Difference between revisions of "2022 GEM Workshop"

From gem
Jump to navigation Jump to search
 
(24 intermediate revisions by 3 users not shown)
Line 9: Line 9:
 
== Sunday, June 19 ==
 
== Sunday, June 19 ==
  
−
=== Student Day ===
+
=== 0800-1530 HST: Student Day ===
 +
The Student Day is organized by the Student Representatives and aims to introduce the students to the GEM workshop. You may find more information at the [[GEM Student Forum|GEM Student Forum]] page.
  
−
Student Day is on June 19th (Sunday), 2022, and aims to introduce the students to the GEM workshop. You may find more information at the [[GEM Student Forum|GEM Student Forum]] page.
+
===  1800-1930 HST: Workshop Icebreaker ===
  
 
== Monday, June 20 ==
 
== Monday, June 20 ==
 
=== 0800-1000 HST: Plenary Session ===
 
=== 0800-1000 HST: Plenary Session ===
 
* '''Opening Remarks''' - Vania Jordanova
 
* '''Opening Remarks''' - Vania Jordanova
−
* '''GSM Tutorial''' - John Dorelli
+
* '''GSM Tutorial''' - John Dorelli: ''From Speiser Orbits to Substorms: What is the Path to a Multiscale GGCM?''
 
* '''IMAG Tutorial''' - Michael Liemohn: ''Hidden Gems of Inner Magnetospheric Research''
 
* '''IMAG Tutorial''' - Michael Liemohn: ''Hidden Gems of Inner Magnetospheric Research''
  
Line 35: Line 36:
 
== Tuesday, June 21 ==
 
== Tuesday, June 21 ==
 
=== 0800-1000 HST: Agency Talks ===
 
=== 0800-1000 HST: Agency Talks ===
−
* '''NSF''' - Lisa Winter, Chia-Lin Huang '' ''
+
* '''NSF''' - Chia-Lin Huang & Lisa Winter: ''GEM Update from the National Science Foundation''
−
* '''NASA''' - Patrick Koehn '' ''
+
* '''NASA''' - Patrick Koehn: ''Heliophysics Division Update''
 
* '''NOAA''' - Howard Singer: ''NOAA Liaison Report: Highlights of Activities''
 
* '''NOAA''' - Howard Singer: ''NOAA Liaison Report: Highlights of Activities''
−
* '''AFRL''' - Shawn Young '' ''
+
* '''AFRL''' - Shawn Young ''Highlights from AFRL work in Geospace''
  
 
=== 1030-1200 HST: Concurrent Session 1 ===
 
=== 1030-1200 HST: Concurrent Session 1 ===
 
* MPEC - 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
−
* DIP - Magnetotail Dipolarization and Its Effects on the Inner Magnetosphere
+
* [https://gem.epss.ucla.edu/mediawiki/index.php/FG:_Magnetotail_Dipolarization_and_Its_Effects_on_the_Inner_Magnetosphere DIP - Magnetotail Dipolarization and Its Effects on the Inner Magnetosphere]
 
* RB - System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling
 
* RB - System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling
−
 
−
====DIP - Magnetotail Dipolarization and Its Effects on the Inner Magnetosphere====
 
−
Models have shown that BBFs/DFBs/Mesoscale Injections are important for both ring current and radiation belt build-up, but it remains difficult to verify with observations and therefore the exact role remains an open question. Model results are inconclusive because existing models do not describe all the relevant domains (e.g., magnetotail, transition region, inner magnetosphere) self-consistently while capturing the required range of spatiotemporal scales. We therefore ask, How is plasma and electromagnetic energy transported through the plasma sheet to the inner magnetosphere at different spatiotemporal scales?
 
−
 
−
In this session, we will discuss the perennial question, '''What is the role of reconnection and/or other plasma instabilities in producing elementary magnetotail dipolarizations? How do the physical properties of the dipolarizations depend on their spatial location and the time of their appearance relative to the Dungey cycle?'''
 
