Basic Algorithms and Data Structures
Niklaus Wirth, a Turing Award laureate and the creator of the Pascal programming language, famously stated: Program = Algorithm + Data Structure. Data structures determine how to organize data efficiently, while algorithms define the steps to solve a problem. Together, they form the core of any software program. Although this is a simplification, it captures the essence of software development. Consequently, algorithms and data structures are the most common topics in technical interviews.
Algorithms and data structures are equally fundamental to LabVIEW. However, because LabVIEW has historically been used to write test and measurement applications—which often rely on a few standard structures—their importance is sometimes overlooked. Yet, the choice of algorithms and data structures has a far greater impact on execution speed than the choice of programming language (e.g., LabVIEW vs. C). Mastering these fundamentals can significantly boost your application's performance. While developers sometimes complain about LabVIEW's execution speed, most inefficient programs simply have poorly optimized algorithms.
Since algorithms and data structures are vast fields that could easily fill a semester-long course, this section only covers the basic concepts and structures most relevant to LabVIEW development.
Time Complexity
To evaluate the efficiency of a program, we use a metric called algorithm complexity, which is divided into time complexity and space complexity. Space complexity measures the memory required to execute an algorithm, while time complexity measures the computational workload relative to the input size, directly determining the execution speed.
Time complexity is expressed as a function using Big O notation, where represents the size of the input data:
- (Constant Time): The runtime remains constant regardless of the input size .
- (Linear Time): The runtime grows proportionally with the input size (e.g., , where is a constant).
- (Quadratic Time), (Cubic Time), etc.: The runtime grows proportionally to the square, cube, or higher powers of the input size.
These are polynomial-time complexities, and algorithms within this range are generally practical for real-world software. However, if an algorithm's complexity grows exponentially (e.g., ) or factorially (e.g., ), it quickly becomes unusable for large inputs. For instance, the naive Fibonacci recursion algorithm has a complexity of , which is too slow for inputs greater than 40 on modern computers. Finding the lowest possible complexity for a given problem is always a primary goal of algorithm design.
Determining Prime Numbers
Let's analyze the time complexity of prime factorization. If a number is known to be the product of two prime numbers, how long does it take to find those primes?
Multiplying two numbers takes nearly constant time . However, factoring their product is much harder. In the worst case (when is the product of two identical primes), we must test potential factors up to . Thus, the time complexity of this trial division is .
Here is a simple program that factors the product of two primes:

Even with optimizations (such as skipping even numbers), the complexity remains . While sounds efficient, it becomes impractically slow for large inputs. If both prime factors are larger than , a standard computer will take years to factor their product.
This asymmetry—where multiplication is easy but factorization is hard—is the foundation of modern cryptography, such as the RSA encryption algorithm. In RSA, a user generates a key by multiplying two massive primes. While anyone can encrypt a message using the public product, only the keyholder can decrypt it easily because decryption requires knowing the individual prime factors.
To use this method, we must first generate large primes. But how can we verify if a large random number is prime without trying to factor it?
Fortunately, there are highly efficient primality tests. For example, Fermat's Primality Test uses Fermat's Little Theorem: if is prime and is not divisible by , then . If a number fails this condition for any base , it is composite. To reduce false positives (known as Fermat pseudoprimes), we test multiple bases. For 64-bit unsigned integers (U64), testing the first five primes () is mathematically sufficient to guarantee primality.
To prevent arithmetic overflow when calculating for large numbers, we must use modular exponentiation rather than direct exponentiation.
We can write a program based on Fermat's Little Theorem. To compute , we use the modular exponentiation algorithm rather than direct exponentiation to avoid number overflow.
[!NOTE] The Python code below implements modular exponentiation, which is commonly used in Fermat primality testing. Although sometimes referred to as Montgomery multiplication, Montgomery reduction is actually a lower-level hardware optimization for fast multiplication under a modulus, whereas the algorithm here is standard modular exponentiation.
def mod_pow(base, exponent, modulus):
result = 1
base %= modulus
while exponent > 0:
if exponent % 2 == 1:
result = (result * base) % modulus
base = (base * base) % modulus
exponent //= 2
return result
def is_prime_fermat(n):
if n < 2:
return False
if n == 2 or n == 3:
return True
# For robust production applications, the Miller-Rabin primality test is recommended.
# The Fermat primality test shown here is a simplified demonstration.
for a in [2, 3, 5, 7, 11]:
if mod_pow(a, n-1, n) != 1:
return False
return True
The corresponding LabVIEW implementation is shown below:

