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209 results for “probabilistic”

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zenodo36/100

Seamless short- to mid-term probabilistic wind power forecasting: Forecasting Results

<div> <div> <div> <div> <div>This dataset contains the predicted time series and the forecast assessment conducted in the paper <strong>Seamless short- to mid-term probabilistic wind power forecasting</strong>.</div> </div> </div> </div> </div>

opencc-by-4.0Nov 2024View details →
zenodo36/100

A probabilistic map of Costa Rican peatlands based on vegetation, ecosystem, and soil inventories

<p>There are the GIS files that accompany a peer-reviewed article.</p> <p>This is the first published effort aimed at developing a peatland map for Costa Rica. A probabilistic approach using vegetation, ecosystem, and soil datasets was used to predict the distribution and extent of peatlands below 700 m in elevation. High-elevation sites found in the Talamanca Mountains were visually identified using satellite imagery; those peatlands are small in size (&lt; 0.05 km<sup>2</sup>). Our analysis produced an estimated low-elevation peatland extent of 1433 km<sup>2</sup> and a high-elevation peatland extent of 23.08 km<sup>2</sup>, yielding an estimated total extent of 1456 km<sup>2</sup> for Costa Rica. This figure is in line with previously published extent estimates for this country (577-2670 km<sup>2</sup>).&nbsp;As for all maps, we stress that the accuracy of this product is ultimately limited by data availability and quality, as well as ground-referencing information. Still, the new map can provide guidance for land management, policymaking, and future science endeavors.</p>

restrictedcc-by-4.0Nov 2024View details →
zenodo36/100

Data and Software for "Probabilistic Trade-offs Analysis for Sustainable and Equitable Management of Climate-Induced Water Risks"

<p><span>Research data supporting the study "Probabilistic trade-offs analysis for sustainable and equitable management of climate-induced water risks"</span></p> <p><span>This repository provides data of the Stochastic Dual Dynamic Programming (SDDP) model, and the output results of the simulations of the various policies and climate scenarios considered in this study, as well as the code used for postprocessing and visualizing the results.</span></p> <p><strong><span>Contents</span></strong></p> <ol> <li><strong><span>Data: Model Inputs</span></strong><span><br>This folder contains the physical river network, reservoir and water demand, and economic data derived from the observed database.<br>The key files are:</span></li> <ul> <li><span>Input_HydrologicalData</span></li> <li><span>Input_SystemData</span></li> </ul> <li><strong><span>Results: Model Output Analysis</span></strong><span><br>This folder includes outputs from the Stochastic Dual Dynamic Programming (SDDP) model under various policies and climate scenarios. The results showcase optimized sectoral water use, including irrigated areas, hydropower generation, and allocations for agriculture, energy, and urban demands across spatial locations (upstream and downstream).<br>Key files include:</span></li> <ul> <li><strong><span>SDDP Model Outputs</span></strong><span> (MATLAB format): </span></li> <ul> <li><span>EnergyPriority_Baseline.mat</span></li> <li><span>EnergyPriority_2070.mat</span></li> <li><span>EnergyPriority_2100.mat</span></li> <li><span>AgriculturePriority_Baseline.mat</span></li> <li><span>AgriculturePriority_2070.mat</span></li> <li><span>AgriculturePriority_2100.mat</span></li> </ul> <li><strong><span>Extracted Model Results</span></strong><span> (Excel format): </span></li> <ul> <li><span>Organized for each policy and climate scenario to facilitate analysis.</span></li> </ul> </ul> <li><strong><span>Software: Data Analysis and Visualization</span></strong><span><br>Python scripts designed for outputs data analysis and visualization are included to reproduce the primary figures from the study.<br>Scripts provided:</span></li> <ul> <li><span>CDF_outflow.py</span><span>: Analyzes cumulative distribution functions for river discharge.</span></li> <li><span>CDF_sectors.py</span><span>: Examines sectoral water use distributions.</span></li> <li><span>PCP_SI.py</span><span>: Generates Parallel Coordinate Plots for trade-offs analysis.</span></li> </ul> <li><strong><span>Instructions: README File</span></strong><span><br>A comprehensive README file explains:</span></li> <ul> <li><span>Details of model input data.</span></li> <li><span>Instructions to interpret the SDDP model outputs.</span></li> </ul> </ol> <p><strong><span>Instructions:</span></strong><span><br></span><span>The Python scripts process Excel files from the model output results folder to generate and visualize the figures for the paper. Each step is clearly documented within the scripts.</span></p>

opencc-by-4.0Nov 2024View details →
dryad36/100

Probabilistic inference of the genetic architecture of functional enrichment of complex traits

