Difference between revisions of "GEM Focus Groups"

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* [[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: 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)
 
* [[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. J. Rigler; RA: Primary – GSM, Secondary – MIC)
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* [[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: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, Emma Spanswick, Yari Collado-Vega, and Bashi Ferdousi; RA: Primary – MPS, Secondary – MIC)
 
* [[FG: Mesoscale drivers of the nightside transition region ionospheric and magnetotail evaluations|Mesoscale drivers of the nightside transition region: ionospheric and magnetotail evaluations]] (2022 - 2026; Bea Gallardo-Lacourt, Gareth Perry, Emma Spanswick, Yari Collado-Vega, and Bashi Ferdousi; 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)
 
* [[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)

Revision as of 15:00, 25 January 2022

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 Group

Past Focus Groups

(RA: Research Area)