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|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)
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* <span style="background:#00ffae">[[FG: The Impact of the Cold Plasma in Magnetospheric Physics|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|Self-Consistent Inner Magnetospheric Modeling]] (2020 - 2025; Cristian Ferradas, Chao Yue, Jacob Bortnik, and Qianli Ma; RA: Primary – IMAG, Secondary – MIC)
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* <span style="background:#00ffae">[[FG: Self-Consistent Inner Magnetospheric Modeling|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|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|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)
* <span style="color:#009999">[[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations (MESO)]]</span> (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).
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*<span style="background:#00ffae"> [[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations (MESO)]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, and Emma Spanswick; RA: Primary – MPS, Secondary – MIC).
* [[FG: Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems|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)
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* <span style="background:#00ffae">[[FG: Magnetospheric Sources of Particle Precipitation and Their Role on Electrodynamic Coupling of Magnetosphere-Ionosphere-Thermosphere Systems|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)
* [[FG: Comparative Planetary Magnetospheric Processes|Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)
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* <span style="background:#00ffae">[[FG: Comparative Planetary Magnetospheric Processes|Comparative Planetary Magnetospheric Processes]] (2023 - 2027; George Clark, Wen Li, Bob Marshall, Dan Gershman, Peter Delamere, Shannon Curry; RA: Primary – SWMI, Secondary – MPS)
 
* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics (KiTS)]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)
 
* [[FG: Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics|Kinetic Plasma Processes in the Magnetotail during Substorm Dynamics (KiTS)]] (2024 - 2028; Harry Arnold, Jason Derr, Akhtar Ardakani, Anton Artemyev; RA: Primary – MPS, Secondary – GSM)
  
  
(RA: Research Area)
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(RA: Research Area).
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Note: FGs and resource groups <span style="background:#00ffae">highlighted in green</span> have expressed interest in collaborating with CEDAR for the 2025 GEM-CEDAR Joint Meeting.
  
 
==Standing Resource Groups==
 
==Standing Resource Groups==
 
* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; Mike Liemohn, Lutz Rastaetter, Alexa Halford and Josh Rigler)
 
* [[RG: Modeling Methods and Validation|Modeling Methods and Validation]] (2020 - present; Mike Liemohn, Lutz Rastaetter, Alexa Halford and Josh Rigler)
* [[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor. Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)
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* <span style="background:#00ffae">[[RG: Machine Learning|Machine Learning]] (2024 - present; Hyunju Connor. Bashi Ferdousi, Xiangning Chu, Matthew Argall, Valluri Sai Gowtam)
  
 
==Past Focus Groups==
 
==Past Focus Groups==

Latest revision as of 13:04, 10 September 2024

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).

Note: FGs and resource groups highlighted in green have expressed interest in collaborating with CEDAR for the 2025 GEM-CEDAR Joint Meeting.

Standing Resource Groups

Past Focus Groups

(RA: Research Area)