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405 results for “FLARES”
Active region magnetograms for solar flare prediction: Full resolution dataset
<p>In this dataset, we provide a comprehensive collection of magnetograms from the National Aeronautics and Space Administration's (NASA's) Solar Dynamics Observatory (SDO). The dataset incorporates data from three sources and provides SDO Helioseismic and Magnetic Imager (HMI) magnetograms of solar active regions as well as labels of corresponding flaring activity. This dataset will be useful for image analysis or solar physics research related to magnetic structure, its evolution over time, and its relation to solar flares. The dataset will be of interest to those researchers investigating automated solar flare prediction methods, including supervised and unsupervised machine learning (classical and deep), binary and multi-class classification, and regression. This dataset is a minimally processed, user configurable dataset of consistently sized images of solar active regions that can serve as a benchmark dataset for solar flare prediction research. This dataset consists of full resolution images (see usage notes below).</p>
Flaring Latitudes in Ensembles of Low Mass Stars
<p>Simulated data, and aggregated results necessary to recreate the results and figures in the forthcoming paper, Ilin et al. 2023: "Flaring Latitudes in Ensembles of Low Mass Stars" (link TBD). The double timestamped files are simulated mean and standard deviation values for ensembles of randomly oriented stars, split into the training and the validation data sets. Their configurations are listed in the _all_runs file. You can find the aggregated mean and standard deviation values in _all_means_std. The flare parameter fits from Fig. 1 are under _a_from_ed and fwhm_from_ed_a. The fit parameters from Table 2 in the paper are in fit_paratemers. The results for the Okamoto et al. (2021) G dwarf flares are in okamoto2021_table.</p>
Towards alternative solutions for flaring : life cycle assessment and carbon substance flow analysis of associated gas conversion into C3 chemicals
<p>Supplementary material and used data for the publication.</p>
Quantification of the global and regional impacts of gas flaring on human health via spatial differentiation
<p>Supplementary material for the associated publication.</p>
The corona of a fully convective star with a near-polar flare
<p>Raw XMM-Newton EPIC data, data reduction scripts for XMM-SAS, and reduced images and spectra extracted with XSPEC. The observations include the X-ray emission of TIC 277539431, a rapidly rotating M7 dwarf star that produced a polar flare in 2021, observed by the Transiting Exoplanet Survey Satellite (see <a href="https://ui.adsabs.harvard.edu/abs/2021MNRAS.507.1723I">Ilin et al. 2021</a>).<br> <br> Publications based on this data set will be linked as they appear.</p>
Dipyridamole Assessment for Flare Reduction in Systemic Lupus Erythematosus (SLE)
ClinicalTrials.gov study NCT01781611. IPD Sharing: YES. Countries: 1. Publications: 2.
Active region magnetograms for solar flare prediction: Full resolution dataset
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Active region magnetograms for solar flare prediction: Reduced resolution dataset
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Active region magnetograms for solar flare prediction: Extra images dataset
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Domus, Moleta dels Flares (Lésera), Forcall, Castellón, Comunitat Valenciana, España, Europa │Proyecto de digitalización 3D, 2D
<p>Proyecto de digitalización <strong>2D</strong> y <strong>3D</strong> de la domus de Lésera, (Moleta del Flares, yacimiento arqueológico) realizado por <strong>AD&D 4D, </strong>proyecto de <strong>recreación virtual</strong> de la domus de Lesera, (Moleta dels Frares, yacimiento arqueológico) realizado por Balam Consultores SL con patrocinio de <strong>Generalitat Valenciana </strong>y el <strong>Ayuntamiento de Forcall.</strong></p> <ul> <li>Fotografía panorámica 360º 27.130 x 3564 puntos 16 bits Tiff <strong>Ref: </strong><a href="https://zenodo.org/record/4075918/files/20200110MoletaDelsFlares-DomusPano360.tif?download=1">20200110MoletaDelsFlares-DomusPano360.tif</a></li> <li>Video 4K (3840x2160 puntos) 10 bits mov <strong>Ref</strong>: <a href="https://zenodo.org/api/files/27fbfa78-979c-4cf2-b362-06daea9d5b45/20200930L%C3%A9sera%20Video4K.7z">20200930Lésera Video4K.7z</a></li> <li>Fichas interactivas pdf (Español, English, Valenciano) <strong>Ref</strong>: <a href="https://zenodo.org/api/files/27fbfa78-979c-4cf2-b362-06daea9d5b45/FichasInteractivas-MoletaDelFlares-Lesesra-Domus2020.7z">FichasInteractivas-MoletaDelFlares-Lesesra-Domus20 ..