<p>We develop a Bayesian model (BayesRR-RC) that provides robust SNP-heritability estimation, an alternative to marker discovery, and accurate genomic prediction, taking 22 seconds per iteration to estimate 8.4 million SNP-effects and 78 SNP-heritability parameters in the UK Biobank. We find that only $\leq$ 10\% of the genetic variation captured for height, body mass index, cardiovascular disease, and type 2 diabetes is attributable to proximal regulatory regions within 10kb upstream of genes, while 12-25% is attributed to coding regions, 32-44% to introns, and 22-28% to distal 10-500kb upstream regions. Up to 24% of all cis and coding regions of each chromosome are associated with each trait, with over 3,100 independent exonic and intronic regions and over 5,400 independent regulatory regions having &gt;95% probability of contributing &gt;0.001% to the genetic variance of these four traits. Our open-source software (GMRM) provides a scalable alternative to current approaches for biobank data.</p>

opencc-zeroNov 2021View details →
zenodo36/100

Dance Your Ph.D. 2018 Physics FINALIST: Dark energy and dark matter via probabilistic data analysis

<p>Dark matter (dancer in black mask; brings dancers together) and dark energy (dancer in black mask; pulls dancers apart) are the mysterious constituents of the universe that determine the evolution of the largest structures, clusters of galaxies (dancers in tie dye), and I (dancer in gold mask) want to learn about them them by analyzing a huge set of 3D galaxy positions. The telescope (dancer in silver mask) gives me 2D images of galaxies with no distances, so I have to estimate galaxy locations with &quot;redshift,&quot; which is correlated with distance. The exciting telescopes of the next decades will build large samples of galaxies by taking lots of superficial color data that&#39;s not informative enough to determine the redshift. One thing that tells us about dark matter and dark energy is the redshift distribution (dancer in red stripes) -- I can still learn about dark energy and dark matter if I can figure out how many galaxies have each redshift. Since I don&#39;t actually know the redshifts of any galaxies, I consider the probability of redshift (dancers in white shirts) for each galaxy based on its limited color data. However, the redshift probabilities are biased by prior beliefs (dancer in gray scarf) about physics that are transmitted by the way we derive the probabilities from the galaxy colors. If unaccounted for, the prior beliefs could cause us to draw the wrong conclusions about dark matter and dark energy, meaning we won&#39;t learn anything from all this amazing telescope data we&#39;re going to have. For my thesis, I developed a method that puts the prior beliefs in their proper place and lets the data guide the inference of the redshift distribution, using an approach called Bayesian statistics. I audition many possible redshift distributions and check how likely each is to have caused the observed galaxy colors, with the redshift probabilities as the judges; this procedure is called Markov chain Monte Carlo (MCMC) sampling, and it leads to an ensemble of possible redshift distributions each with an associated probability of having produced the observed galaxy colors. By doing the math carefully and correctly, we will learn more about dark matter and dark energy even with the coarsest data!</p>

opencc-by-4.0Jan 2019View details →
zenodo36/100

Objective identification of high-wind features within extratropical cyclones using a probabilistic random forest (RAMEFI). Part I: Method and illustrative case studies - Video Supplement

