Difference between revisions of "GEM Focus Groups"

From gem
Jump to navigation Jump to search
Line 9: Line 9:
 
* [[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. 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="background:green"> [[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).
+
*<span style="background:lime"> [[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)
 
* [[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)
 
* [[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)

Revision as of 11:59, 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)

Standing Resource Groups

Past Focus Groups

(RA: Research Area)