University of Exeter
DiRac Complexity computer: jointly funded by Science and Technology Facilities Council (STFC) and the Large Facilities Capital Fund of BI
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