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Lawrence R Lyons
Aerospace Corporation
$3,459,752
Attributed
$7,344,237
Total exposure
20
Grants
11
Lead (contact PI)
Attributed= this PI's even-split share of every grant they're on (the fair, additive number). Exposure = full size of all those grants.
Funding over time
peak $1.7M · FY2006–23$2M$1.5M$1M$500K$0
'06
'07
'08
'09
'10
'11
'12
'13
'14
'15
'16
'17
'18
'19
'20
'21
'22
'23
Funding mix
By agency
NSF$7,344,237 · 20
By mechanism
—$7,344,237 · 20
Top collaborators
- Eftyhia Zesta5 shared
- Yukitoshi Nishimura5 shared
- Athanasios Boudouridis2 shared
- Jiang Liu2 shared
- Margaret W Chen2 shared
- Mark B Moldwin2 shared
- Chih-Ping Wang1 shared
- Christine Gabrielse1 shared
Grant awards (20)
GEM: Fundamental Properties of Dawnside Auroral Polarization Streams and Their Role in Magnetosphere-Ionosphere Instabilities and Dramatic Events$523,629
· FY2023 · GEO
Collaborative Research: Flow Channel Control of Substorm Expansion Phase Spatial Coverage and Duration$379,856
· FY2021 · GEO · contact PI
Collaborative Research: Supersubstorms--Their Driving and Responses in the Magnetosphere, Ionosphere, and Thermosphere$185,364
· FY2019 · GEO · contact PI
Collaborative Research: Coordinated Radar and Optical Analysis of Flow Channel Disturbances within the Nightside Auroral Oval/Plasma Sheet$528,674
· FY2015 · GEO · contact PI
Properties of Meso-scale Polar Cap Structures and their Coupling to Nightside Auroral Dynamics$299,629
· FY2015 · GEO
Collaborative Research: PFISR Ion-Neutral Observations in the Thermosphere (PINOT)$138,309
· FY2012 · GEO · contact PI
CEDAR: Incoherent Scatter Radar (ISR) Measurements of Flow Bursts and Relations to Auroral Electrodynamics$450,000
· FY2011 · GEO · contact PI
Development of Large-Scale Electric Fields in the Inner Magnetosphere during Substorms$300,000
· FY2011 · GEO
Collaborative Research: GEM--Asymmetric Entry and Transport of Magnetospheric Plasma During Periods of Northward Interplanetary Magnetic Field$163,336
· FY2010 · GEO · contact PI
NSWP: Formation and Characteristics of the Harang Reversal and Relations to Substorms: Simulations with the Rice Convection Model$535,000
· FY2009 · GEO
Renewal of the South American Meridional B-field Array (SAMBA): An American-Chilean magnetometer chain$807,520
· FY2007 · GEO
Triggered Large-scale Auroral Disturbances and Poleward Boundary Intensifications (PBIs): Polar Lonospheric Convection Evolution and Structure$460,380
· FY2007 · GEO · contact PI
CEDAR: AMISR Measurements of Auroral Disturbance Electrodynamics, Including Relations to Harang Reversal and Large-Scale Convection Evolution$400,000
· FY2007 · GEO · contact PI
Collaborative Research: GEM: Plasma Transport from the Solar Wind to the Inner Magnetosphere$130,001
· FY2006 · GEO · contact PI
High-Resolution 3-D Simulations of the Thermospheric Response to Magnetic Storms, Substorm Surges and the Diffuse Aurora$264,519
· FY2003 · GEO
Spatial and Temporal Dynamics of Important Types of Geomagnetic Disturbance$572,765
· FY2002 · GEO · contact PI
Collaborative Research: Space Weather--Self-Consistent Modeling of Inner Magnetosphere Under Enhanced Convections$360,000
· FY2002 · GEO · contact PI
Collaborative Research: GEM--Stormtime Particle Transport Studies in More Realistic Models of the Inner Magnetosphere$141,000
· FY2002 · GEO
South American Meridional B-Field Array (SAMBA): A Chilean-American Magnetometer Array$524,255
· FY2001 · GEO
GEM: Stormtime Magnetospheric Electric Fields: Data Analysis, Assimilation, and Modeling$180,000
· FY2000 · GEO