🇮🇳 GATE Geomatics Engineering · subject

GATE Geomatics Engineering Common Syllabus

The Common syllabus for GATE Geomatics Engineering in full: 4 chapters, 25 topics and 18 sub-topics, every one listed below, plus 50 Common flashcards with answers.

4Chapters
25Topics
18Sub-topics
50Flashcards

Common syllabus: all 4 chapters

Expand any chapter to see its topics and sub-topics.

  1. Engineering Mathematics

    7 topics
    • Surveying measurements
      • Accuracy
      • Precision
      • Most probable value
    • Errors and their adjustments
    • Regression analysis
    • Correlation coefficient
    • Least square adjustment
    • Statistical significant value
    • Chi square test
  2. Remote Sensing

    6 topics
    • Basic concept
    • Electromagnetic spectrum
    • Spectral signature
    • Resolutions
      • Spectral
      • Spatial
      • Temporal
      • Radiometric
    • Platforms and Sensors
    • Remote Sensing Data Products
      • PAN
      • Multispectral
      • Microwave
      • Thermal
      • Hyperspectral
      • Visual and digital interpretation methods
  3. GNSS

    5 topics
    • Principle used
    • Components of GNSS
    • Data collection methods
    • DGPS
    • Errors in observations and corrections
  4. GIS

    7 topics
    • Introduction
    • Data Sources
    • Data Models and Data Structures
    • Algorithms
    • DBMS
    • Creation of Databases (spatial and non-spatial)
    • Spatial analysis
      • Interpolation
      • Buffer
      • Overlay
      • Terrain Modeling
      • Network analysis

GATE Geomatics Engineering Common flashcards — 50 questions with answers

  1. What is the fundamental purpose of taking surveying measurements, and why are they never exact?

    Surveying measurements quantify distances, angles, and elevations to determine relative positions of points. They are never exact because every measurement is affected by instrumental imperfections, human limitations, and environmental conditions, so each contains some error.

  2. Define 'accuracy' in the context of surveying measurements.

    Accuracy is the degree of closeness (conformity) of a measured value to its true value. High accuracy means small total error (small deviation from the truth).

  3. Define 'precision' in surveying.

    Precision is the degree of closeness or repeatability among a set of repeated measurements of the same quantity. It reflects the refinement/consistency of the measurements, independent of the true value.

  4. Compare accuracy and precision: can a measurement set be precise but not accurate?

    Yes. Precision = repeatability (small spread); accuracy = closeness to truth. A set can be tightly clustered (precise) yet systematically offset from the true value (inaccurate). High accuracy requires both small random spread and absence of systematic error.

  5. What is the 'most probable value' (MPV) of a quantity measured repeatedly with equal weight?

    The most probable value is the value with the greatest likelihood of being closest to the true value. For equally weighted direct observations it is the arithmetic mean: $$\text{MPV} = \bar{x} = \frac{\sum_{i=1}^{n} x_i}{n}$$

  6. How is the most probable value computed for weighted observations?

    It is the weighted mean: $$\text{MPV} = \frac{\sum w_i x_i}{\sum w_i}$$ where $w_i$ is the weight assigned to observation $x_i$.

  7. Define 'residual' (deviation) in measurement adjustment.

    A residual is the difference between an individual observation and the most probable value: $v_i = x_i - \bar{x}$. It is an estimate of the error and the sum of residuals about the mean is zero, $\sum v_i = 0$.

  8. What are the three main classes of errors in surveying?

    (1) Gross errors (mistakes/blunders) due to carelessness; (2) Systematic (cumulative) errors that follow a physical law and have consistent sign/magnitude; (3) Random (accidental) errors that remain after blunders and systematic errors are removed.

  9. How do systematic errors differ from random errors in behaviour and treatment?

    Systematic errors are predictable, follow a definite law, accumulate, and have a consistent sign — they can be computed and corrected/eliminated. Random errors are unpredictable in sign and magnitude, follow the normal distribution, tend to cancel, and are treated statistically (cannot be removed, only minimized).

  10. Why are only random errors handled by the theory of errors / least squares?

    Because blunders are detected and removed and systematic errors are eliminated by calibration/correction beforehand. The remaining residual random errors obey the normal (Gaussian) probability law, which underlies least-squares adjustment.

