cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.6084/m9.figshare.23814993.v1
title: Design of a Modular Annular Centrifugal Contactor for Lab-Scale Counter-Current Multistage Solvent Extraction

description: Annular centrifugal contactors (ACCs) have appealing properties as counter-current multistage solvent extraction (SX) equipment, allowing high throughput at short residence times, small liquid hold-up, and small footprint. The number of commercial suppliers of laboratory-scale ACCs is limited, and their designs have restricted flexibility. Commercial 25 mm diameter ACCs were customized with transparent PMMA surroundings of the mixing zones, allowing visual process monitoring and identification of operational malfunctions. The separation zone of several rotors was lengthened compared to the factory design, which allows longer average residence times in the modified contactors, while keeping the organic flow rate constant in the bank of interconnected contactors. The Couette gap could be increased or decreased without affecting the mixing performance. A 3D-printed stator allows for more efficient draining of the light and heavy phases, and reduces liquid hold-up and volumes required to efficiently achieve steady-state conditions in the process. The hydrodynamic performance of the modified equipment was demonstrated by a SX process of uranium with TBP. First a literature data set of distribution ratios for uranium in HNO<sub>3</sub> and 30% TBP diluted in dodecane was utilized to create an empirical model in SX Process simulation software. A flowsheet was designed to validate the model, and it provides an example of the methodology to progress from batch to multistage process. Online density measurements were used to monitor and control the uranium concentrations, and to achieve the desired high metal loading steady-state conditions. It was demonstrated that ruthenium decontamination from uranium could be improved in modified ACCs with longer residence time in the mixing zones of the scrubbing section.
DOI: 10.6084/m9.figshare.23921238.v1
title: The output files of MEANGS when assembling mitogenome of the white-spotted bamboo shark

description: The output files of MEANGS The output files of MEANGS when assembling mitogenome of the white-spotted bamboo shark, based on 0.5 Gb (Out-0.5G) and 5 Gb (Out-5G) whole genome sequencing data.
DOI: 10.24378/exe.104
title: Enhancing the magneto-optical Kerr effect through the use of a plasmonic antenna (dataset)

description: This folder contains data underlying the publication "Enhancing the magneto-optical Kerr effect through the use of a plasmonic antenna".
description: The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/32033
DOI: 10.24378/exe.606
title: The acoustic phase resonances and surface waves supported by a compound rigid grating (dataset)

description: We study the radiative and bound acoustic modes supported by a rigid grating formed of three same-depth, narrow grooves per unit cell. One of the grooves is twice the width of the other two, forming a 'compound' grating. The structure supports so-called 'phase' resonances where the phase difference of the pressure field between the grooves on resonance varies by multiples of π. We explore the dispersion of these modes experimentally by monitoring the specularly reflected signal as a function of the angle of incidence. In addition, by near-field excitation, the dispersion of the non-radiative surface modes has been characterised. Our results are compared with the predictions of a finite element method model.
description: Included are 3 COMSOL models which were used for the finite element models. Surface-data.zip is the experimental data used to calculate the surface plots. Experimental data dispersion shows the experimental data used for the radiative experiments. Figure.zip contain all figures in .eps, .svg and .pdf format.
description: The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/33385
DOI: 10.24378/exe.83
title: On the diversity and statistical properties of protostellar discs (dataset)

description: This is the dataset that was used to produce Appendix B for the published MNRAS paper: Bate (2018, DOI:10.1093/mnras/sty169). It contains the output from the SPH simulations discussed in the appendix, including dump files.
description: This repository contains the datasets from the original smoothed particle hydrodynamics (SPH) calculations that were performed for Appendix B of the paper (Bate 2018, DOI:10.1093/mnras/sty169). The dataset from the SPH calculation analysed in the main sections of the paper has already been published on ORE (http://hdl.handle.net/10871/14881). Output from the SPH calculations are contained in the files: Bate2018_Besphere.zip for the calculations discussed in Appendix B1, and in Bate2018_Binary_beta020.zip for the calculations discussed in Appendix B2. When unzipped, each of these directories contains appropriately named sub-directories for each of the separate calculations performed using different numbers of SPH particles. A number of ASCII files give the setup parameters and output logs for each of the calculations. For each calculation in Bate2018_Besphere, the SPH dump files for each calculation begin at BESP000 at time zero and then are numbered sequentially, changing to BES1000 for the 1000th and later dump files. For each calculation in Bate2018_Binary_beta020, the SPH dump files begin at BB79000 at time zero and then are numbered sequentially. The SPH dump files are Fortran binary files, written in big endian format and generated by the sphNG code. They can be read, visualised, and manipulated using the free, publicly available SPLASH visualisation code (which reads sphNG dump files), written by Daniel Price, that can be downloaded from: http://users.monash.edu.au/~dprice/splash/
description: The journal article associated with this dataset is in ORE: http://hdl.handle.net/10871/32002
DOI: 10.24378/exe.203
title: Shaken and stirred: the effects of turbulence and rotation on disc and outflow formation during the collapse of magnetized molecular cloud cores (dataset)

