https://gem.epss.ucla.edu/mediawiki/index.php?action=history&feed=atom&title=GEM_Focus_Groups
GEM Focus Groups - Revision history
2026-05-01T19:48:19Z
Revision history for this page on the wiki
MediaWiki 1.33.0
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7368&oldid=prev
Savvra: /* Active Focus Groups */
2026-04-24T16:39:38Z
<p><span dir="auto"><span class="autocomment">Active Focus Groups</span></span></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 16:39, 24 April 2026</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l11" >Line 11:</td>
<td colspan="2" class="diff-lineno">Line 11:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Comparative Planetary Magnetospheric Processes|<b>(COMP)</b> Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Comparative Planetary Magnetospheric Processes|<b>(COMP)</b> Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|<b>(KiTS)</b> Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|<b>(KiTS)</b> Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Multiscale Dayside Transients and their Effect on Earth's Magnetosphere|<b>(MDT)</b> Multiscale Dayside Transients and their Effect on Earth's Magnetosphere]] (2025 - 2029; Savvas Raptis, Ivan Vasko, Imogen Gingell, Terry Z. Liu, Ying Zou, Runyi Liu, David Tonoian; RA: Primary - SWMI)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Multiscale Dayside Transients and their Effect on Earth's Magnetosphere|<b>(MDT)</b> Multiscale Dayside Transients and their Effect on Earth's Magnetosphere]] (2025 - 2029; Savvas Raptis, Ivan Vasko<ins class="diffchange diffchange-inline">, Yuxi Chen, Gonzalo Cucho-Padin</ins>, Imogen Gingell, Terry Z. Liu, Ying Zou, Runyi Liu, David Tonoian; RA: Primary - SWMI)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td></tr>
</table>
Savvra
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7351&oldid=prev
AllisonJaynes at 23:40, 23 February 2026
2026-02-23T23:40:12Z
<p></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 23:40, 23 February 2026</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l14" >Line 14:</td>
<td colspan="2" class="diff-lineno">Line 14:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetosphere-Aurora Connection|<b>(<del class="diffchange diffchange-inline">MAG</del>)</b> Magnetosphere-Aurora Connection]] (<del class="diffchange diffchange-inline">MAG</del>) (2026-2030; Toshi Nishimura, Tetsuo Motoba, Shannon Hill, and Bea Gallardo-Lacourt; RA: Primary – MIC, Secondary – MPS and IMAG)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetosphere-Aurora Connection|<b>(<ins class="diffchange diffchange-inline">MAC</ins>)</b> Magnetosphere-Aurora Connection]] (<ins class="diffchange diffchange-inline">MAC</ins>) (2026-2030; Toshi Nishimura, Tetsuo Motoba, Shannon Hill, and Bea Gallardo-Lacourt; RA: Primary – MIC, Secondary – MPS and IMAG)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td></tr>
</table>
AllisonJaynes
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7318&oldid=prev
MtDFG: /* Active Focus Groups */
2026-01-30T23:55:20Z
<p><span dir="auto"><span class="autocomment">Active Focus Groups</span></span></p>
<table class="diff diff-contentalign-left" data-mw="interface">
<col class="diff-marker" />
<col class="diff-content" />
<col class="diff-marker" />
<col class="diff-content" />
<tr class="diff-title" lang="en">
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 23:55, 30 January 2026</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l14" >Line 14:</td>
<td colspan="2" class="diff-lineno">Line 14:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[FG: Magnetosphere-Aurora Connection|<b>(MAG)</b> Magnetosphere-Aurora Connection]] (MAG) (2026-2030; Toshi Nishimura, Tetsuo Motoba, Shannon Hill, and Bea Gallardo-Lacourt; RA: Primary – MIC, Secondary – MPS and IMAG)</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td></tr>
</table>
MtDFG
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7235&oldid=prev
MtDFG at 17:19, 16 July 2025
2025-07-16T17:19:29Z
<p></p>
<table class="diff diff-contentalign-left" data-mw="interface">
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<col class="diff-marker" />
<col class="diff-content" />
<tr class="diff-title" lang="en">
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 17:19, 16 July 2025</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l6" >Line 6:</td>