  11. State the laws (axioms) of accidental (random) errors.

    (1) Small errors occur more frequently than large errors; (2) Positive and negative errors of the same magnitude are equally likely; (3) Very large (extreme) errors do not occur (they are blunders). This produces the symmetric bell-shaped normal distribution.

  12. What is the standard deviation $\sigma$ of a set of measurements, and what does it represent?

    It is a measure of dispersion (precision) about the mean: $$\sigma = \sqrt{\frac{\sum v_i^{2}}{n-1}}$$ where $v_i$ are residuals and $n$ the number of observations. Smaller $\sigma$ indicates higher precision.

  13. What is the standard error (standard deviation) of the mean?

    $$\sigma_{\bar{x}} = \frac{\sigma}{\sqrt{n}}$$ It expresses the precision of the most probable value (mean); it decreases as the number of observations $n$ increases.

  14. Define the 'probable error' of a single observation and the constant used.

    The probable error is the magnitude of error such that there is a 50% chance the true error is smaller. For a single observation: $$E_s = 0.6745\,\sigma = 0.6745\sqrt{\frac{\sum v^{2}}{n-1}}$$

  15. How are weights related to the standard error of observations?

    Weight is inversely proportional to the square of the standard error (variance): $$w_i \propto \frac{1}{\sigma_i^{2}}$$ A more precise observation (smaller $\sigma$) receives a larger weight.

  16. State the principle of least squares used in measurement adjustment.

    The most probable values of observed quantities are those that make the sum of the weighted squares of the residuals a minimum: $$\sum w_i v_i^{2} = \text{minimum}$$ For equal weights, $\sum v_i^{2}$ is minimized.

  17. What is the objective of least square adjustment in a redundant survey network?

    To find a unique, statistically optimal set of corrected (adjusted) values that satisfies all geometric conditions when there are more observations than unknowns (redundancy), by minimizing $\sum w v^{2}$. It yields the most probable values and their precision estimates.

  18. In least squares, what is meant by 'degrees of freedom' (redundancy)?

    Degrees of freedom = number of observations minus number of unknowns ($r = n - u$). It is the number of redundant measurements available to check and adjust the network; redundancy enables error detection and statistical adjustment.

  19. Define regression analysis and what it determines.

    Regression analysis is a statistical method that establishes a functional (mathematical) relationship between a dependent variable and one or more independent variables, allowing prediction of the dependent variable. It fits a best line/curve (often by least squares) through the data.

  20. Write the equation of a simple linear regression line of $y$ on $x$ and identify the terms.

    $$y = a + bx$$ where $b$ is the regression coefficient (slope) and $a$ is the intercept. They are found by least squares: $b = \frac{\sum(x-\bar{x})(y-\bar{y})}{\sum(x-\bar{x})^{2}}$ and $a = \bar{y} - b\bar{x}$.

Show the other 30 Common flashcards
  1. What does the regression coefficient $b$ of $y$ on $x$ physically represent?

    It is the slope — the average change in the dependent variable $y$ per unit change in the independent variable $x$: $$b_{yx} = \frac{\text{Cov}(x,y)}{\sigma_x^{2}} = r\frac{\sigma_y}{\sigma_x}$$

  2. Define the correlation coefficient $r$ and give its formula.

    The (Pearson) correlation coefficient measures the strength and direction of the linear relationship between two variables: $$r = \frac{\sum (x-\bar{x})(y-\bar{y})}{\sqrt{\sum (x-\bar{x})^{2}\,\sum (y-\bar{y})^{2}}} = \frac{\text{Cov}(x,y)}{\sigma_x \sigma_y}$$

  3. What is the range of the correlation coefficient and how is each extreme interpreted?

    $-1 \leq r \leq +1$. $r = +1$ perfect positive linear correlation; $r = -1$ perfect negative linear correlation; $r = 0$ no linear correlation. Values near $\pm 1$ indicate strong linear association.

  4. What is the relationship between the correlation coefficient and the two regression coefficients?

    The correlation coefficient is the geometric mean of the two regression coefficients: $$r = \pm\sqrt{b_{yx}\cdot b_{xy}}$$ The sign of $r$ matches the (common) sign of the regression coefficients.

