← LeaderboardsInvestigatorsiAttributed = a PI's even-split share of each grant — a $1M grant with 2 PIs counts $500K each.
Helio Research
La Crescenta, CA
$2,731,303
Total funding
9
Grants
Funding over time
peak $723.3K · FY2005–10$1M$750K$500K$250K$0
'05
'06
'07
'08
'09
'10
Funding mix
By agency
NSF$2,302,971 · 7
NASA$428,332 · 2
By mechanism
—$2,731,303 · 9
Investigators at Helio Research
InvestigatorsiAttributed = a PI's even-split share of each grant — a $1M grant with 2 PIs counts $500K each.
Exposure= the full size of every grant they're on ($1M each).
Rising Stars
First grant in the last 5 yrs
Not enough data
Emerging Leaders
6–10 yrs in
Not enough data
All-Time
Most funded here, all years
Not enough data
Largest grants
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
Collaborative Research: Testing a New Concept for the Long-term Build-up to Coronal Mass Ejections$465,679
· FY2008 · GEO
The Formation, Evolution and Chirality of Filament Channels: A Physical Basis to Elements of Space Weather$442,812
· FY2002 · GEO
Probability Distribution Functions of Field Variations, Non-Gaussianity and Intermittency in the Turbulent Solar Wind$343,690
· FY2010 · GEO
SHINE: How New Active Regions Trigger Erupting Filaments and Associated Coronal Mass Ejections (CMEs)$294,969
· FY2009 · GEO
ANALYSES OF ERUPTING PROMINENCES WITH EMPHASIS ON THEIR HELICITY: WE ARE PROPOSING TO ANALYZE LARGE$275,774
· FY2009 · National Aeronautics and Space Administration
NSWP: Multiscale Study of Magnetic Field-Line and Energetic Particle Dispersal in the Turbulent Solar Wind$152,561
· FY2008 · GEO
FIELD-LINE AND ENERGETIC PARTICLE DISPERSAL IN THE SOLAR WIND:\NTHE MODELING OF INTERPLANETARY ENERG$152,558
· FY2009 · National Aeronautics and Space Administration
RAPID: Acquiring Extensive High Resolution Solar Data for Enhancing Research on the Build-up to Coronal Mass Ejections (CMEs)$124,997
· FY2010 · GEO