<td colspan="2" class="diff-lineno">Line 6:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Active Focus Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Active Focus Groups==</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">* [[FG: The Impact of the Cold Plasma in Magnetospheric Physics|<b>(CP)</b> The Impact of the Cold Plasma in Magnetospheric Physics]] (2020 - 2025; Gian Luca Delzanno, Natalia Buzulukosva, Barbara Giles, Roger Varney, and Joe Borovsky; RA: Primary – IMAG, Secondary – None)</del></div></td><td colspan="2"> </td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">* [[FG: Self-Consistent Inner Magnetospheric Modeling|<b>(SCIMM)</b> Self-Consistent Inner Magnetospheric Modeling]] (2020 - 2025; Cristian Ferradas, Chao Yue, Jacob Bortnik, and Qianli Ma; RA: Primary – IMAG, Secondary – MIC)</del></div></td><td colspan="2"> </td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents|<b>(GIC)</b> Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents]] (2022 - 2026; Xueling Shi, Dogacan Su Ozturk, Mark Engebretson, Zhonghua Xu, E. Joshua Rigler; RA: Primary – GSM, Secondary – MIC)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents|<b>(GIC)</b> Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents]] (2022 - 2026; Xueling Shi, Dogacan Su Ozturk, Mark Engebretson, Zhonghua Xu, E. Joshua Rigler; RA: Primary – GSM, Secondary – MIC)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|<b>(MESO)</b> Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>*[[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|<b>(MESO)</b> Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).</div></td></tr>
<tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l24" >Line 24:</td>
<td colspan="2" class="diff-lineno">Line 22:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Past Focus Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Past Focus Groups==</div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[FG: The Impact of the Cold Plasma in Magnetospheric Physics|<b>(CP)</b> The Impact of the Cold Plasma in Magnetospheric Physics]] (2020 - 2025; Gian Luca Delzanno, Natalia Buzulukosva, Barbara Giles, Roger Varney, and Joe Borovsky; RA: Primary – IMAG, Secondary – None)</ins></div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div><ins style="font-weight: bold; text-decoration: none;">* [[FG: Self-Consistent Inner Magnetospheric Modeling|<b>(SCIMM)</b> Self-Consistent Inner Magnetospheric Modeling]] (2020 - 2025; Cristian Ferradas, Chao Yue, Jacob Bortnik, and Qianli Ma; RA: Primary – IMAG, Secondary – MIC)</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetic Reconnection in the Age of the Heliophysics System Observatory|Magnetic Reconnection in the Age of the Heliophysics System Observatory]] (2018 - 2024; Tori Wilder, Shan Wang, Michael Shay, and Anton Artemyev; RA: Primary – GSM, Secondary – None)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetic Reconnection in the Age of the Heliophysics System Observatory|Magnetic Reconnection in the Age of the Heliophysics System Observatory]] (2018 - 2024; Tori Wilder, Shan Wang, Michael Shay, and Anton Artemyev; RA: Primary – GSM, Secondary – None)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling|System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling]] (2019 - 2024; Hong Zhao, Lauren Blum, Sasha Ukhorskiy, and Xiangrong Fu; RA: Primary – IMAG, Secondary – None)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling|System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling]] (2019 - 2024; Hong Zhao, Lauren Blum, Sasha Ukhorskiy, and Xiangrong Fu; RA: Primary – IMAG, Secondary – None)</div></td></tr>
</table>
MtDFG
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7234&oldid=prev
MtDFG: /* Standing Resource Groups */
2025-07-16T17:18:55Z
<p><span dir="auto"><span class="autocomment">Standing Resource Groups</span></span></p>
<table class="diff diff-contentalign-left" data-mw="interface">
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 17:18, 16 July 2025</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l21" >Line 21:</td>