  5. What does the coefficient of determination $r^{2}$ represent?

    $r^{2}$ is the proportion of the total variance in the dependent variable that is explained by the regression (the independent variable). E.g., $r^{2}=0.81$ means 81% of the variation in $y$ is accounted for by $x$.

  6. Distinguish correlation from regression.

    Correlation measures the degree/strength of mutual linear association between two variables (symmetric, a single coefficient $r$). Regression establishes a cause-effect predictive equation of one variable on another (asymmetric; $b_{yx} \neq b_{xy}$ in general) and is used for estimation/prediction.

  7. What is a 'statistically significant value' (statistical significance)?

    It is a result judged unlikely to have occurred by random chance alone, evaluated against a chosen significance level $\alpha$ (e.g., 0.05 or 5%). If the test statistic's probability ($p$-value) is less than $\alpha$, the result is statistically significant and the null hypothesis is rejected.

  8. Define the significance level $\alpha$ and the confidence level in hypothesis testing.

    $\alpha$ is the probability of rejecting a true null hypothesis (Type I error), commonly 5% or 1%. The confidence level is $1-\alpha$ (e.g., 95% or 99%), the probability that the conclusion is correct.

  9. State the purpose of the Chi-square ($\chi^{2}$) test.

    The Chi-square test is a non-parametric test used to (i) test goodness-of-fit between observed and expected (theoretical) frequencies, and (ii) test independence/association between categorical variables. In surveying it tests whether observed errors follow the assumed (e.g., normal) distribution and checks variance.

  10. Write the Chi-square goodness-of-fit statistic and define its terms.

    $$\chi^{2} = \sum_{i=1}^{k} \frac{(O_i - E_i)^{2}}{E_i}$$ where $O_i$ = observed frequency, $E_i$ = expected frequency, and $k$ = number of categories. A small $\chi^{2}$ indicates good agreement with the expected distribution.

  11. How are degrees of freedom found for a Chi-square goodness-of-fit test with $k$ classes?

    Degrees of freedom $= k - 1 - m$, where $k$ is the number of categories and $m$ is the number of parameters estimated from the data. For a simple goodness-of-fit with no estimated parameters, $\text{df} = k-1$.

  12. How is the Chi-square test decision made using critical values?

    Compare the computed $\chi^{2}$ with the tabulated critical value $\chi^{2}_{\alpha,\,df}$. If $\chi^{2}_{\text{calc}} > \chi^{2}_{\text{critical}}$, reject the null hypothesis (significant difference); otherwise accept it (observed agrees with expected).

  13. What is the basic concept of remote sensing?

    Remote sensing is the science of acquiring information about an object, area, or phenomenon through the analysis of data obtained by a sensor that is not in physical contact with the target — typically by measuring reflected or emitted electromagnetic radiation.

  14. List the basic components/stages of a remote sensing system.

    (1) Energy source/illumination, (2) radiation and the atmosphere, (3) interaction with the target, (4) recording of energy by the sensor, (5) transmission, reception and processing, (6) interpretation and analysis, and (7) application of the information.

  15. Differentiate active and passive remote sensing.

    Passive sensors record natural energy (e.g., reflected sunlight or emitted thermal radiation) and depend on an external source. Active sensors supply their own energy, emit a pulse, and record the reflected/backscattered return (e.g., RADAR, LiDAR), and can operate day or night.

  16. What is the electromagnetic spectrum?

    The electromagnetic spectrum is the continuous, ordered range of all electromagnetic radiation arranged by wavelength (or frequency), from short-wavelength gamma rays and X-rays through ultraviolet, visible, infrared, microwave, to long-wavelength radio waves.

  17. Give the relationship between the speed of light, wavelength, and frequency of EM radiation.

    $$c = \lambda \nu$$ where $c \approx 3\times 10^{8}\ \text{m/s}$ is the speed of light in vacuum, $\lambda$ is wavelength, and $\nu$ is frequency. Wavelength and frequency are inversely related.

  18. State the approximate wavelength range of the visible portion of the spectrum and its colour limits.

    The visible region spans approximately $0.4$ to $0.7\ \mu\text{m}$ (400–700 nm), from violet/blue (~0.4 μm) through green and to red (~0.7 μm).