<p>These videos provide examples of application of RAMEFI (RAndom-forest based MEsoscale wind Feature Identification), a new objective identification of high-wind features within extratropical cyclones, for twelve selected case studies.</p>

opencc-by-4.0May 2022View details →
zenodo36/100

Interpretable Deep Learning for Probabilistic MJO Prediction: CNN Forecasts

<p>This repository contains data produced for the paper &quot;Interpretable Deep Learning for Probabilistic MJO Prediction&quot; by A. Delaunay and H. M. Christensen (2021).</p> <p>&gt;&gt; mu_ens_XX.pt<br> contains the mean forecasts from each ensemble member at a lead time of XX&nbsp;days</p> <p>&gt;&gt; cov_alea_XX.pt<br> contains the aleatoric predictions of each ensemble member at a lead time of XX&nbsp;days</p>

opengpl-2.0-or-laterJul 2022View details →
zenodo36/100

Probabilistic modeling of the indoor climates of residential buildings using EnergyPlus - data set of indoor temperature and relative humidity

<p>This data supplements the journal article:&nbsp;</p> <p>Buechler E, Pallin S, Boudreaux P, Stockdale M. Probabilistic modeling of the indoor climates of residential buildings using EnergyPlus.&nbsp;<em>Journal of Building Physics</em>. 2017;41(3):225-246. doi:<a href="https://doi.org/10.1177/1744259117701893">10.1177/1744259117701893</a></p> <p>Abstract:</p> <p>The indoor air temperature and relative humidity in residential buildings significantly affect material moisture durability, heating, ventilation, and air-conditioning system performance, and occupant comfort. Therefore, indoor climate data are generally required to define boundary conditions in numerical models that evaluate envelope durability and equipment performance. However, indoor climate data obtained from field studies are influenced by weather, occupant behavior, and internal loads and are generally unrepresentative of the residential building stock. Likewise, whole-building simulation models typically neglect stochastic variables and yield deterministic results that are applicable to only a single home in a specific climate. The purpose of this study was to probabilistically model homes with the simulation engine EnergyPlus to generate indoor climate data that are widely applicable to residential buildings. Monte Carlo methods were used to perform 840,000 simulations on the Oak Ridge National Laboratory supercomputer (Titan) that accounted for stochastic variation in internal loads, air tightness, home size, and thermostat set points. The Effective Moisture Penetration Depth model was used to consider the effects of moisture buffering. The effects of location and building type on indoor climate were analyzed by evaluating six building types and 14 locations across the United States. The average monthly net indoor moisture supply values were calculated for each climate zone, and the distributions of indoor air temperature and relative humidity conditions were compared with ASHRAE 160 and EN 15026 design conditions. The indoor climate data will be incorporated into an online database tool to aid the building community in designing effective heating, ventilation, and air-conditioning systems and moisture durable building envelopes.</p> <p>This supplemental data set includes the hourly temperature and relative humidity for the 10th,&nbsp;50th, and 90th percentile simulations for each building type in each climate zone. The column headings are of the following format buildingtype_climatezone_output_percentile.</p> <p>There are six building types, B1 (unfinished basement 1-story), B2 (unfinished basement 2-story), C1 (unvented crawlspace 1-story), C2 (unvented crawlspace 2-story), S1 (slab 1-story), and S2 (slab 2-story).</p>

opencc-by-4.0Jul 2022View details →
zenodo36/100

Data from 'How Did Trilobites Conquer the Oceans? A Probabilistic Palaeobiogeographical Analysis of Cambrian Trilobites'

Open the record for dataset details and reuse information.

opencc-by-4.0Apr 2024View details →
zenodo36/100

Probabilistic Fault Displacement Hazard Assessment materials

<p>The models, data, and information provided here were created as part of the Fault Displacement Hazard Initiative. We provide the Electronic Supplement for Chiou et al., 2023, CDF Fortran subroutines; the ArcGIS least-cost path (LCP) model and implementation guide, LCP MATLAB and Python scripts, and the LCP for 75 events in a shapefile and KMZ format for Thomas et al., 2023; and the Fortran code for Chiou et al. in review for Earthquake Spectra.&nbsp;&nbsp;</p>

opencc-by-4.0Aug 2023View details →
zenodo36/100

Code and Data for "Probabilistic Eddy Identification with Uncertainty Quantification"