−
 
−
'''Speakers'''
 
−
* Toshi Nishimura (work presented by Christine Gabrielse): Kinetic Plasma Structures Associated with Substorm Auroral Beads by Space-Ground Coordinated Observations
 
−
* Shin Ohtani (work presented by Jesper Gjerloev): New Insights into the Substorm Initiation Sequence from the Spatio-temporal Development of Auroral Electrojets
 
−
 
−
Upload Talks here: [https://vgem.org/groups/DIP https://vgem.org/groups/DIP]
 
  
 
=== 1200-1330 HST: Student Rep Candidate Presentations ===
 
=== 1200-1330 HST: Student Rep Candidate Presentations ===
  
 
=== 1330-1500 HST: Concurrent Session 2 ===
 
=== 1330-1500 HST: Concurrent Session 2 ===
−
* GIC - Understanding the causes of geomagnetic disturbances in geospce for hazard analysis on geomagnetically induced currents slack link
+
* GIC - Understanding the causes of geomagnetic disturbances in geospce for hazard analysis on geomagnetically induced currents
−
* DIP - Magnetotail Dipolarization and Its Effects on the Inner Magnetosphere
+
* MESO - Mesoscale drivers of the nightside transition region: Ionospheric and magnetotail evaluations
 
* RB - System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling
 
* RB - System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling
  
Line 71: Line 61:
 
== Wednesday, June 22 ==
 
== Wednesday, June 22 ==
 
=== 0800-1000 HST: Plenary Session ===
 
=== 0800-1000 HST: Plenary Session ===
−
* '''MIC Tutorial''' - Kevin Pham
+
* '''MIC Tutorial''' - Kevin Pham: ''Impact of Thermosphere Dynamics on MI Coupling''
−
* '''SBCCI-DEI Tutorial''' - Caroline Blanco, David Boboltz, Claire Raftery
+
* '''SBCCI-DEI Plenary''' -  
 +
        ‣ David Boboltz and Caroline Blanco: ''NSF Community Engagement in Hawaii''
 +
 
 +
        ‣ Claire Raftery: ''Outreach Strategies for the Daniel K. Inouye Solar Telescope''
  
 
=== 1030-1200 HST: Concurrent Session 1 ===
 
=== 1030-1200 HST: Concurrent Session 1 ===
Line 95: Line 88:
 
== Thursday, June 23 ==
 
== Thursday, June 23 ==
 
=== 0800-1000 HST: Plenary Session ===
 
=== 0800-1000 HST: Plenary Session ===
−
* '''SWMI Tutorial''' - Joe Borovsky
+
* '''SWMI Tutorial''' - Joe Borovsky: ''Solar-Wind/Magnetosphere Coupling: The Basics?''
−
* '''MPS Tutorial''' - Katariina Nykyri
+
* '''MPS Tutorial''' - Katariina Nykyri: ''Influence of the Kelvin-Helmholtz Instability on the Plasma Entry, Transport and Energization at the Magnetospheric Boundary Layers''
  
 
=== 1030-1200 HST: Concurrent Session 1 ===
 
=== 1030-1200 HST: Concurrent Session 1 ===
 
* Joint Session IHMIC/CEDAR
 
* Joint Session IHMIC/CEDAR
−
* DIP - Magnetotail Dipolarization and Its Effects on the Inner Magnetosphere
+
* [https://gem.epss.ucla.edu/mediawiki/index.php/FG:_Magnetotail_Dipolarization_and_Its_Effects_on_the_Inner_Magnetosphere DIP - Magnetotail Dipolarization and Its Effects on the Inner Magnetosphere]
 
* Machine Learning as it pertains in the Geospace Environment
 
* Machine Learning as it pertains in the Geospace Environment
−
 
−
 
−
====DIP - Magnetotail Dipolarization and Its Effects on the Inner Magnetosphere====
 
−
Models have shown that BBFs/DFBs/Mesoscale Injections are important for both ring current and radiation belt build-up, but it remains difficult to verify with observations and therefore the exact role remains an open question. Model results are inconclusive because existing models do not describe all the relevant domains (e.g., magnetotail, transition region, inner magnetosphere) self-consistently while capturing the required range of spatiotemporal scales. We therefore ask, '''How is plasma and electromagnetic energy transported through the plasma sheet to the inner magnetosphere at different spatiotemporal scales?'''
 
