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7 results for “Magnetosheath Jets”

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zenodo44/100

Magnetosheath Jets MMS1 (5/2015 - 6/2020) - Classified

<p><strong>README</strong></p> <p>This dataset contains the time and the class of magnetosheath jets observed by MMS 1 during 05/2015 &ndash; 06/2020.&nbsp;</p> <p>More information about the different classes can be found in the articles:</p> <ol> <li>https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2019JA027754</li> <li>https://www.frontiersin.org/articles/10.3389/fspas.2020.00024/full</li> </ol> <p>While an extension of the classification process has been published in:</p> <ul> <li>https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2021JA029269</li> </ul> <p><strong>INFO</strong>&nbsp;</p> <p>For the attached text file. The first column is the time of maximum dynamic pressure in UTC. The second column is the class of the jet:</p> <p><em>Main Categories:</em><br>11 =&nbsp;Quasi-parallel jet<br>22 =&nbsp;Quasi-perpendicular jet &nbsp;<br>3 =&nbsp;Boundary jet<br>5 =&nbsp;Encapsulated jet&nbsp;</p> <p><em>Secondary Categories:</em><br>1 =&nbsp;Possibly Quasi-parallel jet<br>2 =&nbsp;Possibly Quasi-parallel jet<br>4 =&nbsp;&nbsp;Possibly Boundary jet<br>6 =&nbsp;Possibly Encapsulated jet<br>7 =&nbsp;Close to Magnetopause or Bow Shock jet<br>0 =&nbsp;Unclassified jet<br>8 =&nbsp;Data gap jet</p> <p>Burst availability is given in the third column as:</p> <p>2 =&nbsp;Full burst availability<br>1 = Partial burst availability<br>0 = No burst availability</p> <p>For more information, please contact the author (savvasraptis@gmail.com)&nbsp;</p>

opencc-by-4.0Sep 2022View details →
zenodo40/100

Magnetosheath Jets MMS (5/2015 - 6/2019)

<p>This dataset contains&nbsp;the jets and their classes that are used and analyzed in the paper:&nbsp;<a href="https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2019JA027754">https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2019JA027754</a>&nbsp;</p> <p>The list&nbsp;has been generated using MMS1 satellite with data from 5/2015 to 6/2019.</p> <p>More information can be found in the manuscript and its supplementary material.&nbsp;</p> <p>&nbsp;</p> <p>&nbsp;</p>

opencc-by-4.0Apr 2020View details →
zenodo40/100

Movies (II) for "3D Space-Time Adaptive Hybrid Simulations of Magnetosheath High-Speed Jets"

<p>Movies for the aforementioned paper showing magnetic field lines, dynamic pressure and plasma density in global magnetospheric simulations. NW and SW refer to quasi-radial northward and southward IMF.&nbsp;</p> <p>https://doi.org/10.1029/2020JA029035</p>

opencc-by-4.0Jun 2024View details →
zenodo36/100

Dataset for the paper "The Comprehensive Response of the Magnetopause to the Impact of a Magnetosheath High-Speed Jet"

<p>This dataset is used for the paper "The Comprehensive Response of the Magnetopause to the Impact of a Magnetosheath High-Speed Jet" and contains publicly available data of MMS dayside magnetopause crossing events with high-speed jet events from 2015 to 2020. It includes crossing times, high-speed jet durations, the normals from the model and observations (Timing and MVA methods), and the temporal and spatial response scales of the magnetopause for all 20 MP response events in geocentric solar magnetospheric (GSM) coordinates.</p>

opencc-by-4.0Jul 2024View details →
zenodo32/100

Empirical models of "Magnetosheath Jets Over Solar Cycle 24: An Empirical Model"

<p>The empirical models of jet observations rates as a function of solar wind parameters used in the article&nbsp;&quot;Magnetosheath Jets Over Solar Cycle 24: An Empirical Model&quot; by L.Vuorinen, A. T. LaMoury, H. Hietala, and F. Koller. Please&nbsp;contact L. Vuorinen (lakavu@utu.fi) for additional information.</p>

opencc-by-4.0Aug 2023View details →
zenodo28/100

Magnetosheath Jets (Qpar-Qperp) Classification

<p>Dataset of magnetosheath jets used in the article&nbsp;&ldquo;Classification of Magnetosheath Jets Using Neural Networks and High Resolution OMNI (HRO) Data&rdquo;.</p> <p>The dataset contains the time of observation, the initial classification and the characterization provided by the four different methods presented in the main article.&nbsp;</p> <p>The list&nbsp;has been generated using MMS1 satellite with data from 5/2015 to 6/2019.</p> <p><em>Notes</em>:</p> <p>0 = NaN data (No class)</p> <p>1 = Quasi - Parallel Jet</p> <p>2 = Quasi - Perpendicular Jet</p>

opencc-by-4.0Apr 2020View details →
zenodo28/100

Plot data for the paper "Jets in the Magnetosheath: IMF Control of Where They Occur"

<p>Plot data for the histograms, 2D maps and bar plot&nbsp;of the paper &quot;Jets in the Magnetosheath: IMF Control of Where They Occur&quot; by L.Vuorinen, H. Hietala, and F. Plaschke. Please&nbsp;contact L. Vuorinen (lakavu@utu.fi) for additional information.</p>

opencc-by-4.0Apr 2019View details →

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