<td colspan="2" class="diff-lineno">Line 21:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; Alexa Halford, Josh Rigler, Qusai Al Shidi, Huayue Chen)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; Alexa Halford, Josh Rigler, Qusai Al Shidi, Huayue Chen)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <del class="diffchange diffchange-inline"><span style="background:#ccff99"></del>[[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor, Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor, Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Past Focus Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Past Focus Groups==</div></td></tr>
</table>
MtDFG
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7233&oldid=prev
MtDFG: /* Active Focus Groups */
2025-07-16T17:18:47Z
<p><span dir="auto"><span class="autocomment">Active Focus Groups</span></span></p>
<table class="diff diff-contentalign-left" data-mw="interface">
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 17:18, 16 July 2025</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l6" >Line 6:</td>
<td colspan="2" class="diff-lineno">Line 6:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Active Focus Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Active Focus Groups==</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <del class="diffchange diffchange-inline"><span style="background:#ccff99"></del>[[FG: The Impact of the Cold Plasma in Magnetospheric Physics|<b>(CP)</b> The Impact of the Cold Plasma in Magnetospheric Physics]] (2020 - 2025; Gian Luca Delzanno, Natalia Buzulukosva, Barbara Giles, Roger Varney, and Joe Borovsky; RA: Primary – IMAG, Secondary – None)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: The Impact of the Cold Plasma in Magnetospheric Physics|<b>(CP)</b> The Impact of the Cold Plasma in Magnetospheric Physics]] (2020 - 2025; Gian Luca Delzanno, Natalia Buzulukosva, Barbara Giles, Roger Varney, and Joe Borovsky; RA: Primary – IMAG, Secondary – None)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <del class="diffchange diffchange-inline"><span style="background:#ccff99"></del>[[FG: Self-Consistent Inner Magnetospheric Modeling|<b>(SCIMM)</b> Self-Consistent Inner Magnetospheric Modeling]] (2020 - 2025; Cristian Ferradas, Chao Yue, Jacob Bortnik, and Qianli Ma; RA: Primary – IMAG, Secondary – MIC)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Self-Consistent Inner Magnetospheric Modeling|<b>(SCIMM)</b> Self-Consistent Inner Magnetospheric Modeling]] (2020 - 2025; Cristian Ferradas, Chao Yue, Jacob Bortnik, and Qianli Ma; RA: Primary – IMAG, Secondary – MIC)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents|<b>(GIC)</b> Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents]] (2022 - 2026; Xueling Shi, Dogacan Su Ozturk, Mark Engebretson, Zhonghua Xu, E. Joshua Rigler; RA: Primary – GSM, Secondary – MIC)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents|<b>(GIC)</b> Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents]] (2022 - 2026; Xueling Shi, Dogacan Su Ozturk, Mark Engebretson, Zhonghua Xu, E. Joshua Rigler; RA: Primary – GSM, Secondary – MIC)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*<del class="diffchange diffchange-inline"><span style="background:#ccff99"> </del>[[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|<b>(MESO)</b> Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*[[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|<b>(MESO)</b> Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <del class="diffchange diffchange-inline"><span style="background:#ccff99"></del>[[FG: Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems|<b>(MPEC)</b> Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems]] (2022 - 2026; Dogacan Su Ozturk, Dong Lin, Yiqun Yu, Katherine Garcia-Sage, Stephen Kaeppler; RA: Primary – MIC, Secondary – GSM)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems|<b>(MPEC)</b> Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems]] (2022 - 2026; Dogacan Su Ozturk, Dong Lin, Yiqun Yu, Katherine Garcia-Sage, Stephen Kaeppler; RA: Primary – MIC, Secondary – GSM)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <del class="diffchange diffchange-inline"><span style="background:#ccff99"></del>[[FG: Comparative Planetary Magnetospheric Processes|<b>(COMP)</b> Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Comparative Planetary Magnetospheric