Portal:Geodesy

Image 1Datum shift between NAD27 and NAD83, in metres (from Geodesy)

Image 2Plot of latitude versus tangential speed. The dashed line shows the Kennedy Space Center example. The dot-dash line denotes typical airliner cruise speed. (from Earth's rotation)

Image 3A medieval depiction of the Ecumene (1482, Johannes Schnitzer, engraver), constructed after the coordinates in Ptolemy's Geography and using his second map projection. The translation into Latin and dissemination of Geography in Europe, in the beginning of the 15th century, marked the rebirth of scientific cartography, after more than a millennium of stagnation. (from Cartography)

Image 4Geodetic control mark (from Geodesy)

Image 5Earth's gravity measured by NASA GRACE mission, showing deviations from the theoretical gravity of an idealized, smooth Earth, the so-called Earth ellipsoid. Red shows the areas where gravity is stronger than the smooth, standard value, and blue reveals areas where gravity is weaker. (Animated version.) (from Gravity of Earth)

Image 6Starry circles arc around the south celestial pole, seen overhead at ESO's La Silla Observatory. (from Earth's rotation)

Image 7Initial acquisition of GPS signal in 2D (from Geodesy)

Image 8How very-long-baseline interferometry (VLBI) works (from Geodesy)

Image 9Geoid, an approximation for the shape of the Earth; shown here with vertical exaggeration (10000 vertical scaling factor). (from Geodesy)

Image 10Navigation device, Apollo program (from Geodesy)

Image 11A pre-Mercator nautical chart of 1571, from Portuguese cartographer Fernão Vaz Dourado (c. 1520 – c. 1580). It belongs to the so-called plane chart model, where observed latitudes and magnetic directions are plotted directly into the plane, with a constant scale, as if the Earth were a plane (Portuguese National Archives of Torre do Tombo, Lisbon). (from Cartography)

Image 12Variations in the gravity field of the Moon, from NASA (from Geodesy)

Image 13A plumb bob determines the local vertical direction (from Gravity of Earth)

Image 14Height measurement using satellite altimetry (from Geodesy)

Image 15Axial tilt (or Obliquity), rotation axis, plane of orbit, celestial equator and ecliptic. Earth is shown as viewed from the Sun; the orbit direction is counter-clockwise (to the left). (from Geodesy)

Image 16Topographic map of Easter Island (from Cartography)

Image 17The cartographic process (from Cartography)

Image 18The Bedolina Map and its tracing, 6th–4th century BCE (from Cartography)

Image 19Global gravity anomaly animation over oceans from the NASA's GRACE (Gravity Recovery and Climate Experiment) (from Geodesy)

Image 20Areal distortion caused by Mercator projection (from Cartography)

Image 21Earth's axial tilt is about 23.4°. It oscillates between 22.1° and 24.5° on a 41,000-year cycle and is currently decreasing. (from Earth's rotation)

Image 22A simulated history of Earth's day length, depicting a resonant-stabilizing event throughout the Precambrian era (from Earth's rotation)

Image 23On a prograde planet like Earth, the stellar day is shorter than the solar day. At time 1, the Sun and a certain distant star are both overhead. At time 2, the planet has rotated 360 degrees and the distant star is overhead again but the Sun is not (1→2 = one stellar day). It is not until a little later, at time 3, that the Sun is overhead again (1→3 = one solar day). (from Earth's rotation)

Image 24Earth's rotation imaged by Deep Space Climate Observatory, showing axis tilt (from Earth's rotation)

Image 25A Munich archive with lithography plates of maps of Bavaria (from Geodesy)

Image 26Small section of an orienteering map (from Cartography)

Image 272D grid for elliptical coordinates (from Geodesy)

Image 28A modern instrument for geodetic measurements using satellites (from Geodesy)

Image 29Deviation of day length from SI-based day (from Earth's rotation)

Image 30Gravity measurement devices, pendulum (left) and absolute gravimeter (right) (from Geodesy)

Image 31Relief map Sierra Nevada (from Cartography)

Image 32Illustrated map (from Cartography)

Image 33A relative gravimeter (from Geodesy)

Image 34A 14th-century Byzantine map of the British Isles from a manuscript of Ptolemy's Geography, using Greek numerals for its graticule: 52–63°N of the equator and 6–33°E from Ptolemy's Prime Meridian at the Fortunate Isles. (from Cartography)

Image 35GPS Block IIA satellite orbits over the Earth. (from Geodesy)

Image 36Visual fix by three bearings plotted on a nautical chart (from Geopositioning)

Image 37An artist's rendering of the protoplanetary disk (from Earth's rotation)

Image 38Global plate tectonic movement using GPS (from Geodesy)

Image 39Equatorial (a), polar (b) and mean Earth radii as defined in the 1984 World Geodetic System (from Geodesy)

Image 40Gravity at different internal layers of Earth (1 = continental crust, 2 = oceanic crust, 3 = upper mantle, 4 = lower mantle, 5+6 = core, A = crust-mantle boundary) (from Gravity of Earth)

Image 41The definition of latitude (φ) and longitude (λ) on an ellipsoid of revolution (or spheroid). The graticule spacing is 10 degrees. The latitude is defined as the angle between the normal to the ellipsoid and the equatorial plane. (from Geodesy)

Image 42A map of recent volcanic activity and ridge spreading. The areas where NASA GRACE measured gravity to be stronger than the theoretical gravity have a strong correlation with the positions of the volcanic activity and ridge spreading. (from Gravity of Earth)

Image 43Ellipsoid - a mathematical representation of the Earth. When mapping in geodetic coordinates, a latitude circle forms a truncated cone. (from Geodesy)

Image 44Principles of geolocation using GPS (from Geopositioning)

Image 45Copy (1472) of St. Isidore's TO map of the world. (from Cartography)

Image 46The Tabula Rogeriana, drawn by Muhammad al-Idrisi for Roger II of Sicily in 1154. South is at the top. (from Cartography)

Image 47Europa regina in Sebastian Münster's "Cosmographia", 1570 (from Cartography)

Image 48This long-exposure photo of the northern night sky above the Nepali Himalayas shows the apparent paths of the stars as Earth rotates. (from Earth's rotation)

Image 49Valcamonica rock art (I), Paspardo r. 29, topographic composition, 4th millennium BCE (from Cartography)

Image 50Mapping can be done with GPS and laser rangefinder directly in the field. Image shows mapping of forest structure (position of trees, dead wood and canopy). (from Cartography)