−
 
−
Especially given the upcoming Decadal Survey, we want to use a designated session to discuss the following:
 
−
* What do we currently know from models?
 
−
* What are the limitations of the current models?
 
−
* What modeling advances are required and feasible to resolve these limitations in the near- and long-term future (e.g., 5-10 years vs 10-30 years)?
 
−
* What do we currently know from observations?
 
−
* What can we still learn from existing observations and what are their limitations that inhibit further progress?
 
−
* What new observations are required and feasible to resolve these limitations in the near- and long-term future?
 
−
 
−
'''Discussion Leaders/Speakers (Contact the DIP FG leaders if you want to participate as well!)'''
 
−
*Andrei Runov
 
−
*Trunali Anil Shah
 
−
*Soboh Alqeeq
 
−
*Slava Merkin
 
−
 
−
Upload slides here: [https://vgem.org/groups/DIP https://vgem.org/groups/DIP]
 
  
 
=== 1330-1500 HST: Concurrent Session 2 ===
 
=== 1330-1500 HST: Concurrent Session 2 ===
Line 146: Line 119:
 
* BSH - Particle Heating and Thermalization in Collisionless Shocks in the MMS Era
 
* BSH - Particle Heating and Thermalization in Collisionless Shocks in the MMS Era
 
* Joint Session IHMIC/GIC
 
* Joint Session IHMIC/GIC
−
* Joint Session MESO/DIP
+
* [https://gem.epss.ucla.edu/mediawiki/index.php/FG:_Magnetotail_Dipolarization_and_Its_Effects_on_the_Inner_Magnetosphere Joint Session MESO/DIP]
−
 
 
−
====MESO/DIP Joint Session====
 
−
For the duration of the DIP FG, we have discussed the roles that mesoscale phenomena (e.g. DFBs, BBFs, injections, streamers) play with respect to the global system response (e.g. global dipolarization, MLT wide injections). As our FG winds down, the MESO FG will take the lead on this topic. We therefore are hosting a joint session to address these topics.
 
−
 
 
−
'''Discussion Leaders/Speakers'''
 
−
*Yangyang Shen: Contribution of kinetic Alfvén waves to energetic electron scattering and precipitation from plasma sheet injections
 
−
*James Weygand: ASI and GOES Observations of Nighttime Magnetic Perturbation Events Observed in Canada
 
−
 
 
−
Upload Talks here: [https://vgem.org/groups/DIP https://vgem.org/groups/DIP]
 
  
 
=== 1330-1500 HST: Concurrent Session 2 ===
 
=== 1330-1500 HST: Concurrent Session 2 ===
Line 169: Line 133:
  
 
== Saturday, June 25 ==
 
== Saturday, June 25 ==
−
=== 0830-1200 HST: GEM-SHINE ===
+
=== 0830-1200 HST: [https://helioshine.org/joint-gem-shine-schedule/ GEM-SHINE Day 1] ===
−
* '''08:30''' - Tracking SEPs from the Sun to the near-Earth Space
+
* '''08:30''' - ''Tracking SEPs from the Sun to the near-Earth Space'', Moderator: Yihua Zheng
−
* '''10:00''' - Break
+
* '''Part I: Short Talks'''
−
* '''10:30''' - Shocks
+
** Gang Li: Solar Energetic Particles at the interface of GEM-SHINE
 +
** Katie Whitman: ISEP project and SEP model validation efforts
 +
** Rachael Filwett: Energetic Particle Transport near and into Earth’s Magnetosphere
 +
** Valeriy Tenishev: Modeling SEPs in the magnetosphere
 +
* '''Part II: Discussions and possible collaboration'''
 +
 
 +
* '''10:00''' - Coffee break
 +
* '''10:30''' - ''Shocks'', Moderator: Lynn Wilson III
  
