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GELE Adjustment Computations (Least Squares)Theory of Errors, Weights and Most Probable ValueCheat Sheet

Cheat sheet for GELE Adjustment Computations (Least Squares) — Theory of Errors, Weights and Most Probable Value. Compact, printable, and organised around the concepts Professional Regulation Commission (PRC) — Board of Geodetic Engineering tests most frequently in the GELE 2026. Perfect for the week before exam day.

Exam context

The Geodetic Engineer Licensure Examination is conducted by Professional Regulation Commission (PRC) — Board of Geodetic Engineering and is scheduled for September 2026. The Adjustment Computations (Least Squares) subtest is marked as "Core" in the official pattern, and Theory of Errors, Weights and Most Probable Value appears in position 1st of 5 in the GELE Adjustment Computations (Least Squares) review rotation. Passing mark: 70% weighted average, no sub-test below 50%. Recent GELE 2026 papers have drawn roughly a meaningful share of questions from this subject.

Theory of Errors, Weights and Most Probable Value - Cheat Sheet

Your last-minute rapid-fire reference for error theory, weights, and most probable values in adjustment computations. Focus on formulas, definitions, and exam traps—zero fluff.

Sections

Common Values

Value

0.6745

Symbol

Quantity

Probable Error constant

Section Title

Error Classification & Characteristics

Important Facts

  • Blunders must be detected and rejected—no statistical cure.
  • Systematic errors must be modeled, corrected, or eliminated before least squares.
  • Random errors follow Gaussian (normal) distribution; adjustment assumes they are random and independent.
  • Standard deviation σ and variance σ² quantify random error magnitude.
  • Probable error PE = 0.6745σ (50% of errors fall within ±PE).

Key Definitions

Term

Blunder (Mistake)

Example

Misreading a rod as 1.53 m instead of 2.53 m

Definition

Large, identifiable error from human carelessness or instrument malfunction—always eliminate before adjustment.

Term

Systematic Error

Example

Tape always reads 0.05 m too short due to temperature effect

Definition

Consistent, directional error due to instrument or environment—model and correct mathematically before adjustment.

Term

Random Error (Accidental Error)

Example

Slight centering misalignment varying ±0.001 m per setup

Definition

Small, unpredictable, sign-varying errors governed by normal distribution—handled by adjustment and statistical methods.

Diagrams To Know

  • Bell curve (normal distribution) with σ, 2σ, 3σ marked
  • Error classification flowchart: Identify → Blunder? → Eliminate; Systematic? → Correct; Random? → Adjust

Formulas

Formula

x̄ = Σx / n

Meaning

x̄ = arithmetic mean; Σx = sum of all observations; n = number of observations

Watch Out

Do NOT use this if observations have different precisions—use weighted mean instead.

When To Use

When all observations have equal reliability (equal weight).

Formula

vᵢ = xᵢ − x̄

Meaning

vᵢ = residual of observation i; xᵢ = individual observation; x̄ = arithmetic mean

Watch Out

Residuals are deviations from the MPV, not errors. Sum of residuals must equal zero (within rounding).

When To Use

Always compute residuals to verify Σv ≈ 0 and calculate standard deviation.

Formula

σ = √(Σv² / (n−1))

Meaning

σ = standard deviation of a single observation; Σv² = sum of squared residuals; n−1 = degrees of freedom

Watch Out

Use n−1, NOT n. Using n underestimates error. This is sample, not population, standard deviation.

When To Use

Quantify the precision of individual measurements; use n−1 (sample standard deviation).

Formula

σₓ̄ = σ / √n

Meaning

σₓ̄ = standard deviation of the mean; σ = single-observation std dev; n = number of observations

Watch Out

Improvement is √n, NOT n. Adding 4 measurements reduces error by factor of 2, not 4.

When To Use

Estimate precision of the final MPV result; shows how many measurements improve accuracy.

