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Alexandre Lazarian
University Of Wisconsin-Madison
$2,429,763
Attributed
$2,995,810
Total exposure
12
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 $420.1K · FY2005–23$500K$375K$250K$125K$0
'05
'06
'07
'08
'09
'10
'11
'12
'13
'14
'15
'16
'17
'18
'19
'20
'21
'22
'23
Funding mix
By agency
NSF$2,995,810 · 12
By mechanism
—$2,995,810 · 12
Top collaborators
- Barbara A Whitney1 shared
- Fabian Heitsch1 shared
- Joseph P Cassinelli1 shared
- Kenneth H Nordsieck1 shared
- Michael J Wolff1 shared
- Richard Ignace1 shared
Grant awards (12)
Exploring magnetic fields on the largest scales$420,110
· FY2023 · MPS · contact PI
Collaborative Research: Studying Magnetic Fields in the Interstellar Medium$410,223
· FY2018 · MPS · contact PI
Collaborative Research: Using Observations and Models to Study How Dust Grains Between the Stars Align$311,424
· FY2017 · MPS · contact PI
Collaborative Research: Simulating Two-Fluid MHD Turbulence in Star Forming Molecular Clouds on the Blue Waters System$20,000
· FY2017 · CSE · contact PI
Quantitative insight into interstellar turbulence$299,890
· FY2012 · MPS · contact PI
Collaborative Research: Observational testing of interstellar grain alignment theory$145,332
· FY2011 · MPS · contact PI
Towards Understanding Interstellar Turbulence$280,448
· FY2008 · MPS · contact PI
Collaborative Research: SHINE--Stochastic Particle Acceleration by Turbulence in Solar Flares$139,647
· FY2007 · GEO · contact PI
Radiation Transfer in Aligned Grains: Probing Magnetic Fields in Molecular Clouds, Protostars, and Disks$354,707
· FY2005 · MPS
Fundamentals and Implications of Interstellar Turbulence$154,008
· FY2003 · MPS · contact PI
Circumstellar Magnetic Field Diagnostics from the Polarization of Line Scattering$400,022
· FY2001 · MPS
Collaborative Research: Fast Dynamos in the Computer, the Galaxy, and the Laboratory$59,999
· FY2001 · MPS · contact PI