Strong and weak scaling are crucial concepts in parallel computing, measuring how well programs perform as resources increase. Strong scaling focuses on speeding up fixed-size problems, while weak scaling maintains efficiency as both workload and resources grow.
These scaling approaches help optimize parallel algorithms and systems, balancing factors like communication overhead and load balancing . Understanding their nuances is key to designing scalable software and predicting performance in large-scale computing environments.
Strong vs Weak Scaling
Defining Strong and Weak Scaling
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Top images from around the web for Defining Strong and Weak Scaling Weak scaling of parallel FMM vs. FFT up to 4096 processes :: Lorena A. Barba Group View original
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Strong scaling measures speedup achieved when increasing processor count for a fixed problem size
Aims to reduce execution time
Calculated as speedup divided by number of processors
Weak scaling evaluates execution time changes as problem size and processor count increase proportionally
Maintains constant workload per processor
Calculated as ratio of execution times between scaled and baseline cases
Ideal strong scaling results in linear speedup (doubling processors halves execution time)
Perfect weak scaling maintains constant execution time as both problem size and processor count increase
Theoretical Foundations
Amdahl's Law underpins strong scaling
Describes theoretical maximum speedup achievable for a given parallel fraction of the program
Formula: S ( n ) = 1 ( 1 − p ) + p n S(n) = \frac{1}{(1-p) + \frac{p}{n}} S ( n ) = ( 1 − p ) + n p 1
Where S is speedup, n is number of processors, p is parallel fraction
Gustafson's Law complements Amdahl's Law for weak scaling
Considers potential for problem size expansion with increased computational resources
Formula: S ( n ) = n − α ( n − 1 ) S(n) = n - \alpha(n - 1) S ( n ) = n − α ( n − 1 )
Where S is speedup, n is number of processors, α is serial fraction
Scalability of Parallel Algorithms
Scaling Analysis Techniques
Strong scaling analysis measures execution times for fixed problem size across varying processor counts
Typically plotted as speedup versus processor count
Example: Running a climate model simulation with fixed resolution on 1, 2, 4, 8, 16 processors
Weak scaling analysis adjusts problem size proportionally to processor count
Compares execution times to baseline single-processor run
Example: Increasing the number of particles in a molecular dynamics simulation proportionally to processor count
Isoefficiency analysis combines strong and weak scaling concepts
Determines how problem size must increase with processor count to maintain constant efficiency
Formula: W ( p ) = K ⋅ T 0 ( W ( p ) , p ) W(p) = K \cdot T_0(W(p), p) W ( p ) = K ⋅ T 0 ( W ( p ) , p )
Where W is problem size, p is number of processors, K is isoefficiency constant, T_0 is overhead function
Visualization and Metrics
Log-log plots of execution time versus problem size or processor count reveal scaling limits
Identify regions of diminishing returns
Example: Log-log plot showing execution time flattening as processor count increases beyond a certain point
Strong scaling efficiency quantifies algorithm's utilization of additional processors
Values closer to 1 (or 100%) indicate better scalability
Formula: E s = T 1 n ⋅ T n E_s = \frac{T_1}{n \cdot T_n} E s = n ⋅ T n T 1
Where E_s is strong scaling efficiency, T_1 is execution time on 1 processor, n is number of processors, T_n is execution time on n processors
Weak scaling efficiency calculated by comparing execution times of scaled runs to baseline
Consistent times across scales indicate good weak scalability
Formula: E w = T 1 T n E_w = \frac{T_1}{T_n} E w = T n T 1
Where E_w is weak scaling efficiency, T_1 is execution time on 1 processor, T_n is execution time on n processors with n times larger problem
Problem and Algorithm Characteristics
Problem size significantly impacts strong scaling
Larger problems generally exhibit better strong scaling due to improved computation-to-communication ratios
Example: Matrix multiplication scaling better for 10000x10000 matrices compared to 100x100 matrices
Algorithmic characteristics determine scaling potential
Degree of inherent parallelism affects maximum achievable speedup
Task dependencies limit parallelization opportunities
Example: Embarrassingly parallel algorithms (Monte Carlo simulations) scale better than algorithms with complex dependencies (Gauss-Seidel iteration)
Communication-to-computation ratio often determines practical parallelization limits
High ratios lead to diminishing returns in strong scaling
Example: N-body simulations becoming communication-bound at high processor counts
System and Implementation Factors
Load balancing crucial for both strong and weak scaling
Imbalanced workloads lead to processor idling and reduced efficiency
Example: Uneven particle distribution in spatial decomposition of molecular dynamics simulations
Communication overhead (latency, bandwidth limitations) often limits strong scaling at high processor counts
Example: All-to-all communication patterns in FFT algorithms becoming bottlenecks
Memory hierarchy and cache effects impact both scaling types
Changes in data distribution across processors alter cache utilization
Example: Cache-oblivious algorithms maintaining performance across different problem sizes and processor counts
System architecture influences scaling behavior
Interconnect topology affects communication patterns
Memory organization impacts data access times
Example: Torus interconnects providing better scaling for nearest-neighbor communication patterns compared to bus-based systems
I/O operations can become bottlenecks in both scaling scenarios
Particularly impactful for data-intensive applications
Example: Parallel file systems (Lustre, GPFS) improving I/O scalability in large-scale simulations
Evaluating Parallel System Efficiency
Speedup curves plot relative performance improvement against processor count
Shape indicates degree of scalability
Example: Linear speedup curve for embarrassingly parallel problems vs. sublinear curve for communication-bound algorithms
Efficiency curves demonstrate utilization of additional resources
Declining curves suggest diminishing returns in scalability
Formula: E ( n ) = S ( n ) n E(n) = \frac{S(n)}{n} E ( n ) = n S ( n )
Where E is efficiency, S is speedup, n is number of processors
Iso-efficiency functions determine problem size increase rate to maintain efficiency
Help identify scalability limits
Example: Iso-efficiency function for matrix multiplication: W = Ω ( p 3 / 2 ) W = \Omega(p^{3/2}) W = Ω ( p 3/2 )
Where W is problem size, p is number of processors
Scalability vectors combine multiple metrics for comprehensive performance view
Include factors like speedup, efficiency, and problem size scaling
Example: 3D vector (speedup, efficiency, communication overhead) tracking scaling behavior
Advanced Analysis Techniques
Crossover points in scaling curves identify transitions between scaling regimes
Example: Transition from computation-bound to communication-bound behavior in strong scaling of iterative solvers
Roofline models adapted for scaling analysis
Incorporate communication costs and parallel efficiency into performance bounds
Example: Extended roofline model showing how communication bandwidth limits achievable performance at high processor counts
Scalability prediction models estimate large-scale performance
Based on analytical or empirical approaches
Example: LogGP model predicting communication overhead for different system sizes
Gustafson-Barsis' Law used for weak scaling predictions
Estimates speedup for scaled problem sizes
Formula: S = p − α ( p − 1 ) S = p - \alpha(p - 1) S = p − α ( p − 1 )
Where S is speedup, p is number of processors, α is serial fraction