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Computational Flow Assurance
Recent progress in modelling of multiphase flows in long pipelines Simon Lo, Abderrahmane Fiala (presented by Demetris Clerides) Subsea Asia 2010
Computational Flow Assurance Recent progress in modelling of - - PowerPoint PPT Presentation
www.cd-adapco.com Computational Flow Assurance Recent progress in modelling of multiphase flows in long pipelines Simon Lo, Abderrahmane Fiala (presented by Demetris Clerides) Subsea Asia 2010 Agenda Background Validation studies
www.cd-adapco.com
Recent progress in modelling of multiphase flows in long pipelines Simon Lo, Abderrahmane Fiala (presented by Demetris Clerides) Subsea Asia 2010
– Espedal – stratified flow – TMF - slug flow – StatOil – wavy-slug flow
– Long pipeline
– 1D-3D coupling
– Engineers need to know if proposed designs will function
properly under increasingly harsh operating offshore/subsea conditions
– Experience and “gut feel” become less reliable in new
environments
– Physical testing is increasingly expensive and less reliable
due to scaling assumptions
into a leading position as a design tool: “Up Up-Front” numerical/virtual testing to validate and improve designs before they are built and installed
– Fast enough to provide answers within the design timeframe – Accurate enough to provide sufficiently insightful answers for
better design decisions
Fidelity Simulation to meet these effectiveness requirements, e.g.
– 1-D simulations (OLGA) for long pipeline systems – 3-D simulations (STAR) for equipment, transition regions – A user-friendly computing environment for activating the right
mix of tools for the situation being examined: co-simulation
Computatio ional l Time (wall-clock) Fidelity ity/detail l of Simulatio ion 0.1 1 10 10 100 100 1,000
Higher fidelity (= more detailed insight) requires increasing computational time (wall-clock)
10,000
Piping Network k Dynamics cs (e.g., HYSIS)
1-D D Steady- State Multiphase Flow w (e.g., ., PIPEFLO
1-D Transi sient (e.g., OLGA)
Improve ved 3-D D CFD with STAR & HPC
3-D CFD
Pressure ure gradien ent Liqui uid d level el
Imperial College.
volume fraction.
Experime iment nt STAR-CD CD
Experime iment nt STAR-CD CD
initial development
needed for the instabilities to develop into waves and slugs.
agrees well with measured data.
each.
Experime iment nt STAR-CD CD
Density ity/Den Density ity-oil il calculat lated as density ity of 2 phase mixtu ture re/d /density ity
Usg
sg=1.01 m/s, Usl sl=1.26 m/s
Experime iment nt STAR-CD CD
Experime iment nt STAR-CD CD
Usg
sg=1.01 m/s, Usl sl=1.50 m/s
Experime iment nt STAR-CD CD
Wave speed Experiment (m/s) STAR-CD (m/s) Gas-oil 2.8 2.58 Gas-water 3.2 2.7 Power (FFT) Dominant period Experiment (s) STAR-CD (s) Gas-oil 2.7 2.23 Gas-water 1.34 1.57 Density / Density liquid Experiment STAR-CD Gas-oil 0.63 0.656 Gas-water 0.55 0.68
locations of know distance and time delay between the signals.
be done within 1 week.
slug, churn, and annular flow may occur.
─
Hydrodynamic slugging: induced by growth of Kelvin-
Helmholtz instabilities into waves then, at sufficiently large heights, into slugs
─
Terrain slugging: induced by positive pipeline inclinations,
such as section A
─
Severe slugging: induced by gas pressure build-up behind
liquid slugs. It occurs in highly inclined or vertical pipeline sections, such as section B, at sufficiently low gas velocities.
