Difference between revisions of "2019 GEM-CEDAR Joint Workshop and GEM Workshop"
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Location: Lumpkins Ballroom | Location: Lumpkins Ballroom | ||
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| + | This is the final year for Tail Environment FG, we will summary the major findings from this FG. We will discuss how we will proceed to maintain the discussion platform for the magnetotail physics in GEM community, including a proposal for a new FG. | ||
==== [FG] RB ==== | ==== [FG] RB ==== | ||
Location: New Mexico | Location: New Mexico | ||
Revision as of 14:40, 18 June 2019
Detailed Schedule
Below is a detailed session schedule for the 2019 GEM Summer Workshop. The schedule of the Joint GEM-CEDAR Workshop on June 22 can be found in the Google Doc.
In this page, the tentative speakers and titles in Focus Group sessions are provided by Focus Group Leaders, and other information is taken from the Workshop Coordinator Website. Due to the dynamic nature of the Workshop, Focus Groups may continue to revise their session agenda as needed.
Poster Sessions will be held during 17:00 - 20:00 on Tuesday and Thursday. Poster titles can be found in the Poster Information page at the Workshop Coordinator website.
All other information about the 2019 GEM Summer Workshop can be found at the GEM Workshop Coordinator website.
Contents
- 1 Monday, June 24
- 2 Tuesday, June 25
- 3 Wednesday, June 26
- 4 Thursday, June 27
- 5 Friday, June 28
Monday, June 24
0830-1000: Plenary Session
Location: Lumpkins Ballroom
- Welcome/Intro: J. Bortnik, P. Cassak, R. Millan
- RA MIC Tutorial: W. Li
- RAC SWMI Tutorial: K. Goodrich
- NSF REU Program: D. Baker
1030-1200: Splinter Sessions
[FG] IEMIT
Location: Lumpkins Ballroom
- Olga Verkhoglyadova: Summary of CEDAR MIT coupling efforts
- Hyunju Connor: Relation between reconnection and cross polar cap potential during the sudden enhancement of solar wind pressure; SMILE mission for the MIT coupling study.
- Doga Ozturk: What is the role of meso-scale electric fields in M-I-T Coupling?
- Kevin Pham: CMIT model
- Dong Wei: The magnetospheric driving source of double-peak subauroral ion drifts (DSAIDs): Double ring current pressure peak
- Qianli Ma: diffusion coefficients due to chorus waves and electron precipitation features
- Dmytro Sydorenko: Canadian MIT coupling model, EVERYTHING
[FG] MMV
Location: New Mexico
[FG] BSH
Location: Santa Fe
1200 - 1230: LWS Discussion
Location: New Mexico
1330-1500: Splinter Sessions
[FG] IEMIT
Location: Lumpkins Ballroom North
- Christine Garbrielse: Storm Time Mesoscale Plasma Flows in the Nightside High‐Latitude Ionosphere
- Jiang Liu: SWARM & DMSP observations of the eastward plasma flows in the dawnside ionosphere and their comparison with THEMIS ASI observations.
- Ying Zou: effects of substorms in high-latitude upper thermospheric winds
- Sebastijan Mrak : Storm-time MI-coupling at mid-latitudes: Highly structured plasmapause boundary layer
- Brian Anderson: Observed GIC Events in the Pacific Northwest and Corresponding Ionospheric Electrodynamics: Beyond Substorms as the Dominant Cause of GICs
- Denny Oliveira: A historical finding of a sporadic aurora sighting in Rio de Janeiro, Brazil, on 15 Feb 1875
- Colby Lemon: Role of ion precipitation in plasmasphere erosion
[FG] BSH
Location: Lumpkins Ballroom South
[Joint] TAIL/MMV
1. Natalia Ganjushkina, "Magnetotail structure inferred from observations of isotropic boundaries at NOAA satellites and global MHD modeling"
2. Modeling challenge: An event (06-11 UT of 2017-07-09) will be presented and dicussed to understand the global response of the tail, from near-Earth to mid-tail, and the ionosphere to an IMF southward turning, and an IMF northward turning. This is an midnight conjunction of ERG (r < 5), GOES, Geotail (X = -11), MMS (X = -23), and ARTEMIS (X = -63). The observations will be compared with the BATS-R-US, OpenGGCM, and LFM runs conducted on NASA CCMC. The global models will be compared with ionosphere observations/empirical models, including SuperDARN, Ovation Prime, AMPERE, equivalent current, and ground magnetometers.
Tail (Chih-Ping Wang)
SuperDARN (Xueling Shi)
Ovation Prime (Betsey Mitchell)
AMPERE (Brian Anderson)
Equivalent current (James Weygand)
[FG] GBMAB
Location: Santa Fe
1530-1700: Splinter Sessions
[FG] IHMIC
Location: Lumpkins Ballroom North
[FG] RX
Location: Lumpkins Ballroom South
[Joint] UMEA/MMV
Location: New Mexico
Python
Location: Santa Fe
1700-1800: Town Hall - Decadal midterm assessment
Tuesday, June 25
0830-1000: Plenary Session
Location: Lumpkins Ballroom
Agency Talks
- NSF GS: M. Wiltberger
- NSF GEO: L. Winter
- NASA: M. Kessel
- NOAA: H. Singer
- Air Force: J. McCollough
- CSSP: H. Singer, T. Pulkkinen
1030-1200: Splinter Sessions
[Joint] IHMIC/MAPS
Location: Lumpkins Ballroom
[FG] RB
Location: New Mexico
[FG] RX
Location: Santa Fe
1200 - 1230: CCMC Report
Location: New Mexico
1330-1500: Splinter Sessions
[FG] M3-I2
Location: Lumpkins Ballroom North
[FG] RB
Location: Lumpkins Ballroom South
[FG] RX
Location: New Mexico
[Joint] MMS: Turbulence
Location: Santa Fe
1530-1700: Splinter Sessions
[FG] M3-I2
Location: Lumpkins Ballroom North
[Joint] MMV/IEMIT
Location: Lumpkins Ballroom South
- Overview from the CEDAR conductance challenge on the 17 Mar 2013 storm
- Shin Ohtani: Solar zenith angle dependence of the auroral electrojets and its impact on conductance.
