← LeaderboardsInvestigatorsiAttributed = a PI's even-split share of each grant — a $1M grant with 2 PIs counts $500K each.
Ashima
$3,215,339
Total funding
11
Grants
Funding over time
peak $1.4M · FY2009–14$2M$1.5M$1M$500K$0
'09
'10
'11
'12
'13
'14
Funding mix
By agency
NASA$3,215,339 · 11
By mechanism
—$3,215,339 · 11
Investigators at Ashima
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
THE MARTIAN WATER CYCLETHE OBJECTIVE OF THIS PROPOSAL IS TO DEVELOP AN IMPROVED UNDERSTANDING OF HOW THE MARTIAN WATER CYCLE WORKS. WE PROPOSE TO DO$620,829
· FY2010 · National Aeronautics and Space Administration
PLANETARY ATMOSPHERIC DATA ASSIMILAITION SYSTEM WE PROPOSE TO DEVELOP A PLANETARY ATMOSPHERIC DATA ASSIMILATION SYSTEM FOR THE GLOBAL EXTRAPOLATION O$495,009
· FY2009 · National Aeronautics and Space Administration
THE KEY OBJECTIVES OF THIS PROPOSAL ARE TO GAIN A BETTER UNDERSTANDING OF THE CIRCULATION OF TITAN'S ATMOSPHERE - ESPECIALLY THE SUPER ROTATION OF TH$372,090
· FY2011 · National Aeronautics and Space Administration
MISMATCHES BETWEEN THE OBSERVED DUST AND WATER CYCLES AND THOSE SIMULATED BY GENERAL CIRCULATION MODELS (GCMS) ARE TYPICALLY ASSUMED TO BE DUE TO ERR$324,778
· FY2014 · National Aeronautics and Space Administration
THE OBSERVED THERMAL STRUCTURE WITHOUT AD HOC PRESCRIPTION. SINCE THE FORCING AND RESPONSE OF THE MARTIAN ATMOSPHERE ARE BOTH FAST COMPARED TO A DIUR$281,130
· FY2014 · National Aeronautics and Space Administration
THE OVERALL GOAL OF THIS PROJECT IS TO IMPROVE OUR UNDERSTANDING OF THE RELATIONSHIP BETWEEN DUNES AND WINDS AT THE SURFACE OF MARS. WE WILL USE THEO$278,039
· FY2014 · National Aeronautics and Space Administration
UNDERSTANDING TITAN'S ATMOSPHERIC CIRCULATION AND METHANE CYCLE USING A GENERAL CIRCULATION MODEL THE GOAL OF THIS PROPOSAL IS TO INVESTIGATE THE PRO$189,069
· FY2014 · National Aeronautics and Space Administration
CONSTRAINING MOIST CONVECTION IN GAS GIANT ATMOSPHERES USING OBSERVATIONS AND MODELING OF THE 2010 GREAT WHITE SPOT ON SATURN. MOIST CONVECTION IS LI$180,402
· FY2014 · National Aeronautics and Space Administration
THE PURPOSE OF THIS PROPOSAL IS TO INVESTIGATE TITAN'S GENERAL CIRCULATION AND LARGE-SCALE METHANE CYCLE THROUGH ANALYSIS OF OBSERVATIONS USING A TIT$177,993
· FY2010 · National Aeronautics and Space Administration
EQUATORIAL MESOSCALE WAVES AND ROSSBY WAVES IN THE JOVIAN ATMOSPHERE GENERATION AND MAINTENANCE OF MESOSCALE WAVES AND ROSSBY WAVES CAN CONSTRAIN TH$165,000
· FY2010 · National Aeronautics and Space Administration
GENERAL CIRCULATION MODELS (GCMS) OF THE VENUS ATMOSPHERE USE RELATIVELY SIMPLE PHYSICAL MODELS TO PRODUCE A SUPER-ROTATING ATMOSPHERIC CIRCULATION T$131,000
· FY2014 · National Aeronautics and Space Administration