<p>The code and data used in the paper "Probabilistic Eddy Identification with Uncertainty Quantification".</p>

opencc-by-4.0May 2024View details →
zenodo36/100

Data products associated with "Probabilistic Forward Modeling of Galaxy Catalogs with Normalizing Flows"

<p>These are the data products associated with "Probabilistic Forward Modeling of Galaxy Catalogs with Normalizing Flows" by J. F. Crenshaw, et. al. This includes the input catalog and the outputs of the workflow described here https://github.com/jfcrenshaw/pzflow-paper, as well as a gzip of the github repo.</p>

opencc-by-4.0May 2024View details →
zenodo36/100

Model data for probabilistic projections of the Amery Ice Shelf catchment, Antarctica, under high ice-shelf basal melt conditions

<p>Model data for probabilistic projections of the Amery Ice Shelf catchment,&nbsp;<br>Antarctica, under high ice-shelf basal melt conditions<br>======================================================================</p> <p>This archive contains ice-sheet model output and statistical models&nbsp;<br>used in the manuscript:<br>"Probabilistic projections of the Amery Ice Shelf catchment, Antarctica, under<br>high ice-shelf basal melt conditions" by:<br>Sanket Jantre, Matthew Hoffman, Nathan M. Urban, Trevor Hillebrand, Mauro<br>Perego, Stephen Price, John D. Jakeman</p> <p>OVERVIEW<br>--------</p> <p>Statistical models and corresponding datasets are archived in the file<br>Amery_UQ_Study_Statistical_Models.zip. &nbsp;That file contains a README that<br>describes its contents.<br>Contact for statistical models:<br>Sanket Jantre, Brookhaven National Laboratory, sjantre@bnl.gov</p> <p>The remaining files in this archive contain output from ice-sheet model&nbsp;<br>simulations using the MPAS-Albany Land Ice (MALI) model&nbsp;<br>(Hoffman et al. 2018, https://github.com/MALI-Dev/E3SM)<br>applied to a regional domain of the Amery Ice Shelf catchment<br>of Antarctica with mesh resolution varying from 4 to 20 km.<br>The contents of these files are described below.<br>Contact for MALI simulations:<br>Matthew Hoffman, Los Alamos National Laboratory, mhoffman@lanl.gov</p> <p>ENSEMBLES<br>---------</p> <p>The ensembles consist of all or a subset of 200 model runs with values for 6<br>parameters sampled from a Sobol' sequence over a specified range.</p> <p>Parameters and Sampled Ranges:<br>1. Ice stiffness scaling factor, C&phi;: (0.8, 1.2)<br>2. Basal friction scaling factor, C&mu;: (0.8, 1.2)<br>3. Basal slip exponent, q: (0.1, 0.333)<br>4. Calving yield stress, &sigma;max: (80, 180) kPa<br>5. Ice-shelf melt coefficient, &gamma;0: (9620, 471000) m yr&minus;1<br>6. Ice-shelf basal melt rate, m: (12, 58) Gt yr&minus;1</p> <p>SCENARIOS<br>---------</p> <p>The archive contains output from 4 scenarios described in the manuscript:</p> <p>Historical relaxation (RELX): For each ensemble member, we conducted a 50 year<br>relaxation from the initial condition using historical climate forcing to<br>integrate out fast transient behavior. For surface mass balance, we applied a<br>1995&ndash;2017 climatological average from RACMO2.3p1 (Van Wessem et al., 2014; van<br>den Broeke, 2019). The ocean thermal forcing was the observation-based<br>climatology compiled for ISMIP6-Antarctica, which uses data