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Field procedure of aerial photogrammetry, relief displacement

Short answer

Field procedure includes planning photo scale and overlaps, establishing signalised ground control, flying strips at constant height, processing images, plotting from stereo pairs, and field checking. Relief displacement d = r h / H is the radial image shift due to height, causing scale variation; it allows height measurement and stereoscopic parallax.

Describe the field procedure of aerial photogrammetry and relief displacement of photogrammetry.

Field procedure of aerial photogrammetry

  1. Planning: decide the purpose, scale and accuracy; choose the camera, flying height and overlaps (60 % end lap, 25–30 % side lap); prepare the flight plan.
  2. Ground control: establish horizontal and vertical control points (by traversing, levelling or GPS) that can be identified on the photos, and signalise them with targets before the flight.
  3. Photography: fly the strips at the planned height and speed in suitable weather; the camera exposes at fixed intervals.
  4. Processing: develop the film (or download digital images), prepare contact prints and a photo index.
  5. Photo-control identification and plotting: pass the control to the photos, orient the stereo pairs in a plotter, and draw the map or compute coordinates and contours.
  6. Field completion and checking: annotate names and features, check the map in the field.

Relief displacement

It is the radial shift of the image of a point on a vertical photo, due to its height hh above the datum. From similar triangles,

d=r hHd = \frac{r\,h}{H}

where rr is the radial distance of the image from the principal point and HH is the flying height above the datum. High points move outward from the principal point, low points move inward, and the displacement is zero at the principal point. Because of this, a photograph of undulating ground is not to scale and cannot be used as a map unless corrected (by rectification or orthophoto production). It also lets heights of objects be found: h=dH/rh = dH/r, and it gives the parallax needed for stereoscopic viewing.

✓ Answer checked by Claude Opus 5.5 (high effort)

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