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              <creatorName>Forsyth, Colin</creatorName>
              <givenName>Colin</givenName>
              <familyName>Forsyth</familyName>
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            <creator>
              <creatorName>Lao, Christian</creatorName>
              <givenName>Christian</givenName>
              <familyName>Lao</familyName>
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            <creator>
              <creatorName>Freeman, Mervyn</creatorName>
              <givenName>Mervyn</givenName>
              <familyName>Freeman</familyName>
              <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org">0000-0002-8653-8279</nameIdentifier>
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            <creator>
              <creatorName>Gjerloev, Jesper</creatorName>
              <givenName>Jesper</givenName>
              <familyName>Gjerloev</familyName>
              <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org">0000-0002-7277-9004</nameIdentifier>
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          <titles>
            <title><![CDATA[SOPHIE substorm identifications (EPT90) with varying thresholds for convection enhancement identification]]></title>
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          <subjects>
            <subject>Heliophysics and space weather</subject>
            <subject>Mesospheric, thermospheric, ionospheric and magnetospheric physics</subject>
            <subject>Substorm occurrence</subject>
          </subjects>
          <dates>
            <date dateType="Created">2025-01-27</date>
            <date dateType="Updated">2025-01-27</date>
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          <resourceType resourceTypeGeneral="Dataset">Dataset</resourceType>
          <publicationYear>2025</publicationYear>
          <publisher>University College London</publisher>
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            <description descriptionType="Abstract"><![CDATA[<p dir="ltr">Outputs from the SOPHIE (Forsyth et al., 2015, 10.1002/2015JA021343) substorm onset and phase detection technique for SuperMAG data between 1997 and 2020 (inclusive).</p><p dir="ltr">This version has been updated in to include the MLT and MLAT of the SuperMAG station providing the SML data</p><p dir="ltr">This file provides the start times of growth/energy input, expansion and recovery phases determined by SOPHIE for an EPT of 90.</p><p dir="ltr">Data generated for "Separating DP1 and DP2 current pattern contributions to substorm-like intensifications in SML" by Lao et al., submitted to Journal of Geophysical Research: Space Physics.</p><p><br></p><p dir="ltr">The data is presented in 7 columns: -</p><p dir="ltr">The date and time of the first data point in the given phase (YYYY/MM/DD-HH:MM:SS)</p><p dir="ltr">The phase number (1 for growth/energy input, 2 for expansion, 3 for recovery)</p><p dir="ltr">A flag indicating that the rate of change of SMU is similar to that of SML in the expansion phase. This number is a sum of the following indicators:<br>1 = the ratio of median rate of change of -SML_f and median rate of change of SMU_f is less than the stated threshold</p><p dir="ltr">2 = the ratio of mean rate of change of -SML_f and mean rate of change of SMU_f is less than the stated threshold<br>4 = the ratio of the change in -SML_f and the change in SMU_f is less than the stated threshold<br>8 = the ratio of the change in -SML and the change in SMU is less than the stated threshold<br>SML_f and SMU_f are SML and SMU passed through a 30 min low pass filter.<br>As an example, a flag of 03 indicates that both the median (1) and mean (2) rates of change were less than the threshold. A flag of 05 would indicate that the mean rate of change and the ratio of the filtered SML/U values were less than the threshold, but not the ratio of the median rate of changes.</p><p><br></p><p dir="ltr">MLT of the active SML station at the shown time</p><p dir="ltr">MLAT of the active SML station at the shown time</p><p dir="ltr">Change in SML during the upcoming phase (i.e. if time is for start of expansion phase, this is the drop in SML during that expansion phase)</p><p dir="ltr">SML value at end of phase.</p><p dir="ltr">The original SuperMAG indices can be downloaded from https://supermag.jhuapl.edu/</p>]]></description>
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