from 1995&ndash;2018<br>(Jourdain et al., 2020; Nowicki et al., 2020). The 50 year relaxation duration<br>was chosen as the most rapid adjustments occur in the first few decades of<br>integration, while the long term adjustment to a fully steady state takes<br>thousands of years. Relaxation to full steady state would require<br>substantially more computing resources than our entire set of ensembles and<br>also leads to the complication of different runs having potentially very<br>different initial states. Future improvements to model initialization that<br>account for surface elevation change (Perego et al., 2014) may reduce model<br>drift and adjust this requirement. The final model state in each run at the<br>end of RELX was given the nominal date of January 1, 2015, and all three<br>projection ensembles were branched from these states.</p> <p>Control projection (CTRL): The CTRL projection ensemble were an extension of<br>the RELX configurations, continuing the same surface mass balance and ocean<br>thermal forcing from January 1, 2015, to January 1, 2300. This ensemble was<br>used to assess model drift relative to the forced response of the climate<br>scenarios.&nbsp;</p> <p>SSP1-2.6 projection (SSP1): Our SSP1 projection used annual surface mass<br>balance and ocean thermal forcing derived from a UKESM SSP1-2.6 climate<br>scenario (expAE10 from Seroussi et al., 2024). Surface mass balance and ocean<br>thermal forcing were applied as anomalies relative to the climatological mean<br>forcings in RELX/CTRL to avoid issues related to climate model bias and abrupt<br>changes in forcing. This ensemble was also run from January 1, 2015, to<br>January 1, 2300.</p> <p>SSP5-8.5 projection (SSP5) Our SSP5 projection used the UKESM SSP5-8.5<br>projection forcings (expAE05 from Seroussi et al., 2024), again applied as<br>anomalies and from 2015 to 2300.</p> <p><br>OUTPUT<br>------</p> <p>Each ensemble directory contains at the base level:<br>* branch_ensemble.cfg - configuration file for the ensemble_generator test<br>&nbsp; case (https://mpas-dev.github.io/compass/latest/users_guide/landice/test_groups/ensemble_generator.html)&nbsp;<br>&nbsp; of COMPASS (Configuration Of Model for Prediction Across Scales Setups, https://github.com/MPAS-Dev/compass)<br>&nbsp; used to set up the ensemble.<br>* mesh_vars.nc - netCDF file containing the mesh variables. &nbsp;This file is the<br>&nbsp; same for all ensembles. &nbsp;These fields need to be appended to an output file to<br>&nbsp; visualize in, e.g., Paraview. &nbsp;This can be done with the command:<br>&nbsp; ncks -A mesh_vars.nc output.nc</p> <p>Each ensemble contains subdirectories for each run numbered 000-199. &nbsp;Each run<br>directory contains the files:<br>* globalStats.nc - scalar metrics at every time step<br>* output.nc - spatial fields at 10 year intervals<br>* run_info.cfg - summary of parameter values</p> <p>Notes:<br>* The SSP1 and SSP5 ensembles contain a subset of the full 200 runs<br>&nbsp; because some runs were filtered out as being unnecessary during model<br>&nbsp; calibration (see manuscript).<br>* The RELX ensemble is run for 50 years with an arbitrary start year of 2000.