 
=== 1830-2000 HST: GEM-SHINE Student Joint Event ===
 
=== 1830-2000 HST: GEM-SHINE Student Joint Event ===
  
 
== Sunday, June 26 ==
 
== Sunday, June 26 ==
−
=== 0830-1200 HST: GEM-SHINE ===
+
=== 0830-1200 HST: [https://helioshine.org/joint-gem-shine-schedule/ GEM-SHINE Day 2] ===
−
* '''08:30''' - How does the solar-wind/magnetosphere coupling change in different types of solar wind?
+
* '''08:30''' - ''How does the solar-wind/magnetosphere coupling change in different types of solar wind?'', Moderators: Nicki Vialli & Sarah Vines
−
* '''10:00''' - Break
+
* '''10:00''' - Coffee break
−
* '''10:30''' - Structured magnetotail BBFs and structured coronal supra-arcade downflows
+
* '''10:30''' - ''Structured magnetotail BBFs and structured coronal supra-arcade downflows'', Moderator: Joe Borovsky

Latest revision as of 09:09, 24 June 2022

Schedule

Below is a high-level session schedule for the 2022 GEM Summer Workshop, provided by the Focus Group Leaders and Research Area Coordinators. For the most up to date workshop information, please refer to the GEM Workshop Website.

Please also refer to the GEM Focus Groups, Modeling Methods Methods and Validation Resource Group, and Machine Learning in Geospace pages for more information.

Sunday, June 19

0800-1530 HST: Student Day

The Student Day is organized by the Student Representatives and aims to introduce the students to the GEM workshop. You may find more information at the GEM Student Forum page.

1800-1930 HST: Workshop Icebreaker

Monday, June 20

0800-1000 HST: Plenary Session

  • Opening Remarks - Vania Jordanova
  • GSM Tutorial - John Dorelli: From Speiser Orbits to Substorms: What is the Path to a Multiscale GGCM?
  • IMAG Tutorial - Michael Liemohn: Hidden Gems of Inner Magnetospheric Research

1030-1200 HST: Concurrent Session 1

  • SCIMM - Self-Consistent Inner Magnetospheric Modeling
  • Joint Session IEMIT/CEDAR
  • Joint Session GIC/GBMA

1330-1500 HST: Concurrent Session 2

  • SCIMM - Self-Consistent Inner Magnetospheric Modeling
  • MPEC - Magnetospheric sources of particle precipitation and their role on electrodynamic coupling of magnetosphere-ionosphere-thermosphere systems
  • Joint Session MESO/CEDAR

1530-1700 HST: SBCCI - Speaking Up (Bystander intervention training)

1800-2030 HST: Student Dinner

Tuesday, June 21

0800-1000 HST: Agency Talks

  • NSF - Chia-Lin Huang & Lisa Winter: GEM Update from the National Science Foundation
  • NASA - Patrick Koehn: Heliophysics Division Update
  • NOAA - Howard Singer: NOAA Liaison Report: Highlights of Activities
  • AFRL - Shawn Young Highlights from AFRL work in Geospace

1030-1200 HST: Concurrent Session 1

1200-1330 HST: Student Rep Candidate Presentations

1330-1500 HST: Concurrent Session 2

  • GIC - Understanding the causes of geomagnetic disturbances in geospce for hazard analysis on geomagnetically induced currents
  • MESO - Mesoscale drivers of the nightside transition region: Ionospheric and magnetotail evaluations
  • RB - System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling

1530-1700 HST: Concurrent Session 3

  • GIC - Understanding the causes of geomagnetic disturbances in geospce for hazard analysis on geomagnetically induced currents slack link
  • RB - System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling

1800-2030 HST: Poster Session

Wednesday, June 22

0800-1000 HST: Plenary Session

  • MIC Tutorial - Kevin Pham: Impact of Thermosphere Dynamics on MI Coupling
  • SBCCI-DEI Plenary -