Processes|<b>(COMP)</b> Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|<b>(KiTS)</b> Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|<b>(KiTS)</b> Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Multiscale Dayside Transients and their Effect on Earth's Magnetosphere|<b>(MDT)</b> Multiscale Dayside Transients and their Effect on Earth's Magnetosphere]] (2025 - 2029; Savvas Raptis, Ivan Vasko, Imogen Gingell, Terry Z. Liu, Ying Zou, Runyi Liu, David Tonoian; RA: Primary - SWMI)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Multiscale Dayside Transients and their Effect on Earth's Magnetosphere|<b>(MDT)</b> Multiscale Dayside Transients and their Effect on Earth's Magnetosphere]] (2025 - 2029; Savvas Raptis, Ivan Vasko, Imogen Gingell, Terry Z. Liu, Ying Zou, Runyi Liu, David Tonoian; RA: Primary - SWMI)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <del class="diffchange diffchange-inline"><span style="background:#ccff99"></del>[[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <del class="diffchange diffchange-inline"><span style="background:#ccff99"></del>[[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;"></del></div></td><td colspan="2"> </td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div><del style="font-weight: bold; text-decoration: none;">Note: FGs and resource groups <span style="background:#ccff99">highlighted in green</span> have expressed interest in collaborating with CEDAR for the 2025 GEM-CEDAR Joint Meeting.</del></div></td><td colspan="2"> </td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td></tr>
</table>
MtDFG
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7230&oldid=prev
AllisonJaynes: /* Standing Resource Groups */
2025-07-14T17:42:25Z
<p><span dir="auto"><span class="autocomment">Standing Resource Groups</span></span></p>
<table class="diff diff-contentalign-left" data-mw="interface">
<col class="diff-marker" />
<col class="diff-content" />
<col class="diff-marker" />
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<tr class="diff-title" lang="en">
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 17:42, 14 July 2025</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l22" >Line 22:</td>
<td colspan="2" class="diff-lineno">Line 22:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; <del class="diffchange diffchange-inline">Mike Liemohn, Lutz Rastaetter, </del>Alexa Halford <del class="diffchange diffchange-inline">and </del>Josh Rigler)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; Alexa Halford<ins class="diffchange diffchange-inline">, </ins>Josh Rigler<ins class="diffchange diffchange-inline">, Qusai Al Shidi, Huayue Chen</ins>)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#ccff99">[[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor<del class="diffchange diffchange-inline">. </del>Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#ccff99">[[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor<ins class="diffchange diffchange-inline">, </ins>Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Past Focus Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Past Focus Groups==</div></td></tr>
</table>
AllisonJaynes
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7013&oldid=prev
AllisonJaynes: /* Standing Resource Groups */
2025-05-15T10:30:18Z
<p><span dir="auto"><span class="autocomment">Standing Resource Groups</span></span></p>
<table class="diff diff-contentalign-left" data-mw="interface">
<col class="diff-marker" />
<col class="diff-content" />
<col class="diff-marker" />
<col class="diff-content" />
<tr class="diff-title" lang="en">
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 10:30, 15 May 2025</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l23" >Line 23:</td>
<td colspan="2" class="diff-lineno">Line 23:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; Mike Liemohn, Lutz Rastaetter, Alexa Halford and Josh Rigler)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; Mike Liemohn, Lutz Rastaetter, Alexa Halford and Josh Rigler)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<del class="diffchange diffchange-inline">00ffae</del>">[[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor. Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<ins class="diffchange diffchange-inline">ccff99</ins>">[[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor. Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Past Focus Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Past Focus Groups==</div></td></tr>
