Airbaf Mars
description
Transcript of Airbaf Mars
Design optimization and probabilistic assessment of a vented airbag
landing system for the ExoMarsspace mission
Vassili ToropovProfessor of Aerospace and Structural Engineering
Principal Design Optimization Specialist, Altair Engineering (until 2006)
ESA Aurora exploration programme
240kg mobile robotic exo-biology laboratory
To search for extinct or extant microbial life on Mars
Supporting geology and meteorology experiments
Launch by Ariane 5 or Soyuz in 2013
Currently in Phase B – mission planning and concept design phase
ExoMars Space Mission
Airbags for Space Landers Un-vented type
(inflatable ball)• Multiple bounces• Established
heritage (from Luna-9 in 1966)
• High mass• Vulnerable to
rupture
Mars Pathfinder NASA/JPL Beagle 2 Beagle2
Luna 9 USSR Space Program
Airbags for Space Landers
Vented type• Active control• Single stroke• No space heritage• Low mass• Vulnerable to
over-turning
ExoMars ESA
Kistler Booster Irvin
Design concept considers vented (or “Dead-Beat”) airbag coming to rest on second bounce
Inflated with N2 during descent under main parachute
Stowed rover mounted to platform
Vent patches activated by pyrotechnic cutters
Simple reactive vent control system: simultaneous all-vent trigger at 65g
Airbag Landing Design Concept
Six identical vented chambers
One “anti-bottoming” un-vented toroidal
Airbag Configuration
Study Objectives
Develop methodology for optimisation and probabilistic reliability assessment of vented airbags
Key questions for ExoMars:
1. What is the mass of an optimized vented airbag?
2. What is the probability of a successful landing?
3. What is the sensitivity of landing reliability to changing landing scenarios?
Failure modes:• Roll-over (payload overturns),• Dive-through (payload impacts rock)• Rupture (fabric tears)
Full-scale terrestrial testing is difficult / expensive
Optimization and reliability assessment of ExoMars lander
Analysis Overview
DoE
Surrogate Response Surfaces
Optimisation
Design Variables
DoE
Surrogate Response Surfaces
Monte Carlo Simulations
External Variables
ReliabilityOptimum Design
OPTIMISATION ROBUSTNESS
FE Analysis FE Analysis
Explicit FE analysis of 100ms + impact 10 CPU hours +
Metamodelling approach Metamodels built by MLSM Same approach for
optimization and reliability analyses
Optimization variables• Airbag size, pressure, vent
areas Reliability variables
• Wind speed, rock size, pitch attitude & rate
Finite Element Modelling
HyperMesh / LS-DYNA Rigid rover & platform Silicone-coated Vectran airbag
fabric N2 gas
Simulation Stages1. Inflation 2. Initial Impact (65g vent trigger
filtering)3. Venting
Vent Triggering
65g acceleration threshold Measured at payload CoM Signal noise premature venting Crude filter = cumulative time above threshold
Trigger Occurs at 0.0304s
0.0302s65.3g
0.0303s65.7g
0.0304s65.7g
LS-DYNA • Dynamic Relaxation (steady-state free fall condition)• Airbag functionality (Wang Nefske inflation model)• Advanced contact (internal fabric contact etc.)
HyperMesh • Advanced LS-DYNA model building support• Comprehensive interface
HyperView• Time dependent LS-DYNA animations• Multi results type environment (animations, X-Y data)
HyperMorph• Airbag parameterisation• Rock height, pitch angle variation in reliability assessment
HyperStudy• Airbag size optimisation• Reliability assessment
Software Tools
Mars Environment
• Gravity 3.7 m/s2 = 0.38g
• Pressure 440Pa = 0.4% of Earth air pressure at sea level = at 36.5 km altitude on Earth
• Temperature 187K = - 86º C
Landing Scenarios• Flat Bottom Landing
• Inclined Rock Impact
Mars Environment and Landing Scenarios
Flat Bottom Landing• Vertical velocity 25m/s• Favours ‘tall’ airbag designs• Favours ‘narrow’ airbag designs• Tall, narrow airbag makes most
effective vertical energy absorber
Landing scenarios are chosen to give conflicting design requirements
Inclined Rock Impact• Vertical velocity 25m/s• Lateral wind velocity 16.3m/s• Favours ‘wide’ airbag designs• Wide airbag makes most effective
rock intrusion absorber
Landing Scenarios
• Peak filtered deceleration 66g (Target <70g)• Peak airbag material stresses 135MPa (Target <533MPa)• Constraints satisfied by baseline design
Baseline Response: Flat Bottom Landing
• Peak filtered deceleration 980g (Target <70g)• Peak airbag material stresses 281MPa (Target <533MPa)• Deceleration constraint exceeded due to ‘Dive Through’
Baseline Response: Inclined Rock Impact
• It is critical to prevent ‘direct’ payload to Rock/Ground impact
• Such type of impact guarantees violation of deceleration constraint
Direct payload to rock impact due to ‘dive through’
Dive ThroughDive Through
ExoMars Lander: LS-DYNA Simulation
Design Objective - Minimise system mass (Airbag + Payload + Gas + System)
Design Constraints - Payload acceleration (<70g)- Airbag von Mises stress (<533MPa)- Re-bound and roll over inversion kinematics
Design objective and constraints evaluated for each landing scenario
Design Variables - Airbag base diameter (HyperMorph)- Airbag height (HyperMorph)- Airbag venting area- Airbag steady-state pressure (Mass of gas)
Minimise Design Objective by varying the Design Variables whilst satisfying the Design Constraints
Optimization Set-up
Design Variables : Airbag Height and Diameter
• Airbag geometry defined by dimensional relationships between height (H) and diameter (D) of cross-section, curves are elliptical sections
• Geometric factors a, b, c are constant
¼ ellipse
¼ ellipse
¼ ellipse
Design Parameterization
Need for metamodelling• One LS DYNA analysis of 0.2s after touchdown takes 10 hours of computing
Unifying approach• Both optimization and reliability study utilise metamodels
Accuracy of metamodels• Optimization and reliability studies based on metamodels• High quality metamodel is required
Metamodelling
DOEs for Metamodel Building
Main requirements to a Design of Experiments (DOE) are:• maximum quantity of information• achieved with minimum computational effort (number of numerical
experiments)
Optimal Latin Hypercube DOEs
Optimal Latin Hypercube (OLH) DOEs specify the sample points such that as much of the design space is sampled as possible, with the minimum number of response evaluations - especially useful when the evaluations are expensive.