  19. List the principal spectral regions used in optical remote sensing with approximate ranges.

    Visible: $0.4$–$0.7\ \mu\text{m}$; Near-infrared (NIR): $0.7$–$1.3\ \mu\text{m}$; Shortwave/Mid-IR (SWIR): $1.3$–$3\ \mu\text{m}$; Thermal IR: $3$–$14\ \mu\text{m}$; Microwave: $1\ \text{mm}$–$1\ \text{m}$.

  20. What are 'atmospheric windows' in remote sensing?

    Atmospheric windows are wavelength ranges where the atmosphere is relatively transparent and transmits electromagnetic radiation with little absorption (e.g., visible and certain IR/microwave bands). Sensors are designed to operate within these windows.

  21. Define 'spectral signature'.

    A spectral signature is the characteristic pattern of reflectance (and/or emittance) of a feature as a function of wavelength. Each material — vegetation, water, soil — reflects, absorbs, and emits EM energy uniquely, allowing its identification from remote sensing data.

  22. Describe the typical spectral reflectance behaviour of healthy green vegetation.

    Low reflectance in blue and red (chlorophyll absorption), a small peak in green (hence green appearance), a sharp 'red edge' rise, and high reflectance in the near-infrared (due to leaf internal/mesophyll structure). This high NIR–low red contrast underlies vegetation indices like NDVI.

  23. How does the spectral reflectance of clear water typically behave?

    Water reflects in the blue-green region but absorbs strongly in the near-infrared and beyond, so it appears very dark (near-zero reflectance) in NIR bands. This makes NIR effective for delineating water bodies.

  24. What are the four types of resolution in remote sensing?

    Spatial resolution, spectral resolution, radiometric resolution, and temporal resolution.

  25. Define 'spatial resolution'.

    Spatial resolution is the smallest ground area (size of one pixel / ground sample distance) that a sensor can distinguish — the level of spatial detail. A smaller pixel (e.g., 1 m) means higher spatial resolution; a larger pixel (e.g., 1 km) means coarser detail.

  26. Define 'spectral resolution'.

    Spectral resolution is the ability of a sensor to distinguish fine wavelength intervals — defined by the number and narrowness (bandwidth) of the spectral bands. More, narrower bands (e.g., hyperspectral) give higher spectral resolution and better material discrimination.

  27. Define 'radiometric resolution'.

    Radiometric resolution is the sensitivity of a sensor to differences in signal strength — the number of brightness/grey levels it can record, expressed in bits. An $n$-bit sensor records $2^{n}$ levels (e.g., 8-bit = 256 levels); higher bit depth means finer radiometric resolution.

  28. Define 'temporal resolution'.

    Temporal resolution is the revisit time — the frequency with which a sensor images the same area (e.g., every 16 days). High (fine) temporal resolution means more frequent coverage, important for monitoring dynamic phenomena and change detection.

  29. Explain the typical trade-off between spatial and spectral/temporal resolution.

    Sensor design involves trade-offs: increasing spatial resolution (smaller pixels) reduces the energy per pixel, often forcing wider bands (lower spectral resolution) or a narrower swath that lengthens revisit time (lower temporal resolution). High spatial detail and high temporal frequency usually cannot be maximized simultaneously.

  30. How does radiometric resolution affect an image's appearance and information content?

    Higher radiometric resolution (more bits/grey levels) lets the sensor record finer differences in reflected/emitted energy, producing images that show subtle tonal variations and contrast. Low radiometric resolution gives few grey levels and a coarse, contrast-limited image.

GATE Geomatics Engineering Common FAQ

What is in the GATE Geomatics Engineering Common syllabus?

GATE Geomatics Engineering Common is split into 4 chapters: Engineering Mathematics, Remote Sensing, GNSS and GIS. Together they contain 25 topics and 18 sub-topics.

How many chapters are in GATE Geomatics Engineering Common?

4 chapters, containing 25 topics and 18 sub-topics. The largest chapter is Engineering Mathematics, with 7 topics.

Are there flashcards for GATE Geomatics Engineering Common?

Yes — a 50-card Common deck, printed in full in the flashcards section of this page and available in the Examius app with spaced repetition. The free plan covers one exam of your choice, including its flashcards; Examius Pro, a one-time purchase, unlocks every other exam and deck.