Katharine K Reeves

Smithsonian Institution Astrophysical Observatory

$2,588,445

Attributed

$5,585,264

Total exposure

Grants

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 $1.8M · FY2008–24

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

'08

'09

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'11

'12

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'14

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'24

Funding mix

By agency

NSF$5,585,264 · 12

By mechanism

—$5,585,264 · 12

Top collaborators

Grant awards (12)

Collaborative Research: The Role of Supra-arcade Downflows on Energy Transfer in Solar Flares$335,621

· FY2024 · GEO · contact PI

REU Site: Solar Physics at the Center for Astrophysics, Harvard & Smithsonian$599,498

· FY2023 · GEO

REU Site: Solar Physics at the Harvard-Smithsonian Center for Astrophysics$601,042

· FY2019 · GEO · contact PI

Collaborative Research: Plasma Heating and Energy Partition in Flares and Coronal Mass Ejections (CMEs)$352,588

· FY2019 · GEO · contact PI

Collaborative Research: SHINE--Magnetic Energy Release During Solar Eruptions - From Large to Small Scales$215,114

· FY2017 · GEO · contact PI

REU Site: Solar Physics at the Harvard-Smithsonian Center for Astrophysics$430,273

· FY2016 · GEO · contact PI

Collaborative Research: SHINE: Data-constrained Simulations of Coronal Mass Ejection Initiation and Propagation$193,453

· FY2015 · GEO · contact PI

CIF21 DIBBs: Systematic Data-Driven Analysis and Tools for Spatiotemporal Solar Astronomy Data$1,499,933

· FY2014 · CSE

SHINE: Theoretical Investigation of Small Scale Structure in Solar Flare Current Sheets$342,578

· FY2014 · GEO

REU Site: Solar Physics at the Harvard-Smithsonian Center for Astrophysics$275,269

· FY2013 · GEO · contact PI

SHINE: Plasma Heating During Coronal Mass Ejections$463,848

· FY2012 · GEO

SHINE: Connecting Coronal Mass Ejection (CME) Dynamics to Coronal Emissions through Numerical Modeling$276,047

· FY2008 · GEO · contact PI