<?xml version="1.0" encoding="UTF-8" ?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-10-14T06:23:00Z</responseDate><request identifier="10.35097/gbvnuvzqg1g7ykut" metadataPrefix="oai_dc" verb="GetRecord">https://www.radar-service.eu/oai/OAIHandler</request><GetRecord><record><header><identifier>10.35097/gbvnuvzqg1g7ykut</identifier><datestamp>2026-10-09T10:45:15Z</datestamp><setSpec>IMK</setSpec><setSpec>radar4kit</setSpec></header><metadata><oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/"
           xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/"
           xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
           xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ https://www.openarchives.org/OAI/2.0/oai_dc.xsd">
   <dc:identifier>https://dx.doi.org/10.35097/gbvnuvzqg1g7ykut</dc:identifier>
   <dc:creator>Muth, Lisa</dc:creator>
   <dc:title>ICON-ART Simulations and Satellite Observations from Influence of Fire-Induced Heat and Moisture Release on Pyro-Convective Cloud Dynamics during the Australian New Year’s Event: A Study Using Convection-Resolving Simulations and Satellite Data (egusphere-2025-402)</dc:title>
   <dc:publisher>Karlsruhe Institute of Technology</dc:publisher>
   <dc:date>2025</dc:date>
   <dc:subject>Other</dc:subject>
   <dc:subject>Atmospheric Science</dc:subject>
   <dc:type>dataset</dc:type>
   <dc:subject>Model</dc:subject>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights>
   <dc:description>The folder 3dwinds includes height retrieval data from the NASA 3D Wind Algorithm, which is based on Himawari-8 and MODIS Level 1B in the blue band. Access to this algorithm was granted by Dr. James Carr (jcarr@carrastro.com) and is subject to his approval. The ICON-ART Raw Data of the model output files is zipped for three experiments: model_output_REF.tar.gz (REF), model_output_SH.tar.gz (SH), and model_output_SHLH.tar.gz (SHLH). The folder fire_input+domain includes the fire input file as it is read into the ICON-ART model, along with the model domain grid file. Additionally, the file fire_archive_M-C61_611434.csv contains MODIS active fire product data. The original dataset can be accessed via NASA FIRMS at https://earthdata.nasa.gov/earth-observation-data/near-real-time/firms/mcd14ml.</dc:description>
   <dc:description>This data package contains all datasets required to reproduce the plots presented in the manuscript egusphere-2025-402. nfluence of Fire-Induced Heat and Moisture Release on Pyro-Convective Cloud Dynamics During the Australian New Year's Event: A Study Using Convection-Resolving Simulations and Satellite Data [ACP]</dc:description>
   <dc:subject>Pyro-Convection </dc:subject>
   <dc:subject>Australian New Year’s Event</dc:subject>
   <dc:subject>Convection-Resolving Simulation</dc:subject>
   <dc:subject>ICON-ART model</dc:subject>
   <dc:format>application/x-tar</dc:format>
</oai_dc:dc></metadata></record></GetRecord></OAI-PMH>