description: This 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.
description: The XZ compressed tarballs in this repository contain the binary output data from the smoothed particle radiation magnetohydrodynamics (SPRMHD) calculations presented in the paper.
description: 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.
description: 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.
description: 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.
description: The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/32997
DOI: 10.24378/exe.244
title: Investigating the nature of chiral near-field interactions (dataset)

description: This is the dataset used for the Barr et al. (2018) article "Investigating the nature of chiral near-field interactions" published in Physical Review B.
description: The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/33246
DOI: 10.24378/exe.263
title: The effect of extreme ionization rates during the initial collapse of a molecular cloud core (dataset)

description: What cosmic ray ionization rate is required such that a non-ideal magnetohydrodynamics (MHD) simulation of a collapsing molecular cloud will follow the same evolutionary path as an ideal MHD simulation or as a purely hydrodynamics simulation? To investigate this question, we perform three-dimensional smoothed particle non-ideal MHD simulations of the gravitational collapse of rotating, one solar mass, magnetized molecular cloud cores, which include Ohmic resistivity, ambipolar diffusion, and the Hall effect. We assume a uniform grain size of ag = 0.1 μm, and our free parameter is the cosmic ray ionization rate, ζcr. We evolve our models, where possible, until they have produced a first hydrostatic core. Models with ζcr ≳ 10−13 s−1 are indistinguishable from ideal MHD models, and the evolution of the model with ζcr = 10−14 s−1 matches the evolution of the ideal MHD model within 1 per cent when considering maximum density, magnetic energy, and maximum magnetic field strength as a function of time; these results are independent of ag. Models with very low ionization rates (ζcr ≲ 10−24 s−1) are required to approach hydrodynamical collapse, and even lower ionization rates may be required for larger ag. Thus, it is possible to reproduce ideal MHD and purely hydrodynamical collapses using non-ideal MHD given an appropriate cosmic ray ionization rate. However, realistic cosmic ray ionization rates approach neither limit; thus, non-ideal MHD cannot be neglected in star formation simulations.
description: This is all the data created for Wurster, Bate & Price (2018b). This dataset was created using the SPHMD code Phantom, which included v1.2.1 of the NICIL library (Wurster 2016) to calculate the non-ideal MHD coefficients. The data and important files have been uploaded; the data files can be read with either Phantom, or with the graphics programme Splash. The filenames have the prefix Ionisation_. If the second component is a number or pair of number, then that file includes the data for those ionisation rates (specifically the negative of those numbers). If the second part is 'exe', then it includes the executables, graphing scripts, etc.
description: The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/32176
DOI: 10.5281/zenodo.8251951
title: Steering Angle Prediction (SAP)

description: Steering Angle Prediction
DOI: 10.5281/zenodo.8251950
title: Steering Angle Prediction (SAP)

description: Steering Angle Prediction
DOI: 10.5281/zenodo.8251934
title: Glasses Object Detection (OD)

description: Glasses Object Detection
DOI: 10.5281/zenodo.8251933
title: Glasses Object Detection (OD)

description: Glasses Object Detection
DOI: 10.5281/zenodo.8251928
title: Traffic Signs Recognition (TSR)

description: German Traffic Signs Recognition
DOI: 10.5281/zenodo.8251927
title: Traffic Signs Recognition (TSR)