Section Title

Most Probable Value (MPV) for Equal-Weight Observations

Important Facts

  • For equal-weight observations, the arithmetic mean is the most probable value.
  • Σv = 0 always (within rounding error)—use as a check on calculations.
  • Σv² quantifies total error; larger Σv² means poorer precision.
  • Standard deviation σ represents precision of individual observations.
  • Standard deviation of mean σₓ̄ is always smaller than σ by factor √n.
  • n−1 is used because one degree of freedom is lost estimating the mean.
  • Larger n always improves precision (reduces σₓ̄), but only by √n, not linearly.

Key Definitions

Term

Arithmetic Mean

Example

Five distance readings: 100.01, 100.02, 100.03, 100.02, 100.02 m → mean = 100.02 m

Definition

Sum of all equal-weight observations divided by count—the most probable value for redundant equal-precision data.

Term

Residual

Example

If x̄ = 100.02 m and one reading is 100.03 m, residual v = +0.01 m

Definition

Difference between an observation and the most probable value; v = x − x̄.

Term

Standard Deviation (σ)

Example

σ = 0.015 m means most readings fall within ±0.015 m of the mean

Definition

Root-mean-square of residuals; measures scatter and precision of observations around the mean.

Diagrams To Know

  • Residual scatter plot around mean showing positive and negative deviations
  • Precision improvement curve: σₓ̄ vs. n (hyperbolic decay)

Formulas

Formula

wᵢ = 1 / σᵢ²

Meaning

wᵢ = weight of observation i; σᵢ² = variance (std dev squared) of observation i

Watch Out

Weight is INVERSE to σ², not σ. Never use 1/σ or 1/σᵢ—always 1/σ².

When To Use

Assign weights when observations have different precisions; inverse proportional to variance.

Formula

wᵢ ∝ 1/Kᵢ (leveling)

Meaning

wᵢ = weight; Kᵢ = distance (in km) of leveling route i

Watch Out

Weight is INVERSE to distance. A 1 km route is 2× more reliable than a 2 km route; assign w = 2 vs. w = 1.

When To Use

In leveling networks, shorter routes are more reliable and get higher weight.

Formula

wᵢ ∝ nᵢ (repeated measurements)

Meaning

wᵢ = weight; nᵢ = number of repeated measurements for observation i

Watch Out

Higher n = higher weight (opposite of distance rule). More repeats = more reliable.

When To Use

When an observation is repeated multiple times, weight is directly proportional to repetition count.

Section Title

Weights & Weight Assignment Rules

Important Facts

  • Weight w = 1/σ²—always reciprocal of VARIANCE, not standard deviation.
  • Higher precision (smaller σ) → higher weight (more influence on MPV).
  • In leveling: shorter distance → shorter random error → higher weight; w ∝ 1/K.
  • More repetitions → higher weight; w ∝ n (directly proportional).
  • Weight can be normalized (relative weight) without changing final result.
  • Zero weight means zero influence on weighted mean; should not occur in practice.

Key Definitions

Term

Weight

Example

Observation A with σ = 0.02 m has weight wₐ = 1/0.02² = 2500; observation B with σ = 0.01 m has wᵦ = 10,000 (B is more reliable, higher weight)

Definition

A dimensionless number expressing relative reliability of an observation; inversely proportional to variance (error²).

Term

Relative Weight

Example

If computed weights are 2500 and 10,000, relative weights are 1 and 4 (divide by 2500)

Definition

Weight normalized to a reference; often used to compare observations without absolute variance values.

Diagrams To Know

  • Weight hierarchy chart showing precision vs. weight relationship
  • Leveling network with weights assigned by route distance

Formulas

Formula

x̄w = Σ(wᵢ·xᵢ) / Σwᵢ

Meaning

x̄w = weighted mean; wᵢ = weight of observation i; xᵢ = observation value; Σwᵢ = sum of all weights

Watch Out

Numerator is SUM OF WEIGHTED OBSERVATIONS, not sum of weights times mean. Every xᵢ must be multiplied by its own wᵢ.

When To Use

When observations have different weights (unequal precision); always use for least squares foundation.