</a></li> <li>Nube de puntos georreferenciada 24 M <strong>Ref</strong>: <a href="https://zenodo.org/api/files/27fbfa78-979c-4cf2-b362-06daea9d5b45/20200110MoletaDelsFlares-Domus24M.7z">20200110MoletaDelsFlares-Domus24M.7z</a></li> <li>Modelo digital de elevaciones 2 mm. pixel <strong> Ref</strong>: <a href="https://zenodo.org/api/files/27fbfa78-979c-4cf2-b362-06daea9d5b45/20201001MoletaDomusDEM2mm.7z">20201001MoletaDomusDEM2mm.7z</a></li> <li>Ortofotomapa 2 mm pixel <strong>Ref</strong>.: <a href="https://zenodo.org/api/files/27fbfa78-979c-4cf2-b362-06daea9d5b45/20201001MoletaDomusOrto2mm.7z">20201001MoletaDomusOrto2mm.7z </a></li> <li>Modelo 3D georreferenciado 48 Millones de polígonos <strong>Ref</strong>: <a href="https://zenodo.org/api/files/27fbfa78-979c-4cf2-b362-06daea9d5b45/20200110MoletaDelsFlares-Domus48MGeo.7z">20200110MoletaDelsFlares-Domus48MGeo.7z</a></li> <li>Impresión 3D domus y recreación stl: <a href="https://zenodo.org/api/files/27fbfa78-979c-4cf2-b362-06daea9d5b45/20201105_Impresi%C3%B3n_Domus.7z">20201105_Impresión_Domus.7z</a></li> <li>Aplicación interactiva de realidad virtual mediante Unreal Engine 4 (optimizada para Oculus Rift S, funciona en cualquier plataforma Steam VR. Requisitos mínimos: i5 4550 o equivalente, GeForce GTX 1060 o equivalente, 8GB RAM). Domus recreada en 3D a partir de la hipótesis de su tercera fase (s. I d.C.) con mobiliario y decoración propia de la época y zona. 1,7 millones de polígonos, texturas 1K a 4K <strong>Ref</strong>: <a href="https://zenodo.org/api/files/27fbfa78-979c-4cf2-b362-06daea9d5b45/RecreacionDomusLeseraVR.rar">RecreacionDomusLeseraVR.rar </a></li> </ul> <p> </p> <p><strong>Online:</strong></p> <p><a href="https://sketchfab.com/3d-models/domus-moleta-dels-flares-forcall-castellon-439ca323bc9a43bca6f3775c6e043f67">Visor de Modelo 3D</a> │Sketchfab</p> <p><a href="https://skfb.ly/6WGEF">Visor de Modelo 3D Recreación</a> │Sketchfab</p> <p><a href="https://www.pointbox.xyz/clouds/5f8b368f9cad5d7421eeae37">Nube de Puntos Densa</a> │ Point Box</p> <p><a href="https://www.youtube.com/watch?v=yIOjo3ua7to">Video 4K</a> │ YouTube</p> <p> </p> <p>Sistema de referencia geodésico: <strong>ETRS 89 UTM 30 (EPSG 25830)</strong><br> Altitudes Ortométricas referidas al nivel medio del mar de Alicante.</p> <p>Modelo de Geóide <strong>EGM08</strong> con sobrecorreción de nivelación.</p>
The First Fermi-LAT Solar Flare Catalog Appendix
<p>We present the appendix of the First Fermi-Large Area Telescope (LAT) Solar flare catalog covering the 24thSolar cycle. The catalog (published in ApJS) contains 45 Fermi-LAT Solar flares (FLSFs) with emission in theγ-ray energy band (30 MeV -10 GeV) detected with a significance ≥5σ over the years 2010-2018. A subsample containing 37 of these flares exhibit delayed emission beyond the prompt-impulsive hard X-ray phase with 21 flares showing delayed emission lasting more than two hours. No prompt-impulsive emission is detected in four of these flares. We also report the first time observations of GeV emission from 3 flares originating from Active Regions located behind the limb (BTL) of the visible Solar disk. We report the light curves, spectra, best proton index and localization (when possible) for all the FLSFs and correlations with Solar multi-wavelength phenomena. The gamma-ray spectra is consistent with the decay of pions produced by >300 MeV protons. The work presented in the First Fermi Solar Flare Catalog contains the largest sample of high-energy gamma-ray flares ever reported and provides the unique opportunity to perform population/correlation studies on the different phases of the flare and thus allowing to open a new window in solar physics.</p> <p>This work is on behalf of the Fermi Large Area Telescope Collaboration. The First Fermi LAT Solar Flare Catalog has been accepted for publication on ApJS.</p>
Moleta dels Flares / Forcall / Castellón / Spain
+INFO: [Español](http://www.castellonarqueologico.es/yacimientos/els-ports/la-moleta-dels-frares/) / [Valencià](http://www.castellonarqueologico.es/va/yacimientos/els-ports/la-moleta-dels-frares/) / [English](http://www.castellonarqueologico.es/en/yacimientos/els-ports/la-moleta-dels-frares/)  Date capture: 2018-06-08 Source: Objaverse 1.0 / Sketchfab