description: German Traffic Signs Recognition
DOI: 10.5281/zenodo.8248311
title: Simplified Preservation of Equal Pathways Solid Element

description: The files contain the raw data of the experiments shown in the article: "Simple Preservation of Equal Pathways Solid Element".
description: We acknowledge financial support from the MPI for Multidisciplinary Sciences, and from the Deutsche Forschungsgemeinschaft (Emmy Noether program Grant AN1316).
DOI: 10.5281/zenodo.8248310
title: Simplified Preservation of Equal Pathways Solid Element

description: The files contain the raw data of the experiments shown in the article: "Simple Preservation of Equal Pathways Solid Element".
description: We acknowledge financial support from the MPI for Multidisciplinary Sciences, and from the Deutsche Forschungsgemeinschaft (Emmy Noether program Grant AN1316).
DOI: 10.6069/ba75-f052
title: Longitudinal evaluation of biomarkers in wound fluids of venous leg ulcers treated with a protease-modulating wound dressing

description: Venous leg ulcers (VLU) represent a clinical challenge and impair the patient’s quality of life. Venous insufficiency is underlying the protracted healing. We report the protein expression pattern for biomarkers in VLU wound fluids and compare these with acute split-thickness wound fluids.

Fifty-seven patients with VLU were recruited and treated for 12 weeks with a protease-modulating polyacrylate wound dressing and a two-layer bandage compression system. Ten patients with acute wounds were followed for 21 days. Wound size decreased from 18.7 ± 12.3 cm2 to 11.75 ± 11.39 cm2 in the VLU cohort, 10 wounds healed completely. Relative wound area reduction reached 48.9% ± 51.9% at week 12. 61.4% of the patients achieved a relative wound area reduction of ≥40% and 50.9% a relative wound area reduction of ≥60%.

IL-1beta, TNF-alpha, and MMP9 concentration ranges were similar in VLU and acute wound fluids. Concentrations of S100A8, S100A9, neutrophil elastase, MMP2, and fibronectin were elevated in VLU wound fluids and decreased significantly in abundance after two weeks of treatment. The values remained low, yet, higher than those of acute wounds. Collagen (I) alpha1 abundance was higher in VLU wound fluids and not significantly regulated.

Our data show a robust healing response in venous leg ulcers treated with a protease-modulating polyacrylate wound dressing. The biomarker pattern in VLU wound fluids changed within the first two weeks and we speculate that this might reflect a decrease of STAT3 influence in the wound bed.
DOI: 10.6084/m9.figshare.23898006.v1
title: Supplementary Material for: Remitting seronegative symmetrical synovitis with pitting edema (RS3PE): A case report of an immune-related adverse event following surgery

description: Immune checkpoint inhibitors (ICIs) have emerged as a novel class of anti-neoplastic agent in oncology. Their integration into practice has been accompanied by “immune-related adverse events” (irAEs) wherein off-target immune responses damage healthy tissues. Severe irAEs can cause irreversible organ dysfunction and death. Despite this, little is known about factors which predispose certain patients to develop irAEs or which precipitate their onset. Here, we report a case of a patient with melanoma who completed adjuvant immunotherapy, underwent elective hip replacement, and developed a rare rheumatologic irAE (remitting seronegative symmetrical synovitis with pitting edema (RS3PE)) post-operatively. Mechanistically, we hypothesize that surgery contributed to irAE pathogenesis as a sensitizing event in which self-antigens were presented to an immune system with diminished peripheral tolerance in the context of recent ICI administration. This case highlights a need for future correlative analyses investigating whether iatrogenic interventions such as surgery might be associated with irAE development.
DOI: 10.25345/c5hx16194
title: MassIVE MSV000092665 - Cross-link MS analysis of human 26S proteasome in complex with RPN13:UCHL5 (with substrate).
title: Cross-link MS analysis of human 26S proteasome in complex with RPN13:UCHL5 with the added ubiquitinated Sic1PY substrate.
DOI: 10.34740/kaggle/dsv/6312156
title: Egypt Gold Prices | Daily Updated
DOI: 10.6084/m9.figshare.23966922
title: Mini dataset for High-resolution single-photon imaging with physics-informed deep learning