<br>&nbsp; The CTRL, SSP1, and SSP5 ensembles are started in 2015 from the final state<br>&nbsp; of the corresponding RELX run (nominally 2050). &nbsp;Because spatial data has<br>&nbsp; been saved in this archive at 10 year intervals, the first output for the<br>&nbsp; three projection ensembles is 2020. &nbsp;To get the initial condition for the<br>&nbsp; projection ensembles, use the 2050 state from RELX for the corresponding<br>&nbsp; model run.<br>* Spatial field output at 1 year intervals, as well as run input, log, and<br>&nbsp; restart files are available from the corresponding contact. &nbsp;The complete<br>&nbsp; run data is about 2 TB.</p> <p><br>CITATION<br>--------<br>If you find these data useful, please cite the DOI for this&nbsp;<br>archive (10.5281/zenodo.11166628), as well as our manuscript<br>submitted to The Cryosphere.</p> <p>This archive is approved by Los Alamos National Laboratory<br>for public release under LA-UR-24-24969; distribution is unlimited.</p> <p>&nbsp;</p> <p>REFERENCES<br>----------</p> <p>Hoffman, M. J., Perego, M., Price, S. F., Lipscomb, W. H., Zhang, T.,<br>Jacobsen, D., Tezaur, I., Salinger, A. G., Tuminaro, R., and Bertagna, L.:<br>MPAS-Albany Land Ice (MALI): a variable-resolution ice sheet model for Earth<br>system modeling using Voronoi grids, Geoscientific Model Development, 11,<br>3747&ndash;3780, 2018.</p> <p>Jourdain, N. C., Asay-Davis, X., Hattermann, T., Straneo, F., Seroussi, H.,<br>Little, C. M., and Nowicki, S.: A protocol for calculating basal melt rates in<br>the ISMIP6 Antarctic ice sheet projections, The Cryosphere, 14, 3111&ndash;3134,<br>https://doi.org/10.5194/tc-14-3111-2020, 2020.</p> <p>Nowicki, S., Goelzer, H., Seroussi, H., Payne, A. J., Lipscomb, W. H.,<br>Abe-Ouchi, A., Agosta, C., Alexander, P., Asay-Davis, X. S., Barthel, A.,<br>Bracegirdle, T. J., Cullather, R., Felikson, D., Fettweis, X., Gregory, J. M.,<br>Hattermann, T., Jourdain, N. C., Kuipers Munneke, P., Larour, E., Little, C.<br>M., Morlighem, M., Nias, I., Shepherd, A., Simon, E., Slater, D., Smith, R.<br>S., Straneo, F., Trusel, L. D., van den Broeke, M. R., and van de Wal, R.:<br>Experimental protocol for sea level projections from ISMIP6 stand-alone ice<br>sheet models, The Cryosphere, 14, 2331&ndash;2368,<br>https://doi.org/10.5194/tc-14-2331-2020, 2020.</p> <p>Perego, M., Price, S., and Stadler, G.: Optimal Initial Conditions for<br>Coupling Ice Sheet Models to Earth System Models, Journal of Geophysical<br>Research: Earth Surface, 119, 1894&ndash;1917, https://doi.org/10.1002/2014JF003181,<br>2014.</p> <p>Seroussi, H., et al. 2024. ISMIP6 Projections 2300 Antarctica Protocol.<br>https://theghub.org/groups/ismip6/wiki/ISMIP6-Projections2300-Antarctica.&nbsp;</p> <p>van den Broeke, M.: RACMO2.3p1 annual surface mass balance Antarctica<br>(1979-2014), PANGAEA - Data Publisher for Earth &amp; Environmental Science,<br>https://doi.org/10.1594/PANGAEA.896940, 2019.</p> <p>van Wessem, J., Reijmer, C., Morlighem, M., Mouginot, J., Rignot, E., Medley,<br>B., Joughin, I., Wouters, B., Depoorter, M., Bamber, J., Lenaerts, J., Van De<br>Berg, W., Van Den Broeke, M., and Van Meijgaard, E.: Improved Representation<br>of East Antarctic Surface Mass Balance in a Regional Atmospheric Climate<br>Model, Journal of Glaciology, 60, 761&ndash;770,<br>https://doi.org/10.3189/2014JoG14J051, 2014.</p>

