Award Abstract # 1638156
ISS: Quantifying Cohesive Sediment Dynamics for Advanced Environmental Modeling

NSF Org: CBET
Division of Chemical, Bioengineering, Environmental, and Transport Systems
Recipient: UNIVERSITY OF CALIFORNIA, SANTA BARBARA
Initial Amendment Date: August 20, 2016
Latest Amendment Date: December 15, 2020
Award Number: 1638156
Award Instrument: Standard Grant
Program Manager: Ron Joslin
rjoslin@nsf.gov
 (703)292-7030
CBET
 Division of Chemical, Bioengineering, Environmental, and Transport Systems
ENG
 Directorate for Engineering
Start Date: September 1, 2016
End Date: February 28, 2022 (Estimated)
Total Intended Award Amount: $299,996.00
Total Awarded Amount to Date: $479,990.00
Funds Obligated to Date: FY 2016 = $299,996.00
FY 2019 = $119,997.00

FY 2020 = $59,997.00
History of Investigator:
  • Paolo Luzzatto-Fegiz (Principal Investigator)
    fegiz@engineering.ucsb.edu
  • Eckart Meiburg (Co-Principal Investigator)
Recipient Sponsored Research Office: University of California-Santa Barbara
3227 CHEADLE HALL
SANTA BARBARA
CA  US  93106-0001
(805)893-4188
Sponsor Congressional District: 24
Primary Place of Performance: University of California-Santa Barbara
Office of Research, 3227 Cheadle
Santa Barbara
CA  US  93106-2050
Primary Place of Performance
Congressional District:
24
Unique Entity Identifier (UEI): G9QBQDH39DF4
Parent UEI:
NSF Program(s): PMP-Particul&MultiphaseProcess,
FD-Fluid Dynamics,
Special Initiatives
Primary Program Source: 01001617DB NSF RESEARCH & RELATED ACTIVIT
01001920DB NSF RESEARCH & RELATED ACTIVIT

01002021DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s):
Program Element Code(s): 141500, 144300, 164200
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.041

ABSTRACT

PI: Luzzatto-Fegiz, Paolo
Proposal Number: 1638156

The proposed research is focused on the study of forces between particles that tend to cluster. The physical system is that of sentiments of quartz and clay particles. The advantage of conducting experiments at the International Space Station (ISS) is that it will be possible to separate the forces acting on the particles among short range (adhesive forces) and long range (cohesive forces), since one can observe the clustering dynamics over very long time scales without gravitational settling, which complicates the measurements when doing experiments on Earth. The quartz/clay system is commonly found in a wide variety of environment settings (rivers, lakes, oceans) and plays an important role in technological efforts related to deep sea hydrocarbon drilling and CO2 sequestration. Oil companies typically spend millions per well to fund exploratory drilling operations, and might require multiple exploration missions to find one good site. Results from this work could lead to a better computation model that will allow oil companies to find spots on the deep sea for drilling productive oil wells with higher precision.