description: This is a mini dataset for High-resolution single-photon imaging with physics-informed deep learning to interpret, verify and extend the research for readers. The mini dataset includes the input and output based on our method, as well as the dark count data we calibrated.
DOI: 10.26050/wdcc/ar6.c6damohgl
title: IPCC DDC: MOHC HadGEM3-GC31-LL model output prepared for CMIP6 DAMIP

description: Project: Coupled Model Intercomparison Project Phase 6 (CMIP6) datasets - These data have been generated as part of the internationally-coordinated Coupled Model Intercomparison Project Phase 6 (CMIP6; see also GMD Special Issue: http://www.geosci-model-dev.net/special_issue590.html). The simulation data provides a basis for climate research designed to answer fundamental science questions and serves as resource for authors of the Sixth Assessment Report of the Intergovernmental Panel on Climate Change (IPCC-AR6). CMIP6 is a project coordinated by the Working Group on Coupled Modelling (WGCM) as part of the World Climate Research Programme (WCRP). Phase 6 builds on previous phases executed under the leadership of the Program for Climate Model Diagnosis and Intercomparison (PCMDI) and relies on the Earth System Grid Federation (ESGF) and the Centre for Environmental Data Analysis (CEDA) along with numerous related activities for implementation. The original data is hosted and partially replicated on a federated collection of data nodes, and most of the data relied on by the IPCC is being archived for long-term preservation at the IPCC Data Distribution Centre (IPCC DDC) hosted by the German Climate Computing Center (DKRZ). The project includes simulations from about 120 global climate models and around 45 institutions and organizations worldwide. Summary: These data include the subset used by IPCC AR6 WGI authors of the datasets originally published in ESGF for 'CMIP6.DAMIP.MOHC.HadGEM3-GC31-LL' with the full Data Reference Syntax following the template 'mip_era.activity_id.institution_id.source_id.experiment_id.member_id.table_id.variable_id.grid_label.version'. The HadGEM3-GC3.1-N96ORCA1 climate model, released in 2016, includes the following components: aerosol: UKCA-GLOMAP-mode, atmos: MetUM-HadGEM3-GA7.1 (N96; 192 x 144 longitude/latitude; 85 levels; top level 85 km), land: JULES-HadGEM3-GL7.1, ocean: NEMO-HadGEM3-GO6.0 (eORCA1 tripolar primarily 1 deg with meridional refinement down to 1/3 degree in the tropics; 360 x 330 longitude/latitude; 75 levels; top grid cell 0-1 m), seaIce: CICE-HadGEM3-GSI8 (eORCA1 tripolar primarily 1 deg; 360 x 330 longitude/latitude). The model was run by the Met Office Hadley Centre, Fitzroy Road, Exeter, Devon, EX1 3PB, UK (MOHC) in native nominal resolutions: aerosol: 250 km, atmos: 250 km, land: 250 km, ocean: 100 km, seaIce: 100 km.
DOI: 10.26050/wdcc/ar6.c6damohglsg
title: IPCC DDC: MOHC HadGEM3-GC31-LL model output prepared for CMIP6 DAMIP ssp245-GHG