opencc-by-4.0May 2024View details →
zenodo36/100

Dataset for MRes Thesis: Probabilistic Operator Learning for Climate Model Parameterisation

<p>This dataset was collated for use in experiments presented in the MRes Thesis "Probabilistic Operator Learning for Climate Model Parameterisation" submitted to the University of Cambridge.<br><br>All data included was generated by other researchers, this is simply a subset to allow easy reproduction of the experiments contained in the work above.</p> <p>The data for the Burgers' equation (<a href="../api/records/12529654/draft/files/burgers_data_R10.mat/content" target="_blank" rel="noopener noreferrer">burgers_data_R10.mat</a>) and the Darcy Flow (<a href="../api/records/12529654/draft/files/piececonst_r421_N1024_smooth1.mat/content" target="_blank" rel="noopener noreferrer">piececonst_r421_N1024_smooth1.mat</a>, <a href="../api/records/12529654/draft/files/piececonst_r421_N1024_smooth2.mat/content" target="_blank" rel="noopener noreferrer">piececonst_r421_N1024_smooth2.mat</a>) experiments were generated by Lu et al. (2022). Creative Commons Attribution Non Commercial Share Alike 4.0 International applies.</p> <p>The data for the Helmholtz (<a href="../api/records/12529654/draft/files/Helmholtz_inputs.npy/content" target="_blank" rel="noopener noreferrer">Helmholtz_inputs.npy</a>, <a href="../api/records/12529654/draft/files/Helmholtz_outputs.npy/content" target="_blank" rel="noopener noreferrer">Helmholtz_outputs.npy</a>) and Navier-Stokes (<a href="../api/records/12529654/draft/files/NavierStokes_inputs.npy/content" target="_blank" rel="noopener noreferrer">NavierStokes_inputs.npy</a>, <a href="../api/records/12529654/draft/files/NavierStokes_outputs.npy/content" target="_blank" rel="noopener noreferrer">NavierStokes_outputs.npy</a>) experiments were generated by de Hoop et al. (2022). Creative Commons Attribution 4.0 International applies.</p> <p>References:</p> <div> <div> <div>1.&nbsp;Lu L, Meng X, Cai S, Mao Z, Goswami S, Zhang Z, et al. A comprehensive and fair comparison of two neural operators (with practical extensions) based on FAIR data. Computer Methods in Applied Mechanics and Engineering. 2022 Apr 1;393:114778.</div> <div>&nbsp;</div> <div> <div> <div> <div>2.&nbsp;de Hoop MV, Huang DZ, Null EQ, Stuart AM. The Cost-Accuracy Trade-Off in Operator Learning with Neural Networks. JML. 2022 Jun;1(3):299&ndash;341.</div> </div> </div> </div> </div> </div> <p>&nbsp;</p>

opencc-by-4.0Jun 2024View details →
zenodo36/100

Probabilistic Shaping over Multi-Subcarrier Modulation - LAB Data

<p>Experimental data of long-haul transmission with probabilistic shaping 36QAM and multi-subcarrier 16QAM. Data sets include optical back-to-back (OB2B) and recirculating loop (LOOP) measurements for 1, 4 and 8 subcarriers.</p>

opencc-by-4.0Mar 2018View details →
zenodo36/100

Integrated Probabilistic Annotation (IPA): A Bayesian-based annotation method for metabolomic profiles integrating biochemical connections, isotope patterns and adduct relationships - Supplementary Data

<ol> <li>Supplementary_data_1: data and code for standards analysis and database update</li> <li>Supplementary_data_2.zip: data and code used for the generation of the synthetic experiment</li> <li>Supplementary_data_3.zip: data, code, and results of the <em>E. coli</em> dataset analysis</li> <li>Supplementary_data_4.zip: data, code, and results of the beer dataset analysis</li> <li>Supplementary_data_5.zip: data, code, and results of the comparison with xMSannotator</li> </ol>

opencc-by-4.0Sep 2019View details →
zenodo36/100

Probabilistic reanalysis of storm surge extremes in Europe

<p>This dataset contains the probabilistic reanalysis of storm surge extremes presented in the paper:</p> <p>Calafat, F. M., and M. Marcos (2020), Probabilistic reanalysis of storm surge extremes in Europe. Proc. Natl. Acad. Sci. U. S. A.</p> <p>Please cite that paper when using this&nbsp;dataset.</p> <p>This dataset includes estimates of the GEV parameters (location, scale and shape) and surge annual maxima at both gauged and ungauged locations.</p>