        ‣ David Boboltz and Caroline Blanco: NSF Community Engagement in Hawaii

        ‣ Claire Raftery: Outreach Strategies for the Daniel K. Inouye Solar Telescope

1030-1200 HST: Concurrent Session 1

  • RB - System Understanding of Radiation Belt Particle Dynamics through Multi-spacecraft and Ground-based Observations and Modeling
  • IEMIT - 3D Ionospheric Electrodynamics and its Impact on MIT Coupling
  • MMV - Modeling Methods and Validation

1200-1330 HST: GEMEE Lunch

1330-1500 HST: Concurrent Session 2

  • Joint Session SCIMM/MPEC
  • RX - Magnetic Reconnection in the Age of the Heliophysics System Observatory
  • MMV - Modeling Methods and Validation

1530-1700 HST: Concurrent Session 3

  • Joint Session RB/CP/SCIMM/MPEC
  • RX - Magnetic Reconnection in the Age of the Heliophysics System Observatory
  • MMV - Modeling Methods and Validation

1800-2030 HST: Banquet

Thursday, June 23

0800-1000 HST: Plenary Session

  • SWMI Tutorial - Joe Borovsky: Solar-Wind/Magnetosphere Coupling: The Basics?
  • MPS Tutorial - Katariina Nykyri: Influence of the Kelvin-Helmholtz Instability on the Plasma Entry, Transport and Energization at the Magnetospheric Boundary Layers

1030-1200 HST: Concurrent Session 1

1330-1500 HST: Concurrent Session 2

  • Joint Session MPEC/IEMIT
  • CP - The Impact of the Cold Plasma in the Magnetospheric Physics
  • Machine Learning as it pertains in the Geospace Environment

1530-1700 HST: Concurrent Session 3

  • Joint Session IHMIC/IEMIT
  • RX - Magnetic Reconnection in the Age of the Heliophysics System Observatory
  • CP - The Impact of the Cold Plasma in the Magnetospheric Physics

1800-2030 HST: Poster Session

Late: SBCCI - Queer Beers

Friday, June 24

0800-1000 HST: Plenary Session

  • Student Tutorial - Robert Allen: Heliophysics missions and instrumentation: Past progress towards future implementations
  • MMV Tutorial - KD Leka: Here, There, or Everywhere? Validation and Evaluation in Solar and Heliospheric (SHINE) Science
  • Closing Remarks - Vania Jordanova

1030-1200 HST: Concurrent Session 1

  • BSH - Particle Heating and Thermalization in Collisionless Shocks in the MMS Era
  • Joint Session IHMIC/GIC
  • Joint Session MESO/DIP

1330-1500 HST: Concurrent Session 2

  • BSH - Particle Heating and Thermalization in Collisionless Shocks in the MMS Era
  • Joint Session GIC/IEMIT
  • Machine Learning as it pertains in the Geospace Environment

1500 HST: SBCCI - Social/Sam Bingham memorial

1630 HST: GEM SC meeting

1700 HST: HON magnetic observatory

Saturday, June 25

0830-1200 HST: GEM-SHINE Day 1

  • 08:30 - Tracking SEPs from the Sun to the near-Earth Space, Moderator: Yihua Zheng
  • Part I: Short Talks
    • Gang Li: Solar Energetic Particles at the interface of GEM-SHINE
    • Katie Whitman: ISEP project and SEP model validation efforts
    • Rachael Filwett: Energetic Particle Transport near and into Earth’s Magnetosphere
    • Valeriy Tenishev: Modeling SEPs in the magnetosphere
  • Part II: Discussions and possible collaboration
  • 10:00 - Coffee break
  • 10:30 - Shocks, Moderator: Lynn Wilson III

1830-2000 HST: GEM-SHINE Student Joint Event

Sunday, June 26

0830-1200 HST: GEM-SHINE Day 2

  • 08:30 - How does the solar-wind/magnetosphere coupling change in different types of solar wind?, Moderators: Nicki Vialli & Sarah Vines
  • 10:00 - Coffee break
  • 10:30 - Structured magnetotail BBFs and structured coronal supra-arcade downflows, Moderator: Joe Borovsky
Retrieved from "https://gem.epss.ucla.edu/mediawiki/index.php?title=2022_GEM_Workshop&oldid=5929"