</table>
AllisonJaynes
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7012&oldid=prev
AllisonJaynes: /* Active Focus Groups */
2025-05-15T10:30:03Z
<p><span dir="auto"><span class="autocomment">Active Focus Groups</span></span></p>
<table class="diff diff-contentalign-left" data-mw="interface">
<col class="diff-marker" />
<col class="diff-content" />
<col class="diff-marker" />
<col class="diff-content" />
<tr class="diff-title" lang="en">
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">← Older revision</td>
<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 10:30, 15 May 2025</td>
</tr><tr><td colspan="2" class="diff-lineno" id="mw-diff-left-l6" >Line 6:</td>
<td colspan="2" class="diff-lineno">Line 6:</td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Active Focus Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Active Focus Groups==</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<del class="diffchange diffchange-inline">cfeb34</del>">[[FG: The Impact of the Cold Plasma in Magnetospheric Physics|<b>(CP)</b> The Impact of the Cold Plasma in Magnetospheric Physics]] (2020 - 2025; Gian Luca Delzanno, Natalia Buzulukosva, Barbara Giles, Roger Varney, and Joe Borovsky; RA: Primary – IMAG, Secondary – None)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<ins class="diffchange diffchange-inline">ccff99</ins>">[[FG: The Impact of the Cold Plasma in Magnetospheric Physics|<b>(CP)</b> The Impact of the Cold Plasma in Magnetospheric Physics]] (2020 - 2025; Gian Luca Delzanno, Natalia Buzulukosva, Barbara Giles, Roger Varney, and Joe Borovsky; RA: Primary – IMAG, Secondary – None)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<del class="diffchange diffchange-inline">00ffae</del>">[[FG: Self-Consistent Inner Magnetospheric Modeling|<b>(SCIMM)</b> Self-Consistent Inner Magnetospheric Modeling]] (2020 - 2025; Cristian Ferradas, Chao Yue, Jacob Bortnik, and Qianli Ma; RA: Primary – IMAG, Secondary – MIC)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<ins class="diffchange diffchange-inline">ccff99</ins>">[[FG: Self-Consistent Inner Magnetospheric Modeling|<b>(SCIMM)</b> Self-Consistent Inner Magnetospheric Modeling]] (2020 - 2025; Cristian Ferradas, Chao Yue, Jacob Bortnik, and Qianli Ma; RA: Primary – IMAG, Secondary – MIC)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents|<b>(GIC)</b> Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents]] (2022 - 2026; Xueling Shi, Dogacan Su Ozturk, Mark Engebretson, Zhonghua Xu, E. Joshua Rigler; RA: Primary – GSM, Secondary – MIC)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents|<b>(GIC)</b> Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents]] (2022 - 2026; Xueling Shi, Dogacan Su Ozturk, Mark Engebretson, Zhonghua Xu, E. Joshua Rigler; RA: Primary – GSM, Secondary – MIC)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*<span style="background:#<del class="diffchange diffchange-inline">00ffae</del>"> [[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|<b>(MESO)</b> Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*<span style="background:#<ins class="diffchange diffchange-inline">ccff99</ins>"> [[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|<b>(MESO)</b> Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<del class="diffchange diffchange-inline">00ffae</del>">[[FG: Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems|<b>(MPEC)</b> Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems]] (2022 - 2026; Dogacan Su Ozturk, Dong Lin, Yiqun Yu, Katherine Garcia-Sage, Stephen Kaeppler; RA: Primary – MIC, Secondary – GSM)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<ins class="diffchange diffchange-inline">ccff99</ins>">[[FG: Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems|<b>(MPEC)</b> Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems]] (2022 - 2026; Dogacan Su Ozturk, Dong Lin, Yiqun Yu, Katherine Garcia-Sage, Stephen Kaeppler; RA: Primary – MIC, Secondary – GSM)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<del class="diffchange diffchange-inline">00ffae</del>">[[FG: