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James M Stone

University Of Maryland, College Park

Google Scholar ↗PubMed ↗ORCID ↗

$2,873,609

Attributed

$5,470,477

Total exposure

13

Grants

10

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 $1.3M · FY2006–17

$2M$1.5M$1M$500K$0

'06

'07

'08

'09

'10

'11

'12

'13

'14

'15

'16

'17

Funding mix

By agency

NSF$5,470,477 · 13

By mechanism

—$5,470,477 · 13

Top collaborators

Grant awards (13)

Collaborative Research: Predicting the Observational Signatures of Accreting Black Holes$408,418

· FY2017 · MPS · contact PI

A Max-Planck/Princeton Research Center for Plasma Physics$540,000

· FY2015 · MPS · contact PI

Collaborative Research: Black Hole Accretion Theory and Computation Network$501,276

· FY2013 · MPS · contact PI

MHD Models of Accretion Disks in Close Binaries$311,500

· FY2013 · MPS · contact PI

SAVI: A Max-Planck/Princeton Research Center for Plasma Physics$950,002

· FY2012 · MPS · contact PI

II-New: A Platform for Data-Parallel GPU Computing at Princeton$350,000

· FY2012 · CSE

MRI: Acquisition of a High-Performance Computing Cluster for Astrophysics$663,315

· FY2007 · MPS · contact PI

Laboratory Study of Magnetorotational Instability and Hydrodynamic Stability at Large Reynolds Numbers in a Short Couette Flow$542,598

· FY2006 · MPS

ITR/AP Development of a Next Generation Community Code for Astrophysical Gas Dynamics$181,367

· FY2003 · MPS · contact PI

Computational Studies of MHD Accretion Flows$130,395

· FY2003 · MPS · contact PI

Dynamical Studies of Molecular Cloud Formation in Spiral Galaxies$229,921

· FY2002 · MPS

ITR/AP Development of a Next Generation Community Code for Astrophysical Gas Dynamics$480,823

· FY2001 · MPS · contact PI

Computational Studies of MHD Accretion Flows$180,862

· FY2001 · MPS · contact PI