The dynamics of cohesive sediment is governed by the interplay of gravitational, electrostatic and hydrodynamic forces. Earth-based laboratories do not allow for the investigation of cohesive and adhesive forces in isolation, as these are usually obscured by the effects of gravity and gravitational settling. Consequently, existing models for the dynamics of cohesive sediment have severe shortcomings, and reliable scaling laws for the magnitude of the inter-particle forces and the resulting flocculation rates and erodibility as functions of such parameters as grain size, surface size, grain material and water salinity are not available. This represents a serious impediment for predictive modeling efforts of a range of environmental systems in which cohesive sediment plays a central role, among them rivers, lakes, estuaries, the coastal ocean, fisheries and benthic habitats. Furthermore, given the high cost of deep-sea drilling, computational sediment transport models also play an increasingly important role in deep-water hydrocarbon exploration, where improved modeling tools will result in tangible economic benefits. The ISS microgravity laboratory will enable us to investigate cohesive and adhesive forces in isolation, without interference from gravity and the associated settling motion. In this way, the proposed research will allow us to formulate scaling laws for the dynamics of cohesive sediment as function of grain size, grain material and water salinity. The ISS experiments will to a large extent take advantage of an existing experimental apparatus that was employed in a previous investigation, so that the time and cost of preparing the experiments can be kept to a minimum. The scaling laws identified via the ISS experiments will subsequently be implemented into an existing, particle-resolving CFD code for detailed follow-up investigations of cohesive sediment dynamics under conditions with and without gravity. The proposed research will result in advanced predictive models for such environmental systems as rivers, lakes, estuaries, the coastal ocean, fisheries and benthic habitats, as well as for deep-sea hydrocarbon exploration and proposed CO2 sequestration strategies. On the educational side, the proposed research project will educate and train a postdoctoral scholar, as well as graduate, undergraduate and high school students in the broad concepts of microgravity fluid dynamics and computational model development.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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Vowinckel, B. and Withers, J. and Luzzatto-Fegiz, Paolo and Meiburg, E. "Settling of cohesive sediment: particle-resolved simulations" Journal of Fluid Mechanics , v.858 , 2019 10.1017/jfm.2018.757 Citation Details
Vowinckel, B. and Withers, J. and Meiburg, E. and Luzzatto-Fegiz, P. "Grain-Resolved Simulations of Cohesive Sediment" EuroMech Colloquium 588: Coupling mechanisms and multi-scaling in granular-fluid flows, 2 October 5 October 2017, Toulouse, France. , 2017 Citation Details
Vowinckel, Bernhard and Biegert, Edward and Luzzatto-Fegiz, Paolo and Meiburg, Eckart "Consolidation of freshly deposited cohesive and noncohesive sediment: Particle-resolved simulations" Physical Review Fluids , v.4 , 2019 10.1103/PhysRevFluids.4.074305 Citation Details

PROJECT OUTCOMES REPORT

Disclaimer

This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.

Fine sediment (e.g. mud) can display ?cohesion?, which is manifested by strong attractive forces between particles, which arise at short distances. As a result, cohesive sediment particles can form larger aggregates, whose settling rates are much faster than those of the original particles. Predicting cohesion as a function of sediment type and water salinity is therefore essential for modeling ecosystems, pollutant transport, and structure of hydrocarbon reservoirs. However, whereas sediment sinking in the oceans can aggregate over long times, the duration of Earth-based, laboratory experiments is inherently limited by the size of the experimental facility. By contrast, microgravity experiments aboard the International Space Station (ISS) can observe aggregation over months. 

 

Detailed ground-based experiments were conducted to identify the most scientifically valuable types of sediment and salt concentrations. In parallel, a supercomputer program was developed, capable of simulating the interactions of cohesive particles, which was used to carefully investigate the dynamics of sediment both in an earth-based setting and in microgravity, synergistically with the experiments. The selected array of sediment mixtures was launched to the ISS, where aggregation processes were recorded for nearly 100 days, alongside with the detailed structure of the resulting aggregates.

The ground-based experiments clarified the role of salinity for clay aggregation in environmental fluid mechanics, demonstrating that trace amounts of salt, commonly found in lakes and rivers, can be sufficient to trigger aggregation. The computer simulations successfully reproduced key features of aggregation in gravitational settings, ranging from interactions between particle pairs to the dynamics of large particle ensembles. The ISS experiments successfully measured aggregation rates as a function of sediment composition, even for very weakly cohesive sediment. In addition, aggregation was observed for much longer, and for larger particles, than had been expected based on established models. A physical process was proposed to explain these unexpected dynamics, arising from the interplay of small-amplitude, broadband vibration (which is common aboard spacecraft) and particle polydispersity.  The simulation program was extended to also capture these vibrational effects, and to carefully test this hypothesis. This long-term aggregation mechanism, applicable to relatively large particles, may also find applications in on-orbit manufacturing and in understanding planetary formation.


Outreach components comprised contributions to the South by Southwest (SXSW) conference, including a hands-on demonstration; an appearance in the first ultra-HD video from space (https://www.nasa.gov/8k- science), and in a Video Research Spotlight for the ISS mission SpaceX CRS-15; a contribution to a National Space Council discussion on future of microgravity research; and a feature in the ISS National Lab ?Upward? magazine.


Last Modified: 06/29/2022
Modified by: Paolo Luzzatto-Fegiz

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