← Leaderboards
Katharine K Reeves
Smithsonian Institution Astrophysical Observatory
$2,588,445
Attributed
$5,585,264
Total exposure
12
Grants
8
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
'10
'11
'12
'13
'14
'15
'16
'17
'18
'19
'20
'21
'22
'23
'24
Funding mix
By agency
NSF$5,585,264 · 12
By mechanism
—$5,585,264 · 12
Top collaborators
- Henry D Winter3 shared
- John C Raymond3 shared
- Chengcai Shen2 shared
- Nicholas A Murphy2 shared
- Chad A Madsen1 shared
- Edward E Deluca1 shared
- Petrus C Martens1 shared
- Rafal A Angryk1 shared
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