Formula

vᵢ = xᵢ − x̄w

Meaning

vᵢ = weighted residual; xᵢ = observation; x̄w = weighted mean

Watch Out

Residuals from weighted mean do NOT sum to zero in general (unlike unweighted case). Use Σ(wᵢ·vᵢ) ≈ 0 as check.

When To Use

Compute residuals around weighted mean for error analysis and standard deviation of weighted mean.

Formula

σw = √(Σ(wᵢ·vᵢ²) / (n−1))

Meaning

σw = standard deviation of weighted observations; wᵢ·vᵢ² = weighted squared residual; n−1 = degrees of freedom

Watch Out

Use n−1 for sample; numerator must include weights (wᵢ·vᵢ², NOT just vᵢ²).

When To Use

Measure precision of individual weighted observations.

Formula

σx̄w = σw / √(Σwᵢ)

Meaning

σx̄w = standard deviation of weighted mean; σw = weighted single-observation std dev; Σwᵢ = sum of all weights

Watch Out

Denominator is NOT √n; it is √(Σwᵢ). With unequal weights, use sum of weights, not count.

When To Use

Estimate precision of the final weighted-mean result.

Section Title

Weighted Mean & Unequal-Weight Observations

Important Facts

  • Higher weight observations have greater influence on weighted mean.
  • More reliable (lower σ) measurements pull the result toward their value.
  • Weighted mean always lies between minimum and maximum observation values.
  • Σ(wᵢ·vᵢ) ≈ 0 should hold for unweighted data as internal consistency check.
  • Standard deviation of weighted mean depends on Σwᵢ, not n.
  • Relative weights (scale factor) do NOT change the weighted mean value.
  • Weight assignment errors directly affect final result; double-check w = 1/σ² calculation.

Key Definitions

Term

Weighted Mean

Example

Two distance measurements: 100.02 m (σ=0.02) and 100.05 m (σ=0.01) → weighted mean pulls toward the more precise 100.05 m value

Definition

Best estimate of a quantity from observations with unequal reliability; gives higher influence to more precise measurements.

Diagrams To Know

  • Weighted mean visualization showing contribution of each observation
  • Weight distribution pie chart for typical network

Formulas

Formula

wᵢ = 1/Kᵢ (relative weights for leveling)

Meaning

wᵢ = relative weight; Kᵢ = distance of leveling route i in km

Watch Out

Use DISTANCE (path length), not elevation difference. Longer loops accumulate more random error.

When To Use

In spirit or trigonometric leveling networks, assign weights inversely to distance.

Formula

σleveling ≈ c·√K

Meaning

σ = standard deviation of level network; c = constant (depends on method); K = total route distance in km

Watch Out

Error grows as √K, NOT linearly with K. Doubling network length increases error by √2 ≈ 1.41, not 2.

When To Use

Estimate expected precision of leveling given total network distance; standard deviation grows with √K.

Section Title

Practical Leveling & Distance Measurement Applications

Important Facts

  • In leveling networks, shorter routes are inherently more precise due to fewer setup stations and less accumulated error.
  • Weight assignment: if three routes are 2 km, 1 km, and 4 km, relative weights are 1/2, 1/1, 1/4 = 0.5, 1.0, 0.25.
  • Standard deviation in leveling roughly proportional to √(distance); longer networks naturally have lower precision.
  • For Philippine leveling surveys (RA 8560), network design should account for distance-based weight distribution.
  • PRS92 datum implementation often uses multiple leveling routes; proper weighting is essential for adjustment.

Key Definitions

Term

Leveling Route Distance (K)

Example

A closed leveling loop from point A → B → C → A covering 2 + 1.5 + 1.5 = 5 km has K = 5 km

Definition

Total horizontal distance (in km) traveled along a leveling circuit; primary factor determining measurement precision.

