<?xml version="1.0" encoding="UTF-8"?><rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcq="http://purl.org/dc/terms/"><records count="1" morepages="false" start="1" end="1"><record rownumber="1"><dc:product_type>Journal Article</dc:product_type><dc:title>Super Dual Auroral Radar Network Expansion and Its Influence on the Derived Ionospheric Convection Pattern</dc:title><dc:creator>Walach, M.‐T.; Grocott, A.; Staples, F.; Thomas, E. G.</dc:creator><dc:corporate_author/><dc:editor/><dc:description>Key Points                                                            We identify changes in derived convection maps when PolarDARN and StormDARN are added, and show the impact of different processing                                                  Derived convection parameters are highly susceptible to processing variables and which radars are included                                                  We show how the number of backscatter echoes per map is critical to the integrity of the maps, and discuss how this impacts map quality</dc:description><dc:publisher/><dc:date>2022-02-01</dc:date><dc:nsf_par_id>10450451</dc:nsf_par_id><dc:journal_name>Journal of Geophysical Research: Space Physics</dc:journal_name><dc:journal_volume>127</dc:journal_volume><dc:journal_issue>2</dc:journal_issue><dc:page_range_or_elocation/><dc:issn>2169-9380</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.1029/2021JA029559</dc:doi><dcq:identifierAwardId>1934997</dcq:identifierAwardId><dc:subject/><dc:version_number/><dc:location/><dc:rights/><dc:institution/><dc:sponsoring_org>National Science Foundation</dc:sponsoring_org></record></records></rdf:RDF>