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Amitava Bhattacharjee
University Of Iowa
$6,061,244
Attributed
$10,719,535
Total exposure
23
Grants
15
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 $3.6M · FY2006–23$5M$3.8M$2.5M$1.3M$0
'06
'07
'08
'09
'10
'11
'12
'13
'14
'15
'16
'17
'18
'19
'20
'21
'22
'23
Funding mix
By agency
NSF$10,719,535 · 23
By mechanism
—$10,719,535 · 23
Top collaborators
- Anatoly Spitkovsky2 shared
- Joachim Raeder2 shared
- Liang Wang2 shared
- Terry G Forbes2 shared
- Ammar H Hakim1 shared
- Chung-Sang Ng1 shared
- Eliot Quataert1 shared
- Eroma Abeysinghe Mudalige1 shared
Grant awards (23)
Collaborative Research: SHINE--Exploring Reconnection-Driven Solar Explosive Events in Different Regimes through Modeling and Observation$542,904
· FY2023 · GEO · contact PI
Collaborative Research: Frameworks: A Software Ecosystem for Plasma Science and Space Weather Applications$2,004,434
· FY2022 · CSE · contact PI
Collaborative Research: WoU-MMA: Multimessenger Plasma Physics Center (MPPC)$986,449
· FY2022 · MPS
WoU-MMA: Role of the Dynamo Effect in Neutron Star Mergers$600,000
· FY2022 · MPS · contact PI
Max-Planck-Princeton Center for Plasma Physics: A Collaboration in Plasma Astrophysics$600,000
· FY2018 · MPS
SHINE: Plasma Instabilities in Post-Eruption Solar Corona, Formation of Plasmoids and Supra-Arcade Downflows$357,000
· FY2015 · GEO
Collaborative Research: Integration of Extended Magnetohydrodynamic (MHD) and Kinetic Effects in Global Magnetosphere Models$612,689
· FY2014 · GEO · contact PI
Collaborative Research: Integration of Extended Magnetohydrodynamic (MHD) and Kinetic Effects in Global Magnetosphere Models$1,280,000
· FY2013 · GEO · contact PI
SHINE: Instability of Large-Scale Current Sheets, Plasmoid Formation, and Particle Acceleration in Coronal Plasmas$157,775
· FY2013 · GEO · contact PI
Structure and Dynamics of the Diffusion Region During Asymmetric Magnetic Reconnection$525,735
· FY2012 · GEO
SHINE: Instability of Large-Scale Current Sheets, Plasmoid Formation, and Particle Acceleration in Coronal Plasmas$379,120
· FY2010 · GEO · contact PI
Advanced Computational Capabilities for Exploration in Heliophysical Science (ACCHS) Workshop; Boulder, Colorado; August 16-18, 2010$10,000
· FY2010 · GEO
Stability of Thin Current Sheet in the Magnetotail: Theory, Simulations, and Observations$360,000
· FY2009 · GEO · contact PI
Collaborative Research: GEM: Plasma Sheet Instabilities prior to THEMIS Substorm Expansion Onsets$130,000
· FY2009 · GEO
GEM: Can Global Magnetohydrodynamics (MHD) Codes Model Magnetic Reconnection in the High Lundquist Number Limit?$300,000
· FY2008 · GEO · contact PI
Collaborative Research: Global Simulations of Substorm Trigger with GGCM: Synergistic Coupling of Magnetic Reconnection and Ballooning-Interchange Instabilities in the Magnetotail$154,853
· FY2006 · GEO · contact PI
Role of Collisionless Reconnection Mechanisms in Solar Flares and Coronal Mass Ejections (CMEs)$374,001
· FY2004 · GEO · contact PI
Stability of Thin Current Sheets in the Earth's Magnetotail: Theory, Simulations, and Observations$329,998
· FY2004 · GEO · contact PI
Modeling of Auroral Kilometric Radiation (AKR) Ordered Fine Structure via Electromagnetic and Electrostatic Ion Cyclotron (EMIC/EIC) Wave Stimulation and Particle Interaction$300,000
· FY2004 · GEO
Acquisition of a Computer Cluster for Geospace Modeling$261,439
· FY2004 · GEO
Three-Dimensional Dynamics of Thin Current Sheets and Their Role in the Triggering and Spatio-Temporal Evolution of Magnetotail Substorms$32,258
· FY2003 · GEO · contact PI
Three-Dimensional Dynamics of Thin Current Sheets and Their Role in the Triggering and Spatio-Temporal Evolution of Magnetotail Substorms$248,000
· FY2001 · GEO · contact PI
Reduced Models for Compressible Turbulence in the High-Lundquist-Number Solar Wind$172,880
· FY2000 · GEO · contact PI