Diagrams To Know

  • Leveling network diagram showing routes with distances and assigned weights
  • Weight reduction curve: w vs. distance (hyperbolic decay)

Section Title

Numerical Worked Examples (Board-Exam Style)

Important Facts

  • EXAMPLE 1 — Arithmetic mean and standard deviation: Five distance measurements are 100.01, 100.02, 100.03, 100.02, 100.02 m. Find mean and std dev. SOLUTION: x̄ = 500.10/5 = 100.02 m. Residuals: v = [−0.01, 0, +0.01, 0, 0]. Σv² = 0.0002. σ = √(0.0002/4) = √0.00005 = 0.00707 m ≈ 0.007 m.
  • EXAMPLE 2 — Precision improvement with replication: A measurement has σ = 0.024 m from a single observation. If measured 9 times, what is the standard deviation of the mean? SOLUTION: σₓ̄ = 0.024/√9 = 0.024/3 = 0.008 m. Precision improves by factor 3.
  • EXAMPLE 3 — Weighted mean with two observations: Distance measured twice: 100.02 m (σ = 0.02 m) and 100.05 m (σ = 0.01 m). Find weighted mean. SOLUTION: w₁ = 1/0.02² = 2,500; w₂ = 1/0.01² = 10,000. x̄w = (2,500 × 100.02 + 10,000 × 100.05) / 12,500 = (250,050 + 1,000,500) / 12,500 = 1,250,550 / 12,500 = 100.0440 m.
  • EXAMPLE 4 — Leveling weights by distance: Three level routes to a bench mark have lengths 3 km, 5 km, and 2 km. Assign relative weights. SOLUTION: w ∝ 1/K. w₁ = 1/3 ≈ 0.333; w₂ = 1/5 = 0.2; w₃ = 1/2 = 0.5. Normalize to integers: multiply by 6 → weights are 2, 1.2, 3. Or keep as 1/3, 1/5, 1/2.
  • EXAMPLE 5 — Standard deviation of weighted mean: Three observations with values 50.10, 50.14, 50.12 and weights 2, 3, 1. Find weighted mean and std dev of mean. SOLUTION: x̄w = (2×50.10 + 3×50.14 + 1×50.12)/(2+3+1) = (100.20 + 150.42 + 50.12)/6 = 300.74/6 = 50.1233 m. Residuals: v₁ = −0.0233, v₂ = +0.0167, v₃ = −0.0033. σw = √[(2×0.0233² + 3×0.0167² + 1×0.0033²)/(3−1)] = √[0.00109]/2 ≈ 0.0233. σx̄w = 0.0233/√6 ≈ 0.0095 m.

Must Remember

  • Weight w = 1/σ² (INVERSE of VARIANCE, not std dev). Never use 1/σ.
  • Arithmetic mean x̄ = Σx/n is the MPV for EQUAL-weight observations only.
  • Weighted mean x̄w = Σ(wᵢ·xᵢ)/Σwᵢ for UNEQUAL-weight observations (foundation of least squares).
  • Standard deviation σ = √(Σv²/(n−1))—use n−1, NOT n. Sample std dev, not population.
  • Precision improves by √n, NOT n. Adding 4 measurements reduces σₓ̄ by factor 2, not 4.
  • Leveling weight w ∝ 1/K (inverse distance); shorter route → higher weight → more reliable.
  • Residual sum: Σv = 0 for unweighted; Σ(wᵢ·vᵢ) ≈ 0 for weighted (internal check).
  • Standard deviation of mean: σₓ̄ = σ/√n (unweighted); σx̄w = σw/√(Σwᵢ) (weighted—use weight sum, not count).
  • Eliminate BLUNDERS and CORRECT SYSTEMATIC errors BEFORE adjustment; only RANDOM errors are handled by least squares.
  • Probable error PE = 0.6745σ—represents 50% confidence interval; memorize the constant 0.6745.