101.6 m 10.9 m
(A) (B)
Diameter D=70 mm
→ butterfly mesh
─
Inlet: Velocity
»
Uliq = 1.7 m/s
»
Ugas = 5.4 m/s
»
Liquid Holdup αL = 0.5
»
ρliq = 914 kg/m3
─
Outlet: Pressure
»
p = 105 Pa
─
αL = 0.5 , αG = 0.5
─
U = V = W = 0.0 m/s
─
μliq = 0.033 Pa.s
─
μgas = 1.5x10-5 Pa.s
Application Proving Group
Run for about two flow passes, based on inlet liquid velocity
─
Total Physical Time = 132 s
─
Start-up run physical time, t1 ≈ 74.5 s
─
Restart run physical time, t2 ≈ 57.5 s
A variable time step size based on an Average Courant
Number criterion
─
CFLavg = 0.25
Run on 64 cores (Rogue cluster)
─
27500 cells per core – expected linear scalability
Start-up Restart Total
Number of Time Steps 174036 138596 312632 Physical Time (s) 74.534 57.610 132.144 CPU time (s) 834523 664441 1498964 Elapsed time (s) 866038 690601 1556639 CPU time (d/h/min/s) 9d 15h 48min 43s 7d 16h 34min 1s 17d 8h 22min 44s Elapsed time (d/h/min/s) 10d 0h 33min 58s 7d 23h 50min 1s 18d 0h 23min 59s CPU (s) / TimeStep 4.80 4.79 4.79 CPU / Physical 11197 (3.11 h/s) 11533 (3.20 h/s) 11343 (3.15 h/s) Elapsed / Physical 11619 (3.23 h/s) 11987 (3.33 h/s) 11780 (3.27 h/s) TimeStep size (ms) 0.43 0.42 0.42 Outer ITERmax 9.69 9.42 9.55 CFLmax 31.45 26.45 28.95
Transient data monitored at 10 locations:
─
Inlet
─
Monitor (1): end of positive inclined section
─
Monitor (2): end of negative inclined section prior to riser
─
Monitors (3) to (8): as shown in schematic below
─
Outlet
Type of data monitored:
─
Liquid hold-up (i.e., VOF scalar)
─
Pressure
─
Density
─
Velocity
Inlet Monitor (1) Monitor (2) Outlet
Monito tor r (3) (4) (5) (6) (7) (8)
Area-averaged liquid holdup at monitoring point (1) Area-averaged liquid hold-up – Monitor (1)
Area-averaged liquid hold-up – Monitor (2)
The simulation of a two-phase oil-gas flow
in a realistic geometry pipeline was carried
STAR-CD was able to successfully
capture:
─
Wavy flow
─
Slug flow
─
Severe slugging
─
Churn flow
─
Annular flow
Inlet et
Outle let Flow w rates from OLGA to STAR Pressure re from STAR to OLGA Flow w rates from STAR to OLGA Pressure re from OLGA to STAR
To seamless essly study 3D effects ts in in-lin ine e equipme ment nt: : valves, es, juncti tion
, elbows
les, jumpers ers, separators tors, , slug g catche hers, , compres essors
, ... Note: strati tifi fied ed flow becomes es annular ar flow due to two circum umferen ferential tial pipe dimples es
Inlet et Outlet Flow w rates from OLGA to STAR Pressure ure from STAR to OLGA
OLGA pipe:
STAR pipe:
flow area (valve, fouling/hydrate deposit,...)
– OLGA sends outlet mass flow rates to STAR for inlet
conditions.
– OLGA sends outlet mass flow rates to STAR for inlet
conditions.
– STAR returns computed pressure at inlet to OLGA for outlet
pressure value.
Inlet et
Outlet let
Flow w rates from OLGA to STAR Pressure ure from STAR to OLGA Flow w rates from STAR to OLGA Pressure ure from OLGA to S STAR
Note te: Annular lar flow at outlet let of STAR pipe.
One OLGA session
ende dent t pipel eline nes.
Inlet et Outle t Flow w rates from OLGA to STAR Pressure ure from STAR to OLGA Flow w rates from STAR to OLGA Pressure ure from OLGA to STAR Note: Annular ar flow at outlet of STAR pipe. Water Oil
Upstre tream am pipe Downstr tream am pipe – flows ws are getting ng throug ugh the STAR pipe e into the downstre tream am pipe
Inlet et Outlet Flow w rates from OLGA to STAR Pressure ure from STAR to OLGA
long pipelines.
(compared to traditional 1D methods).
STAR for 1D analysis of long pipeline with detailed 3D simulation to study effects in local regions (the “3-D microscope”).
two-way coupling.
cases and more detailed analyses will follow.