- Toshi Nishimura: Ionospheric conductance observations of the 17 March 2013 event
- Doga Ozturk: GTIM empirical results.
- Gang Lu: AMIE results on the 17 Mar 2013 storm
- Bob Robinson: The 17 Mar 2013 storm results from a new empirical ionospheric electrodynamics model
- Hyunju Connor: OpenGGCM results on the 17 Mar 2013 storm
- Kevin Pham: CMIT-IPWM results on the 17 Mar 2013 storm
- Agnit Mukhopadhya: BATSRUS results on the 17 Mar 2013 storm
- Magaret Chen: Magnetosphere-Ionosphere Electron Precipitation Dynamics and Conductance during the 17 March 2013 Storm
See session description at the FG page.
[FG] DIP
Location: New Mexico
[Joint] MMS: Turbulence
Location: Santa Fe
1700-2000: Poster Session
Please visit the Poster Information page for details.
Wednesday, June 26
0830-1000: Plenary Session
Location: Lumpkins Ballroom
- RA GSM Tutorial: J. Burch
- MMV Tutorial: K. Garcia-Sage
1030-1200: Splinter Sessions
[FG] M3-I2
Location: Lumpkins Ballroom
[FG] MAPS
Location: New Mexico
General substorm session
- Kyle Murphy Tracking pre-onset aurora
- Toshi Nishimura Tracking pre-onset aurora
- Bea Gallardo-Lacourt (by Murphy) Tracking pre-onset aurora
- Jiang Liu Ionosphere flows during substorms
- Larry Lyons Substorm precursors and expansion phase activity
- Nithin Sivadas Energetic electron precipitation
[Joint] UMEA/DAYS/IHMIC
Location: Santa Fe
1200 - 1230: URM Event
Location: New Mexico
1330-1500: Splinter Sessions
[FG] M3-I2
Location: Lumpkins Ballroom North
[Joint] DAYS/BSH
Location: Lumpkins Ballroom South
[FG] DIP
Location: New Mexico
1530-1700: Splinter Sessions
[FG] DIP
Location: Lumpkins Ballroom North
[Joint] UMEA/IEMIT
Location: Lumpkins Ballroom South
- (Invited) Boyi Wang: ULF wave challenge event
- (Invited) Xiaojia Zhang / Anton Artemyev: ULF modulation of VLF waves and precipitation
- Doga Ozturk: Update from GEM/CEDAR joint session, PFISR E/ground magnetometer comparisons
- Anatoly Streltsov: Effects of Hall conductivity on generation of ULF waves in magnetosphere-ionosphere interactions
- Mergen Aligabetov: ULF waves observed in space and on the ground at high and low latitudes
- Mark Engebretson: Multi-Instrument Observations of Nighttime Impulsive Magnetic Events
- Bob Lysak: the effect of the ionospheric boundary condition on modeling GICs
- Yan Song: ULF wave, M-I coupling and Auroral formation.
[Joint] MMS: Bowshock
Location: New Mexico
[Joint] MMS: Inner M'sphere
Location: Santa Fe
Thursday, June 27
0830-1000: Plenary Session
Location: Lumpkins Ballroom
- RA MPS Tutorial: A. Runov
- RA IMAG Tutorial: H. Zhao
- Mission/Modeling: M. Gkioulidou, T. Nishimura
1030-1200: Splinter Sessions
[FG] Rx
Location: Lumpkins Ballroom
[Joint] UMEA/RB
Location: New Mexico
SPEDAS
Location: Santa Fe
1330-1500: Splinter Sessions
[Joint] MAPS/DIP
Location: Lumpkins Ballroom North
[Joint] RX/DAYS
Location: Lumpkins Ballroom South
[FG] UMEA
Location: New Mexico
1530-1700: Splinter Sessions
[FG] TAIL
Location: Lumpkins Ballroom North
[FG] UMEA
Location: Lumpkins Ballroom South
[Joint] MMS: SPEDAS
Location: New Mexico
[Joint] DAYS/MMV
Location: Santa Fe
1700-2000: Poster Session
Please visit the Poster Information page for details.
Friday, June 28
0830-1000: Plenary Session
Location: Lumpkins Ballroom
- Students Awards, Student Invited Tutorial: M. Argall
- Mission/Modeling: J. Sample
1030-1200: Splinter Sessions
[FG] TAIL
Location: Lumpkins Ballroom
This is the final year for Tail Environment FG, we will summary the major findings from this FG. We will discuss how we will proceed to maintain the discussion platform for the magnetotail physics in GEM community, including a proposal for a new FG.
[FG] RB
Location: New Mexico