Comparative Planetary Magnetospheric Processes|<b>(COMP)</b> Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<ins class="diffchange diffchange-inline">ccff99</ins>">[[FG: Comparative Planetary Magnetospheric Processes|<b>(COMP)</b> Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|<b>(KiTS)</b> Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|<b>(KiTS)</b> Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Multiscale Dayside Transients and their Effect on Earth's Magnetosphere|<b>(MDT)</b> Multiscale Dayside Transients and their Effect on Earth's Magnetosphere]] (2025 - 2029; Savvas Raptis, Ivan Vasko, Imogen Gingell, Terry Z. Liu, Ying Zou, Runyi Liu, David Tonoian; RA: Primary - SWMI)</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Multiscale Dayside Transients and their Effect on Earth's Magnetosphere|<b>(MDT)</b> Multiscale Dayside Transients and their Effect on Earth's Magnetosphere]] (2025 - 2029; Savvas Raptis, Ivan Vasko, Imogen Gingell, Terry Z. Liu, Ying Zou, Runyi Liu, David Tonoian; RA: Primary - SWMI)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<del class="diffchange diffchange-inline">00ffae</del>">[[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<ins class="diffchange diffchange-inline">ccff99</ins>">[[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<b>(RX)</b> Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<del class="diffchange diffchange-inline">00ffae</del>">[[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<ins class="diffchange diffchange-inline">ccff99</ins>">[[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>Note: FGs and resource groups <span style="background:#<del class="diffchange diffchange-inline">00ffae</del>">highlighted in green</span> have expressed interest in collaborating with CEDAR for the 2025 GEM-CEDAR Joint Meeting.</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>Note: FGs and resource groups <span style="background:#<ins class="diffchange diffchange-inline">ccff99</ins>">highlighted in green</span> have expressed interest in collaborating with CEDAR for the 2025 GEM-CEDAR Joint Meeting.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Standing Resource Groups==</div></td></tr>
</table>
AllisonJaynes
https://gem.epss.ucla.edu/mediawiki/index.php?title=GEM_Focus_Groups&diff=7011&oldid=prev
AllisonJaynes: /* Active Focus Groups */
2025-05-15T10:28:28Z
<p><span dir="auto"><span class="autocomment">Active Focus Groups</span></span></p>
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<td colspan="2" style="background-color: #fff; color: #222; text-align: center;">Revision as of 10:28, 15 May 2025</td>
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<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Active Focus Groups==</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>==Active Focus Groups==</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<del class="diffchange diffchange-inline">00ffae</del>">[[FG: The Impact of the Cold Plasma in Magnetospheric Physics|(CP) The Impact of the Cold Plasma in Magnetospheric Physics]] (2020 - 2025; Gian Luca Delzanno, Natalia Buzulukosva, Barbara Giles, Roger Varney, and Joe Borovsky; RA: Primary – IMAG, Secondary – None)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#<ins class="diffchange diffchange-inline">cfeb34</ins>">[[FG: The Impact of the Cold Plasma in Magnetospheric Physics|<ins class="diffchange diffchange-inline"><b></ins>(CP)<ins class="diffchange diffchange-inline"></b> </ins>The Impact of the Cold Plasma in Magnetospheric Physics]] (2020 - 2025; Gian Luca Delzanno, Natalia Buzulukosva, Barbara Giles, Roger Varney, and Joe Borovsky; RA: Primary – IMAG, Secondary – None)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Self-Consistent Inner Magnetospheric Modeling|(SCIMM) Self-Consistent Inner Magnetospheric Modeling]] (2020 - 2025; Cristian Ferradas, Chao Yue, Jacob Bortnik, and Qianli Ma; RA: Primary – IMAG, Secondary – MIC)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Self-Consistent Inner Magnetospheric Modeling|<ins class="diffchange diffchange-inline"><b></ins>(SCIMM)<ins class="diffchange diffchange-inline"></b> </ins>Self-Consistent Inner Magnetospheric Modeling]] (2020 - 2025; Cristian Ferradas, Chao Yue, Jacob Bortnik, and Qianli