OLH DOEs are highly structured in a way that:• They provide an optimal uniform distribution of sample points.• They spread out the sample points efficiently (space filling) through
out the design space.
LH DOE – conventional (random) and optimal
Random Latin hypercube
Optimal Latin hypercube
DOE Optimization: Objective Function (Audze & Eglais 1977)
Physical analogy: a system consisting of points of unit mass exert repulsive forces on each other causing the system to have potential energy. When the points are released from an initial state, they move. They will reach equilibrium when the potential energy of the repulsive forces between the masses is at a minimum. If the magnitude of the repulsive forces is inversely proportional to the distance squared between the points then minimize:
= = +
∑ ∑ 21 1
1P P
p q p pqLUmin = min
Potential energy (objective function) Distance between points p and q
permGA Iteration History for 2 Design Variables & 50 Points
permGA Iteration History for 2 Design Variables & 400 Points
Extended Uniform Latin Hypercube
Extended Uniform Latin Hypercube sampling, 21 point + 3 existing points
Extended Uniform Latin Hypercube sampling, 21 point + corners
Uniform Latin Hypercube sampling, 21 point
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Four Design Variables – 40 DOE Points (EULH) per Landing Scenario (80 in total)
Metamodelling: DoE
Metamodel building using Moving Least Squares Method (MLSM)
Suggested for generation of surfaces given by points
Used in meshless (mesh-free) form of FEM
Useful for metamodel building
Simple
Moving Least Squares Method
Generalization of a weighted least squares method where weights do not remain constant but are functions of Euclidian distance rk from a k-th sampling point to a point x where the surrogate model is evaluated.
xi
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DoE point
Evaluation point x
Moving Least Squares Method
The weight wi , associated with a sampling point xi , decays as a point x moves away from xi .
Because the weights wi are functions of x, the polynomial basis function coefficients are also dependent on x.
This means that it is not possible to obtain an analytical form of the approximation function but its evaluation is still computationally inexpensive.
( ) ( ) ( )[ ] min~)()(1
2→−= ∑
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pppp FFwG a,xxxxa
Gaussian weight decay function
wi = exp(-θri2)
where θ is “closeness of fit parameter”
θ = 1 θ = 10 θ = 100
Example: six-hump camel back functionF(x1,x2) = (4 - 2.1 x1
2 + x14 / 3) x1
2+x1x2+(- 4 + 4x22) x2
2, -2 ≤ x1 ≤ 2, -1 ≤ x2 ≤ 1.
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Example: six-hump camel back function
Original function Approximation on 20 sampling points, θ = 10
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Example: six-hump camel back function
Original function Approximation on 100 sampling points, θ = 120
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Example: Computing and Rendering Point Set Surfaces by M. Alexa et al. 2001
larger θ smaller θ
MLSM provides a high quality response surface to accurately approximate a highly nonlinear system.
Important feature of MLSM is efficient handling of numerical noise by adjusting “closeness of fit” parameter to provide close fit to a low noise situation or loose fit when the response exhibits a largeramount of noise
Direct Payload to Rock/Ground Impact resulting in high payload accelerations (>100g) occurred at high percentage of DOE points
These high results ‘swamp’ the responses of interest in the approximation
Suggestion: cap response at 100g
Metamodel Generation using MLSM
Noise outside area of interest
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To minimise this function, a good quality approximation of the valley should be obtained whilst ignoring numerical noise outside the valley
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MLSM Illustrative Example: Rosenbrock’s Banana Valley Function
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MLSM Illustrative Example: Rosenbrock’s Banana Valley Function
Capped function0
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MLSM approximation of capped function, 100 sampling points gives good approximation of function
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MLSM Illustrative Example: Rosenbrock’s Banana Valley Function
Optimization results
• Optimized Mass was 403.5kg (baseline 392.8kg)
• Flat Bottom Impact Payload Acceleration increased from 65.5g to 67.7g
• Rock Impact Payload Acceleration decreased from 980.3g to 69.1g
• Maximum Material Stresses were reduced from 281MPa to 157MPa
• While 3 variables are in middle of range, Vent Area pushes upper limit
• On review of the response data set obtained from the test plan points it was observed that there was a high percentage of runs that failed to meet the constraints
• This was reflected in the approximations and resulted in a small ‘sweet spot’ on the response surface where the constraints could be met
• Model mass varied very little (<0.25%) within this area (all runs in this area had more mass than baseline run)
Optimization results (cont.)