Last Minute Tips

  • Always double-check: Is the problem asking for a SINGLE-OBSERVATION std dev (σ) or the MEAN std dev (σₓ̄)? They differ by √n. Wrong choice = wrong answer.
  • For leveling problems: Weight w ∝ 1/DISTANCE. Shorter route = higher weight. Verify by logic: 1 km route should be more reliable (higher weight) than 5 km route.
  • Verify Σv ≈ 0 (unweighted) or Σ(wᵢ·vᵢ) ≈ 0 (weighted) after computing residuals—catches arithmetic errors before you finish.
  • Remember: n−1 in σ formula, not n. Using n is a common board exam trap and underestimates error significantly.
  • If given variance σ², convert to std dev first (σ = √(σ²)), then compute weights. Forgetting this step is a frequent mistake.

Comparison Tables

Rows

Values

  • Large (>3σ)
  • Random
  • Misreading, instrument failure
  • Detect & eliminate before adjustment
  • NO—reject observation

Property

Blunder

Values

  • Constant or gradual
  • Always same sign
  • Temperature, equipment bias
  • Model mathematically & correct
  • NO—correct first, then adjust

Property

Systematic

Values

  • Small (<3σ)
  • Mixed +/−
  • Inherent instrument/observer limit
  • Statistical adjustment (least squares)
  • YES—adjust using weights & MPV

Property

Random

Columns

  • Error Type
  • Magnitude
  • Sign Pattern
  • Cause
  • How to Handle
  • Use in Adjustment?

Table Title

Error Types: How to Identify & Handle

Rows

Values

  • x̄ = Σx/n
  • x̄w = Σ(wᵢ·xᵢ)/Σwᵢ

Property

Formula

Values

  • All observations equal precision
  • Observations have unequal precision

Property

When to use

Values

  • All equal (implicitly w = 1)
  • w = 1/σ² (explicit assignment)

Property

Weight basis

Values

  • Σv = 0 (always)
  • Σ(wᵢ·vᵢ) ≈ 0 (as check)

Property

Residual sum

Values

  • σₓ̄ = σ/√n
  • σx̄w = σw/√(Σwᵢ)

Property

Std dev of mean

Values

  • Equal (full 1/n share)
  • Reduced (low weight if poor precision)

Property

Influence of outlier

Columns

  • Aspect
  • Unweighted Mean
  • Weighted Mean

Table Title

Unweighted vs. Weighted Mean Comparison

Rows

Values

  • w = 1/σ²
  • w ∝ 1/σ² (inverse)
  • σ = 0.01 m → w = 10,000; σ = 0.02 m → w = 2,500

Property

From variance/precision

Values

  • w = 1/K (relative)
  • w ∝ 1/K (inverse)
  • K = 1 km → w = 1; K = 2 km → w = 0.5

Property

Leveling by distance

Values

  • w = n (relative)
  • w ∝ n (direct)
  • n = 3 repeats → w = 3; n = 1 → w = 1

Property

Repeated measurements

Values

  • w = n/σ² (or n/K)
  • w ∝ n; w ∝ 1/σ²
  • If obs repeated 4 times with σ = 0.02: w = 4/0.0004 = 10,000

Property

Combined rules

Columns

  • Situation
  • Weight Formula
  • Proportionality
  • Example

Table Title

Weight Assignment Rules Summary

Rows

Values

  • σ = √(Σv²/(n−1))
  • σw = √(Σ(wᵢ·vᵢ²)/(n−1))
  • Scatter of individual measurements
  • Use n−1, NOT n. One DoF lost fitting mean.

Property

Single observation

Values

  • σₓ̄ = σ/√n
  • σx̄w = σw/√(Σwᵢ)
  • Precision of final answer
  • Denominator in weighted case is √(Σwᵢ), not √n. Weight sum matters.

Property

Mean/MPV

Values

  • √n (always)
  • √(Σwᵢ) (for equal wᵢ = √n)
  • More measurements → √n× better precision
  • Not linear! Doubling n improves by √2 ≈ 1.41, not 2.

Property

Improvement factor

Columns

  • Statistic
  • Unweighted Formula
  • Weighted Formula
  • Interpretation
  • Board Exam Pitfall

Table Title

Standard Deviation Formulas: Single Observation vs. Mean

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