opencc-by-4.0Oct 2019View details →
zenodo36/100

Probabilistic Data Generating Process-based Crop Type Map for the EU 2010-2020

<h3>General Description</h3> <p>This dataset consists of probabilistic crop type maps for the EU-28 for the years 2010-2020 that distinguish 28 crop types at 1km resolution (EPSG:3035). The maps were generated using the Data Generating Process-based procedure developed by Baumert, Heckelei and Storm (2024) [<em><span><a href="https://doi.org/10.1016/j.ecoinf.2024.102836">https://doi.org/10.1016/j.ecoinf.2024.102836</a></span></em>]. We refer to this paper for details on the generation and validation of the maps. The code used to create the maps including a detailed list of the input data can be found here: <a href="https://github.com/JoBaumert/Probabilistic_Crop_Mapping_EU">GitHub - JoBaumert/Probabilistic_Crop_Mapping_EU</a> .&nbsp;</p> <h3>Downloadable Data</h3> <p>The file &ldquo;EU_expected_crop_shares.zip&rdquo; consists of 11 raster files, one for each year from 2010 &ndash; 2020. The raster files indicate the expected shares for each of the 28 distinguished crop types in a grid cell for the entire EU-28 (see readme.txt contained in the zipped folder). Note that this raster file does not contain uncertainty information.</p> <p>The other 28 zip files contain the entire crop map ensemble (i.e., including uncertainty information), each for one of the EU countries and the United Kingdom. Each of those zip files contain 11 raster files, one for each year from 2010 &ndash; 2020. Each raster file has 2830 bands: the first two bands indicate the weight of the cell (proportional to the utilized agricultural area in a cell) and the estimated number of agricultural fields in a cell, respectively. The next 28 bands indicate the expected shares for each of the 28 crops in the respective cell. The remaining 2800 bands compose the crop type map ensemble, i.e., 100 simulated crop shares for each of the 28 crops. The zipped country folder also includes a csv file named &ldquo;bands&rdquo; that describes which band refers to which crop. Note that all crop shares were multiplied by 1000 when writing them to the raster files (saving them as integers requires less storage capacity), i.e., if a crop share is 0.325 or 32.5% it will appear as 325 in the raster files.&nbsp;</p> <p>The distinguished crops are (with abbreviation used in "bands.csv"):</p> <ul> <li>Apples and other fruits, nuts and berries (APPL+OFRU)</li> <li>Barley (BARL)</li> <li>Citrus fruits (CITR)</li> <li>Durum wheat (DWHE)</li> <li>Flowers and ornamental plants (FLOW)</li> <li>Grassland (GRAS)</li> <li>Maize (both green maize as well as grain maize, LMAIZ)</li> <li>Rape and turnip (LRAPE)</li> <li>Nurseries (NURS)</li> <li>Oats (OATS)</li> <li>Other cereals (OCER)</li> <li>Other permanent crops (OCRO)</li> <li>Other forage plants (OFAR)</li> <li>Other industrial plants (OIND)</li> <li>Olives (OLIVGR)</li> <li>Rice (PARI)</li> <li>Potatoes (POTA)</li> <li>Pulses (PULS)</li> <li>Fodder roots and brassicas (ROOF)</li> <li>Rye (RYEM)</li> <li>Soybeans (SOYA)</li> <li>Sugar beets (SUGB)</li> <li>Sunflowers (SUNF)</li> <li>Soft/common wheat (SWHE)</li> <li>Other oilseeds and fibre crops (TEXT)</li> <li>Tobacco (TOBA)</li> <li>Fresh vegetables, melons, strawberries (TOMA+OVEG)</li> <li>Vineyards (VINY)</li> </ul> <p>&nbsp;</p> <p>&nbsp;</p>

opencc-by-4.0Sep 2024View details →
zenodo36/100

Time-Dependent Probabilistic Tsunami Inundation Assessment Using Mode Decomposition to Assess Uncertainty for an Earthquake Scenario

<p>This is the dataset of the manuscript submitted to JGR&nbsp;Ocean (Feb 2021).</p>

opencc-by-4.0May 2021View details →
zenodo36/100

Data and GrADS scripts needed to reproduce the figures in the article "Probabilistic forecasts of near-term climate change: verification for temperature and precipitation changes from years 1971-2000 to 2011-2020"

<p>Data and GrADS scripts needed to reproduce the figures in the article &quot;Probabilistic forecasts of near-term climate change: verification for temperature and precipitation changes from years 1971-2000 to 2011-2020&quot;, submitted for publication in Climate Dynamics.</p> <p>Please see the file README for further details.</p> <p>&nbsp;</p>

opencc-ncJul 2021View details →

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