Ultimately, the reliability figure gives the probability of a successful landing for a given design under a range of conditions
Alternatively it can be used to establish an envelope of conditions for a given success probability
For this project, the limited number of variables (4) considered, results in a reliability index 'figure of merit', rather than an overall probability of success
Establishing this 'figure of merit', index for the reliability of a design gives a useful comparison with alternative designs
Reliability Assessment of ExoMars Lander
Adopt airbag design variables determined by optimization study Consider only rock impact loadcase (though rock height may be zero, i.e.
flat surface) Failure defined by exceeding similar constraints to optimisation study
• Resultant deceleration < 80g• Kinematic metrics, re-bound, roll-over• No bag tearing
Environment Variables
Design Variable Description
Lower Bound Upper Bound
DV1 Lateral Wind Velocity 0 m/s 20 m/sDV2 Rock Height 0 m 0.8 mDV3 Lander Pitch Attitude -20 º 20 ºDV4 Lander Pitch Rate -30 º/s 30 º/s
Reliability Assessment: Model Definitions
Wind Speed Probability Distribution
European Mars Climate Database (EMCD) - general circulation model
45°N to 45°S latitudes Season 12 Mars Global Surveyor dust
loading scenario PDF fit to EMCD model data Weibull distribution Mean = 8.0 m/s SD = 3.7 m/s
Mean Resultant Wind Speed
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Rock Height Probability Distribution
NASA/JPL rock size distribution model
Viking 1 & 2, MPF landing sites + Earth analogues
Landing Site rock coverage ≤20%
Overall rock coverage from orbital thermal imaging
Rock height = 0.5 x diameter Exponential PDF Mean = 0.196 m SD = 0.196 m
Probability Density Function f(H)
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Mars Pathfinder landing site panorama NASA/JPL
Pitch Angle and Pitch Rate
Pendulum motion + gust reaction under parachute at landing Assumed to be random with independent Gaussian Normal PDFs
Pitch Angle Mean = 0 degs 3σ = 30 degs
Pitch Rate Mean = 0 deg/s 3σ = 20 deg/s
• DOE – Uniform Latin HyperCube with Extremities Extension
• Eighty Test Points – 80 LS-DYNA runs executed (single load case)
• Metamodelling using Moving Least Squares Method
• Process is the same as used to generate optimization metamodel, but with different variables
Reliability Assessment of ExoMars Lander: Metamodel generation
Another one bites the dust!
Counting failures…..
Baseline Reliability Analysis & Results
Sample Size Success Probability 100 67.0% 1000 68.3% 10000 68.6%
100, 1000 and 10000 point Monte Carlo simulations
5 mins cpu on PC for 10000 sample points
Low reliability ~ 69% Inversion failure mode is
primary contributor Failed Monte Carlo samples +
FE runs indicate trailing edge contact problem
Sensitivity to Relaxed Landing Conditions
PDF Changed Success Probability Baseline 68.6% Wind Velocity 70.7% Rock height 70.8% Pitch Angle & Rate 80.8%
Reduced latitude band 45°N to 10°S
Morning landing for lighter winds
Landing sites with ≤ 10% rock coverage
Pitch angle and pitch rate variability reduced (knowledge / ‘chute design)
Cumulative improvement in reliability to ~ 81%
Pitch Angle and Rate yield biggest improvement
Parameter PDF Wind Velocity VH Weibull
α = 2 β = 7.49 m/s
Rock Height h Exponential
β = 0.151m
Pitch Angle θ0 Gaussian
3σ = 20°
Pitch Rate Ω0 Gaussian
3σ = 15°/s
Conclusions
General Successful development of methodology to vented
airbags Valuable tool for
• Design Optimization• Probabilistic robustness / reliability analysis• Can be extended to probabilistic design optimization
Importance of simulation-based methods because of difficulty / high cost of representative testing on earth
ConclusionsExoMars application The optimization study arrived at a design that satisfies the
requirements with only a small increase in mass Poor reliability estimated: 69 – 81% Vent areas could be increased Change in un-vented toroidal More complex venting control (e.g. differential triggering)
likely Reliability analysis uncovered failure modes that had not
previously been considered Consider pitch-up and pitch-down in future optimisation Increase simulation times to reduce inversion criteria
uncertainties Reliability analysis process can be employed in future phases
of the ExoMars project, with more comprehensive reliability analyses aiming at determining the overall airbag reliability
Astrium Mars Lander: LS-DYNA Simulation
Any questions?