Ma; RA: Primary – IMAG, Secondary – MIC)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents|(GIC) Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents]] (2022 - 2026; Xueling Shi, Dogacan Su Ozturk, Mark Engebretson, Zhonghua Xu, E. Joshua Rigler; RA: Primary – GSM, Secondary – MIC)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents|<ins class="diffchange diffchange-inline"><b></ins>(GIC)<ins class="diffchange diffchange-inline"></b> </ins>Understanding the causes of geomagnetic disturbances in geospace for hazard analysis on geomagnetically induced currents]] (2022 - 2026; Xueling Shi, Dogacan Su Ozturk, Mark Engebretson, Zhonghua Xu, E. Joshua Rigler; RA: Primary – GSM, Secondary – MIC)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>*<span style="background:#00ffae"> [[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|(MESO) Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>*<span style="background:#00ffae"> [[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|<ins class="diffchange diffchange-inline"><b></ins>(MESO)<ins class="diffchange diffchange-inline"></b> </ins>Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems|(MPEC) Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems]] (2022 - 2026; Dogacan Su Ozturk, Dong Lin, Yiqun Yu, Katherine Garcia-Sage, Stephen Kaeppler; RA: Primary – MIC, Secondary – GSM)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems|<ins class="diffchange diffchange-inline"><b></ins>(MPEC)<ins class="diffchange diffchange-inline"></b> </ins>Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems]] (2022 - 2026; Dogacan Su Ozturk, Dong Lin, Yiqun Yu, Katherine Garcia-Sage, Stephen Kaeppler; RA: Primary – MIC, Secondary – GSM)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Comparative Planetary Magnetospheric Processes|(COMP) Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Comparative Planetary Magnetospheric Processes|<ins class="diffchange diffchange-inline"><b></ins>(COMP)<ins class="diffchange diffchange-inline"></b> </ins>Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|(KiTS) Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|<ins class="diffchange diffchange-inline"><b></ins>(KiTS)<ins class="diffchange diffchange-inline"></b> </ins>Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Multiscale Dayside Transients and their Effect on Earth's Magnetosphere|(MDT) Multiscale Dayside Transients and their Effect on Earth's Magnetosphere]] (2025 - 2029; Savvas Raptis, Ivan Vasko, Imogen Gingell, Terry Z. Liu, Ying Zou, Runyi Liu, David Tonoian; RA: Primary - SWMI)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* [[FG: Multiscale Dayside Transients and their Effect on Earth's Magnetosphere|<ins class="diffchange diffchange-inline"><b></ins>(MDT)<ins class="diffchange diffchange-inline"></b> </ins>Multiscale Dayside Transients and their Effect on Earth's Magnetosphere]] (2025 - 2029; Savvas Raptis, Ivan Vasko, Imogen Gingell, Terry Z. Liu, Ying Zou, Runyi Liu, David Tonoian; RA: Primary - SWMI)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|(RX) Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Magnetic Reconnection: The Key to Understanding Earth's Space Environment|<ins class="diffchange diffchange-inline"><b></ins>(RX)<ins class="diffchange diffchange-inline"></b> </ins>Magnetic Reconnection: The Key to Understanding Earth's Space Environment]] (2025-2029; Yi Qi, John Dorelli, Katherine Goodrich, Chen Shi, M. Hasan Barbhuiya, Krishna Khanal; RA: Primary - SWMI, Secondary - GSM)</div></td></tr>
<tr><td class='diff-marker'>−</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Radiation Belts as a System of Systems|<b>(RBSoS) </b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td><td class='diff-marker'>+</td><td style="color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>* <span style="background:#00ffae">[[FG: Radiation Belts as a System of Systems|<b>(RBSoS)</b> Radiation Belts as a System of Systems]] (RB-SoS) (2025-2029; Harriet George, Man Hua, Adam Michael, Luisa Capannolo; RA: Primary - IMAG)</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td><td class='diff-marker'> </td><td style="background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>(RA: Research Area).</div></td></tr>
</table>
AllisonJaynes