Difference between revisions of "GEM Focus Groups"

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==Active Focus Groups==
 
==Active Focus Groups==
  
* [[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)
 
* [[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)
 
 
* [[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)
 
* [[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)
 
*[[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).
 
*[[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).
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==Standing Resource Groups==
 
==Standing Resource Groups==
 
* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; Alexa Halford, Josh Rigler, Qusai Al Shidi, Huayue Chen)
 
* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; Alexa Halford, Josh Rigler, Qusai Al Shidi, Huayue Chen)
* <span style="background:#ccff99">[[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor, Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)
+
* [[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor, Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)
  
 
==Past Focus Groups==
 
==Past Focus Groups==
 +
* [[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)
 +
* [[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)
 
* [[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)
 
* [[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)
 
* [[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)
 
* [[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)

Latest revision as of 10:19, 16 July 2025

Introduction

The hallmark of GEM workshops is its community-led workshop-style sessions, carried out through focus groups. Interested in applying to run a focus group and are not sure how to do it? Are you currently running a focus group and need ideas for how to achieve the workshop-style in your focus groups? Advice from previous focus group leaders on proposing and running a focus group, updated in October 2019, is available here.

Active Focus Groups

(RA: Research Area).

Standing Resource Groups

Past Focus Groups

(RA: Research Area)