By testing sequential integers starting from , this program instantly identifies the next prime number: .
Arrays
Efficiency of Basic Operations
In Arrays and Loops, we covered basic array operations. Here, we analyze their performance characteristics, which depend directly on how arrays are laid out in memory.
An array stores elements of the same datatype in a contiguous block of memory:
Because elements are contiguous and uniform in size, calculating the address of any element is a simple arithmetic operation: address = start_address + index * element_size. Consequently, accessing or modifying an array element by index has a time complexity of .
However, inserting or deleting elements is much slower. Since elements must remain contiguous, inserting an element in the middle requires shifting all subsequent elements to the right. Deleting an element requires shifting elements to the left. In the worst case (inserting at the beginning), every element must be moved, yielding a time complexity of .
Consider a program that constructs a 100,000-element array containing integers from 99,999 down to 0 in descending order.
A naive approach might insert the loop index at index 0 on each iteration, as shown in the top sequence structure below:

Because inserting at the beginning has a complexity of , doing this times results in a total complexity of .
In LabVIEW, the most efficient way to build an array is by enabling auto-indexing on the output tunnel of a loop. The middle and bottom sequence structures show two optimal methods. On my computer, the execution times for time, time 2, and time 3 were 450 ms, 1 ms, and 2 ms, respectively—demonstrating a massive performance difference.
Here's a thought for the readers: Inserting data at the array's start is evidently slow, but what about inserting at the end of the array? If the new element is the array's last, then moving other elements isn't necessary. Is that correct?
Inserting or deleting data at the end of an array does not require shifting other elements, so its time complexity is —the same as indexing. Therefore, this is also a recommended and efficient operation, provided you avoid inserting or deleting elements at the beginning or middle of the array.
However, even though they share the same time complexity, appending/removing elements at the end of an array is still slower than pre-initializing an array and modifying elements by index. This is due to two reasons:
- Length Update Overhead: Appending elements requires updating the array's size metadata, though this step takes negligible time.
- Dynamic Memory Allocation: LabVIEW allocates memory with some headroom to allow the array to grow at the end. However, if you add too many elements, the contiguous memory block might run out of space (as subsequent addresses are occupied by other variables). In this case, LabVIEW must request a new, larger memory block from the OS and copy the entire array to the new location. This reallocation and copying process is very expensive. While it happens infrequently enough that the amortized time complexity is still , it is a potential performance bottleneck.
Therefore, the most efficient way to build a large array in LabVIEW is to pre-initialize it with a fixed size using the Initialize Array function, or use a loop's auto-indexing tunnel. Both methods allow LabVIEW to determine the required memory size upfront and allocate it in a single operation, avoiding repeated memory reallocation and copy overhead.
Multidimensional Arrays
LabVIEW does not support "arrays of arrays" (nested arrays where each row has a different length) because array indexing relies on a fixed, predictable memory offset. Instead, we use multidimensional arrays, where every row must have the same length.
A 2D array represents data in rows and columns:
In memory, a 2D array is stored in a contiguous block row by row (row-major order). Because each row has exactly elements, finding the element at row , column is fast: address = start_address + (m * i + j) * element_size.
For variable-length datatypes (like strings or clusters), LabVIEW stores an array of pointers (references) to the actual data. Since the pointers are uniform in size (typically 4 or 8 bytes), the array can still be indexed in time, while the actual string data is allocated elsewhere in memory. See Flattening Data to Strings for details.
Sorting
Sorting is a fundamental programming task. While LabVIEW provides built-in sorting functions, understanding the underlying algorithms helps you write custom, optimized routines.
Consider sorting a pile of apples by size:
- Selection Sort: Find the largest apple, place it first. Find the largest of the remaining, place it second, and so on.
- Insertion Sort: Take an apple and insert it into its correct position relative to the apples already sorted.
- Bubble Sort: Compare adjacent apples, swap them if they are in the wrong order, and repeat. After passes, the array is sorted.
Bubble Sort is popular for its simplicity. Here is a LabVIEW implementation:

These three algorithms have a time complexity of because they perform redundant comparisons. If you know and , you do not need to compare and .
Quick Sort avoids redundant comparisons. It selects a pivot element, divides the array into elements larger than the pivot and elements smaller, and then recursively sorts the sub-arrays. This reduces the time complexity to . LabVIEW's built-in sorting functions use Quick Sort.
Can we sort faster than