description: Project: Coupled Model Intercomparison Project Phase 6 (CMIP6) datasets - These data have been generated as part of the internationally-coordinated Coupled Model Intercomparison Project Phase 6 (CMIP6; see also GMD Special Issue: http://www.geosci-model-dev.net/special_issue590.html). The simulation data provides a basis for climate research designed to answer fundamental science questions and serves as resource for authors of the Sixth Assessment Report of the Intergovernmental Panel on Climate Change (IPCC-AR6). CMIP6 is a project coordinated by the Working Group on Coupled Modelling (WGCM) as part of the World Climate Research Programme (WCRP). Phase 6 builds on previous phases executed under the leadership of the Program for Climate Model Diagnosis and Intercomparison (PCMDI) and relies on the Earth System Grid Federation (ESGF) and the Centre for Environmental Data Analysis (CEDA) along with numerous related activities for implementation. The original data is hosted and partially replicated on a federated collection of data nodes, and most of the data relied on by the IPCC is being archived for long-term preservation at the IPCC Data Distribution Centre (IPCC DDC) hosted by the German Climate Computing Center (DKRZ). The project includes simulations from about 120 global climate models and around 45 institutions and organizations worldwide. Summary: These data include the subset used by IPCC AR6 WGI authors of the datasets originally published in ESGF for 'CMIP6.DAMIP.MOHC.HadGEM3-GC31-LL.ssp245-GHG' with the full Data Reference Syntax following the template 'mip_era.activity_id.institution_id.source_id.experiment_id.member_id.table_id.variable_id.grid_label.version'. The HadGEM3-GC3.1-N96ORCA1 climate model, released in 2016, includes the following components: aerosol: UKCA-GLOMAP-mode, atmos: MetUM-HadGEM3-GA7.1 (N96; 192 x 144 longitude/latitude; 85 levels; top level 85 km), land: JULES-HadGEM3-GL7.1, ocean: NEMO-HadGEM3-GO6.0 (eORCA1 tripolar primarily 1 deg with meridional refinement down to 1/3 degree in the tropics; 360 x 330 longitude/latitude; 75 levels; top grid cell 0-1 m), seaIce: CICE-HadGEM3-GSI8 (eORCA1 tripolar primarily 1 deg; 360 x 330 longitude/latitude). The model was run by the Met Office Hadley Centre, Fitzroy Road, Exeter, Devon, EX1 3PB, UK (MOHC) in native nominal resolutions: aerosol: 250 km, atmos: 250 km, land: 250 km, ocean: 100 km, seaIce: 100 km.
DOI: 10.26050/wdcc/ar6.c6damou0
title: IPCC DDC: MOHC UKESM1.0-LL model output prepared for CMIP6 DAMIP

description: Project: Coupled Model Intercomparison Project Phase 6 (CMIP6) datasets - These data have been generated as part of the internationally-coordinated Coupled Model Intercomparison Project Phase 6 (CMIP6; see also GMD Special Issue: http://www.geosci-model-dev.net/special_issue590.html). The simulation data provides a basis for climate research designed to answer fundamental science questions and serves as resource for authors of the Sixth Assessment Report of the Intergovernmental Panel on Climate Change (IPCC-AR6). CMIP6 is a project coordinated by the Working Group on Coupled Modelling (WGCM) as part of the World Climate Research Programme (WCRP). Phase 6 builds on previous phases executed under the leadership of the Program for Climate Model Diagnosis and Intercomparison (PCMDI) and relies on the Earth System Grid Federation (ESGF) and the Centre for Environmental Data Analysis (CEDA) along with numerous related activities for implementation. The original data is hosted and partially replicated on a federated collection of data nodes, and most of the data relied on by the IPCC is being archived for long-term preservation at the IPCC Data Distribution Centre (IPCC DDC) hosted by the German Climate Computing Center (DKRZ). The project includes simulations from about 120 global climate models and around 45 institutions and organizations worldwide. Summary: These data include the subset used by IPCC AR6 WGI authors of the datasets originally published in ESGF for 'CMIP6.DAMIP.MOHC.UKESM1-0-LL' with the full Data Reference Syntax following the template 'mip_era.activity_id.institution_id.source_id.experiment_id.member_id.table_id.variable_id.grid_label.version'. The UKESM1.0-N96ORCA1 climate model, released in 2018, includes the following components: aerosol: UKCA-GLOMAP-mode, atmos: MetUM-HadGEM3-GA7.1 (N96; 192 x 144 longitude/latitude; 85 levels; top level 85 km), atmosChem: UKCA-StratTrop, land: JULES-ES-1.0, ocean: NEMO-HadGEM3-GO6.0 (eORCA1 tripolar primarily 1 deg with meridional refinement down to 1/3 degree in the tropics; 360 x 330 longitude/latitude; 75 levels; top grid cell 0-1 m), ocnBgchem: MEDUSA2, seaIce: CICE-HadGEM3-GSI8 (eORCA1 tripolar primarily 1 deg; 360 x 330 longitude/latitude). The model was run by the Met Office Hadley Centre, Fitzroy Road, Exeter, Devon, EX1 3PB, UK (MOHC) in native nominal resolutions: aerosol: 250 km, atmos: 250 km, atmosChem: 250 km, land: 250 km, ocean: 100 km, ocnBgchem: 100 km, seaIce: 100 km.