← LeaderboardsInvestigatorsiAttributed = a PI's even-split share of each grant — a $1M grant with 2 PIs counts $500K each.
University Of Pacific
$2,069,632
Total funding
8
Grants
Funding over time
peak $1M · FY2009–23$2M$1.5M$1M$500K$0
'09
'10
'11
'12
'13
'14
'15
'16
'17
'18
'19
'20
'21
'22
'23
Funding mix
By agency
DOE$1,635,612 · 3
DOD$342,279 · 3
NASA$91,741 · 2
By mechanism
—$2,069,632 · 8
Investigators at University Of Pacific
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
TAS::89 0321::TAS RESEARCH AND DEVELOPMENT OF A NEW SILICA-ALUMINA BASED CEMENTITIOUS MATERIAL LARGELY USING COAL REFUSE FOR MINE BACKFILL, MINE S$1,046,250
· FY2010 · Department of Energy
STATISTICAL ANALYSIS OF INDIVIDUAL PARTICLE MIXING STATE AND MORPHOLOGY$328,249
· FY2015 · Department of Energy
RELATING THE CHEMICAL & PHYSICAL PROPERTIES OF AEROSOLS TO THE WATER UPTAKE & ICE NUCLEATION POTENTIAL OF PARTICLES COLLECTED DURING THE CARBONACEOUS$261,113
· FY2012 · Department of Energy
MOLECULAR INDICATORS OF PHYSIOLOGICAL STRESS AND ITS HEALTH EFFECTS IN CETACEANS$191,329
· FY2023 · Department of the Navy
FIBER REINFORCED POLYMER COMPOSITES FOR INFRASTRUCTURE APPLICATIONS, FOCUSING ON INNOVATION AND TECHNOLOGY IMPLEMENTATION$95,000
· FY2009 · Department of the Army
QUANTITATIVE GENE EXPRESSION SYSTEM FOR STATE-OF-THE-ART BIOMARKER RESEARCH AND DEVELOPMENT AT AN UNDERGRADUATE INSTITUTION$55,950
· FY2018 · Department of the Navy
THE DISCOVERY OF COMPACT SYSTEMS OF MULTIPLE LOW-MASS LOW-DENSITY PLANETS WITHIN A FRACTION OF 1AU HAS TRIGGERED A WELLSPRING OF PLANET FORMATION THEORIES. SOME OF THESE OFFER TESTABLE PREDICTIONS OF OUTER PLANETARY SYSTEM ARCHIECTURES INCLUDING WHETHER GIANT PLANETS ARE EXPECTED AT DISTANCES BEYOND 1AU. OBERVATIONALLY THE OCCURRENCE RATE OF JOVIAN MASS PLANETS IN SYSTEMS WITH MULTIPLE MINI-NEPTUNES WITHIN A FRACTION OF 1AU IS UNKNOWN. HENCE CONSTRAINTS ON THE OCCURRENCE RATE OF JOVIANS IN SYSTEMS OF MULTIPLE LOW-MASS CLOSE-IN NEPTUNES IS OF GREAT INTEREST IN PLANET FORMATION THEORY. WE PROPOSE TO RUN DYNAMICAL SIMULATIONS OF COMPACT SYSTEMS OF MULTIPLE PLANETS TO QUANTIFY THE EFFECT OF POTENTIAL UNDETECTED JOVIAN PERTURBERS ON THE ORBITAL CONFIGURATIONS OF THE KNOWN PLANETS. IN PARTICULAR IN ORDER FOR MANY PLANETS IN THE SAME SYSTEM TO BE OBSERVED TRANSITING REQUIRES LOW MUTUAL INCLINATIONS BETWEEN THE KNOWN PLANETS. SUCH A CONDITION WOULD BE EASILY DISTURBED BY A MASSIVE PLANET INCLINED BY JUST A FEW DEGREES TO THE ORBITAL PLANE OF THE TRANSITING PLANETS. WE PROPOSE TO PLACE DYNAMICAL CONSTRAINTS ON THE ORBITAL DISTANCES AND INCLINATIONS OF ANY SUCH JOVIAN PLANETS AND COMPARE THESE LIMITS TO THE CONSTRAINTS ON JOVIAN PLANET OCCURRENCE FROM RV SURVEYS. WHILE THERE ARE VARIOUS ESTIMATES OF JOVIAN PLANET OCCURRENCE FROM1-3AU FROM RV (E.G. WITTENMEYER ET AL. 2011 SCHLAUFMAN AND WINN 2016) THE SIZE OF SUB-SAMPLE KNOWN TO HAVE THREE OR MORE MINI- NEPTUNES CLOSE TO THE STAR IS JUST FIVE. OUR PROPOSED STUDY WILL PLACE A DYNAMICAL CONSTRAINT ON THE DISTANCES OUT TO WHICH JOVIAN PLANETS ARE VERY UNLIKELY. THIS WILL ENABLE A STATISTICAL COMPARISON WITH THE RESULTS OF RV SURVEYS TO DETERMINE IF THE COMPACT SYSTEMS OF MULTIPLE MINI-NEPTUNES ARE DRAWN FROM THE SAME POPULATION AS RV DETECTIONS OF JOVIANS GENERALLY.$54,616
· FY2017 · National Aeronautics and Space Administration
OUR PROPOSED PROGRAM WILL BE CRUCIAL TO PLANNING THE CHARACTERIZATION OF EXOPLANET ATMOSPHERES AT MERCURY TO VENUS-LIKE DISTANCES.$37,125
· FY2020 · National Aeronautics and Space Administration