Ionosphere-Thermosphere Data Published in "Responses of the Thermosphere and Ionosphere System to Concurrent Solar Flares and Geomagnetic Storms"
<p>This dataset supports the Journal of Geophysical Research publication "Responses of the Thermosphere and Ionosphere System to Concurrent Solar Flares and Geomagnetic Storms" by Qian et al., 2019. The data files are selected output and related analyses from the thermosphere-ionosphere-electrodynamics general circulation model (TIEGCM). The format of the data files are either IDL save files or NetCDF files or ASCII.</p>
A Possible Mechanism for "Late Phase" in Stellar White-Light Flares
<p>This is the simulation data used for the paper "A Possible Mechanism for 'Late Phase' in Stellar White-Light Flares" that was accepted for publication on ApJ.</p>
Supplementary material for "Stellar flares" (Living Reviews in Solar Physics)
<p>The file supplementary.tar.gz contains a Jupyter notebook (Figs.ipynb) and supplementary material for recreating Figures 13, 35, 38, and 40 in Kowalski, A.F. (2024), "Stellar flares", <em>Living Reviews in Solar Physics</em> 24, 1 (<a href="10.1007/s41116-024-00039-4">https://doi.org/10.1007/s41116-024-00039-4</a>).</p>
The data for Time-dependent Stellar Flare Models of Deep Atmospheric Heating
<p>This repository contains model output (within two .tar.gz files) and a pdf document (analysis_tools_mdwarfradyngrid-v1.0.pdf) that explains the contents and use. The models are described in Kowalski, A.F., Allred, J.C., & Carlsson, M. <em>Time-dependent Stellar Flare Models of Deep Atmospheric Heating, </em>published 2024 July 5 in <em>The Astrophysical Journal</em> Volume 969, Number 2 (DOI: <a href="https://iopscience.iop.org/article/10.3847/1538-4357/ad4148">10.3847/1538-4357/ad4148</a>).</p> <p>The Jupyter notebook demo, radyn_xtools_Demo.ipynb is included in the PyPI package installation that is described in analysis_tools_mdwarfradyngrid-1.0.pdf.</p>
Solar Flare List for Pre-Flare Emission Variability Study
<p>Flare file: dates, GOES flare class, cutout coordinates used, and eruptivity/131 spike flags for pre-flare emission study</p> <p>Quiet file: dates, NOAA AR designation for non-flaring control cases</p>
Data for AU Mic Flares Observed with HST/COS
<p>Data products and tables affiliated with "AU Microscopii in the FUV: Observations in Quiescence, During Flares, and Implications for AU Mic b and c" (Feinstein et al. 2022). This directory contains the following data products:</p> <ul> <li><strong>A demonstration Jupyter notebook on how to create the SED for AU Mic (</strong>panchromatic_spectrum_demo.ipynb<strong>) and all affiliated spectra and errors</strong> <ul> <li>X-ray -- XMM-Newton (xmm_newton_spectrum.npy)</li> <li>Differential Emission Measurement flux (au_mic_dem_quiescent_spectrum.fits)</li> <li>FUV -- FUSE (fuse_spectra.npy)</li> <li>FUV -- HST/COS (hst_cos_quiescent_spectrum.txt)</li> <li>NUV -- IUE (iue_spectra.npy)</li> <li>Optical -- HARPS-N (harps_spectra.npy)</li> <li>Optical/NIR -- PHOENIX model (phoenix_grid_3700_4.5_0.0.npy)</li> </ul> </li> <li><strong>A table of 176 measured emission lines from the HST/COS spectra of AU Mic (</strong>au_mic_full_emission_line_list.txt<strong>)</strong></li> <li><strong>The modeled transmission spectra for AU Mic b and c and a demonstration Jupyter notebook for how to read in the files</strong> (tp_profile_demo.ipynb): <ul> <li>Disequilibrium model for AU Mic b (au_mic_b_disequil_profile.dat)</li> <li>Disequilibrium model for AU Mic c (au_mic_c_disequil_profile.dat)</li> <li>Equilibrium model for AU Mic b (au_mic_b_equil_profile.dat)</li> <li>Equilibrium model for AU Mic c (au_mic_c_equil_profile.dat)</li> </ul> </li> </ul>
THE FLARING ACTIVITY OF M DWARFS IN KEPLER FIELD
<p>The Kepler flux, M dwarfs that include flares,the format consist of four columns:<br> <br> BKJD Relative Flux Fit line Flare Flux</p> <p>the Relative flux wil be empty when flares occur, the flares flux will be empty when quiescent flux.</p> <p>the file lamost_obsid is the spectra used in this work, one can use the obsid to download the fits through the following website: http://dr4.lamost.org/</p>
Fig. 1 in Form and formation of flares and parabolae based on new observations of the internal shell structure in lytoceratid and perisphinctid ammonoids
Fig. 1. Different expressions of flares (A) and parabolae (B).
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OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.