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Terry G Forbes
University Of New Hampshire
$2,184,177
Attributed
$7,204,489
Total exposure
9
Grants
4
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 $5M · FY2005–11$5M$3.8M$2.5M$1.3M$0
'05
'06
'07
'08
'09
'10
'11
Funding mix
By agency
NSF$7,204,489 · 9
By mechanism
—$7,204,489 · 9
Top collaborators
- Amitava Bhattacharjee2 shared
- Yuri E Litvinenko2 shared
- Alexei A Pevtsov1 shared
- Harlan Spence1 shared
- Jack E Dibb1 shared
- Katharine K Reeves1 shared
- Nathan A Schwadron1 shared
- Ruth K Varner1 shared
Grant awards (9)
FESD Type 1: Sun to Ice--Impacts on Earth of Extreme Solar Events$5,000,000
· FY2011 · GEO
SHINE: Instability of Large-Scale Current Sheets, Plasmoid Formation, and Particle Acceleration in Coronal Plasmas$379,120
· FY2010 · GEO
SHINE: Connecting Coronal Mass Ejection (CME) Dynamics to Coronal Emissions through Numerical Modeling$276,047
· FY2008 · GEO
Collaborative Research: Testing a New Concept for the Long-term Build-up to Coronal Mass Ejections$64,772
· FY2008 · GEO · contact PI
Viscous Effects in Magnetic Reconnection and Energy Dissipation in the Solar Corona$294,061
· FY2007 · GEO · contact PI
NSWP: Collaborative Analyses of the Formation, Activation and Long-term Slow Rise of Filaments as Precursors to Coronal Mass Ejections (CMEs)$478,263
· FY2005 · GEO
Role of Collisionless Reconnection Mechanisms in Solar Flares and Coronal Mass Ejections (CMEs)$374,001
· FY2004 · GEO
SHINE: Linking Flare Radiation to the Dynamics of Coronal Mass Ejections$297,928
· FY2003 · GEO · contact PI
U.S.-Japan Cooperative Science: Solar Explosive Phenomena with YOHKOH/SOHO/TRACE/Solar-B$40,297
· FY2000 · O/D · contact PI