Question 1
How are the P code and C/A code cycles characterized?
Correct Answer:
The P code repeats every 38 weeks, and each week is assigned to a different satellite
Explanation:
The P code is designed as a long, time-sharing sequence whose overall pattern stretches over many weeks. In this system, each week within a 38-week cycle is assigned to a different satellite, so the P-code signal for a given satellite is unique within that week but shifts with each successive week. After the full 38-week cycle, the pattern repeats, bringing the same weekly assignments back to the start. That’s why this option describes the P code cycle length accurately: a 38-week repetition with each week tied to a distinct satellite. In contrast, the civilian C/A code operates on a much shorter timescale, repeating its pseudorandom sequence very quickly, which is why receivers can acquire it rapidly. The key point for the P code’s behavior is the 38-week cycle with weekly satellite assignments, which is what makes the described option the best fit.
Question 2
For first-order geodetic control, the average triangle closure should be which value?
Correct Answer:
1.0 arcseconds
Explanation:
Triangle closure error is the difference between the sum of the measured angles in a triangle and the theoretical 180 degrees. In first-order geodetic control, angle measurements are extremely precise, and after adjustment the average angular misclosure per triangle is about 1 arcsecond. This tiny value shows the network is internally consistent and well tied to the reference frame. Larger misclosures, like a few arcseconds or more, would indicate less precision or issues needing re-measurement or re-adjustment. Therefore, the expected value for first-order control is around 1 arcsecond.
Question 3
What is the angular distance measured along the hour circle from the celestial equator to the celestial body?
Correct Answer:
Declination
Explanation:
Declination is the angular distance north or south of the celestial equator, measured along the hour circle that passes through the celestial body. This is exactly how far the object sits from the celestial equator on its vertical circle, with north being positive and south negative. Right ascension, on the other hand, is measured along the celestial equator from the vernal equinox to the object’s hour-angle crossing, not from the equator to the body along the hour circle. Polar distance is the angle from the celestial pole to the object (related by p = 90° − declination), and zenith distance is the angle from the observer’s zenith to the object (dependent on latitude and altitude). So the described angular distance corresponds to declination.
Question 4
In first-order geodetic control, the maximum triangle closure should not exceed how many arcseconds?
Correct Answer:
3 arcseconds
Explanation:
In first-order geodetic control, you aim for extremely small angular inconsistencies in each triangle of the network. The triangle closure, or angular misclosure, is how far the measured angles deviate from summing to exactly 180 degrees. Since arcseconds are a tiny angular unit (one arcsecond is 1/3600 of a degree), keeping misclosure to a few arcseconds ensures the network is internally consistent enough to be reliable after adjustment. The commonly accepted limit for a first-order network is about 3 arcseconds. This threshold balances practicality with precision: it’s tight enough to maintain high accuracy, but not so strict that routine measurements would be repeatedly flagged as errors. If a triangle shows a larger misclosure, it indicates problematic measurements or geometry and typically triggers re-measurement or re-observation. Choices requiring much smaller limits (like 0.5 or 1 arcsecond) are more stringent than standard for first-order, while a threshold as large as 10 arcseconds would be too lax for keeping the network trustworthy.
Question 5
What is the term for the difference in direction between Earth's gravity vector and a reference direction such as the normal to a reference ellipsoid?
Correct Answer:
Deflection of the vertical
Explanation:
The term describes the angular difference between the direction of local gravity (the true vertical) and the normal to the reference ellipsoid. Because the gravity field is influenced by rotation and local mass variations, the plumb line does not line up perfectly with the ellipsoid’s normal. This misalignment is the deflection of the vertical, often with two components in the meridian (north-south) and prime-vertical (east-west) directions. The other terms refer to magnetic directions or directions in the horizontal plane, not to the difference between gravity and the ellipsoid normal.
Question 1
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About this Exam

Prepare with the Geodesy Refresher Practice Exam practice quiz. This question bank includes 10 questions covering geodetic, celestial, direction, code, and first-order. Use it to review important concepts, identify knowledge gaps, and build confidence for the related exam, course, or assessment.

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Geodesy Refresher Practice Exam

This practice set contains 10 questions from the matching question bank and focuses on geodetic, celestial, direction, code, and first-order. Work through each question carefully, review the provided solutions, and revisit topics that need more study before your next attempt.

This is an independent study resource intended for practice and review; it is not an official examination or an endorsement by any organization named in the title.

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