<?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>Quantum Calculation of the Vibrational Excitation of Nitrogen Molecules by Fast Ions: Can It Contribute to STEVE Formation?</dc:title><dc:creator>Liang, Jun [Department of Physics &amp;amp; Astronomy University of Calgary  Calgary AB Canada] (ORCID:0000000245902978); Donovan, Eric [Department of Physics &amp;amp; Astronomy University of Calgary  Calgary AB Canada]</dc:creator><dc:corporate_author/><dc:editor/><dc:description>&lt;title&gt;Abstract&lt;/title&gt; &lt;p&gt;The vibrational‐translational (VT) excitation of nitrogen molecules led by collisions with fast ions in subauroral ion drifts (SAID) has been conceived as a potential underlying mechanism contributing to the formation of the Strong Thermal Emission Velocity Enhancement (STEVE) phenomenon (Harding et al., 2020,&lt;ext-link href='https://doi.org/10.1029/2020gl087102'&gt;https://doi.org/10.1029/2020gl087102&lt;/ext-link&gt;). In this study, we perform quantum calculations of the VT excitation rates of N&lt;sub&gt;2&lt;/sub&gt;led by fast‐drifting ions, and evaluate the resulting vibrational distribution of N&lt;sub&gt;2&lt;/sub&gt;with ionospheric/thermospheric parameters expected under intense SAID condition. We conclude that, while the VT energy transfer led by SAID plays a distinguishable role in the vibrational excitation of N&lt;sub&gt;2&lt;/sub&gt;, it is incapable of populating the high vibrational levels to the required concentration (Harding et al., 2020,&lt;ext-link href='https://doi.org/10.1029/2020gl087102'&gt;https://doi.org/10.1029/2020gl087102&lt;/ext-link&gt;) to produce adequate nitric oxide density, and in turn the nitrogen‐dioxide continuum intensity, to account for the STEVE brightness.&lt;/p&gt;</dc:description><dc:publisher>Wiley</dc:publisher><dc:date>2024-09-16</dc:date><dc:nsf_par_id>10674359</dc:nsf_par_id><dc:journal_name>Geophysical Research Letters</dc:journal_name><dc:journal_volume>51</dc:journal_volume><dc:journal_issue>17</dc:journal_issue><dc:page_range_or_elocation/><dc:issn>0094-8276</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.1029/2024GL110986</dc:doi><dcq:identifierAwardId>2445467</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>