Introduction to NAVSTAR GPS Scott M. Haag, Rutgers Center for Remote Sensing and Spatial Analysis (Revised from Chuck Colvard and Joe Geib) Class Schedule ) Computer Login ) Questions from last week ) GPS error budget ) Geographic Information Systems ) ) ) ) ) ) ) ) ) ) ) ) ) ) Name Account New?? ===================================== Les Small small No Erica Cress ecress Yes Aaron Newland bcaapi Yes Brian Switek sandshrk Yes Dan Betz drbetz Yes Zeeshan Khan zkhan13 Yes York Bergin-Pugh ruhungry Yes David Bennet dbnett No David Gates gates No Aaron Love aalove No Anton Getz agetz No Keith Aubin kaubin Yes Questions from Last Week ) Knots and the Rope and how that works? ) A ships speed is determined in nautical miles. A nautical mile is equal to one minute of latitude. Since there are 360 degrees and 60 minutes in a degree, the earth is (360 * 60) or 21,600 knots in circumference. ) In order to determine speed a ship would throw a log tied to a rope off the side of the ship. Questions from Last Week ) This rope had a knot placed every 47 ft 3 inches. ) The amount of knots that were pulled in 30 second intervals was equal to the speed in knots per hour. This allowed the navigator to ) fix a dead reckoning position. ) Questions from Last Week ) How to see the North Star from the South Pole? ) Well you can’t do that but most early navigation took place in the northern hemisphere, and there are other celestial objects that can be used in the southern hemisphere. Questions from Last Week ) The equation to converting time to degrees longitude? ) It takes the earth 24 hours to completely turn around. This can be observed for earth because the sun’s zenith is separated by a period of 24 hours. Questions from Last Week The equation to So if an observer in New converting York has an accuratetime clockto showingdegrees the timelongitude? in London ) he-she could calculate the temporal difference between solar noon in London and New York City. This time difference can be converted to degrees longitude by the fact that it takes 24 hours for the earth to completely rotate and has 360 degrees of longitude. Therefore the sun appear to be moving at 360/24 or 15 degrees per hour. Questions from Last Week ) The equation to So if an observer in New converting time4to York records solar noon degrees longitude? hours later then in London. This observer would know that they are 15*4 or 60 degrees away from London. Also a navigator knows that as they move towards home port local noon will converge temporally with the home port. Questions from Last Week ) Link Between GPS and Time? / The mechanics of GPS? ) GPS works by determining the range from know positions (the satellites). ) In order to determine the range from a known position we need very accurate clocks because. y The Satellites are moving (not fixed). y GPS determines range by measuring how long it takes an electromagnetic signal to travel from the satellite to the ground receiver. ) ) ) ) GPS determines the precise position of the Satellites in space using an almanac which is downloaded from the satellites. To find the range to the satellites your GPS receiver uses something called a Pseudo Random Code. Each satellite is “singing” a unique PRC that is started at a specific time. By recording what time this song is heard at the GPS receiver we can determine how long it took for the electromagnetic signal to reach the earth. This Difference in time can then be multiplied times the speed of propagation of an electromagnetic signal (3.00 X 10 ^8 meters per second) to get the range to the satellite. Trilateration Knowing that we're 12,600 miles from a particular satellite narrows down all the possible locations we could be in the whole universe to the surface of a sphere that is centered on this satellite and has a radius of 12,600 miles. 12,600 miles We’re somewhere on the surface of this Sphere Trilateration A second measurement narrows our position down to the intersection of two spheres - an imaginary circle 12,600 miles 16,000 miles The intersection of two spheres is a circle Trilateration A third measurement narrows our possible position to just two points 12,600 miles Intersection of three spheres is only two points 16,000 miles 14,000 miles Trilateration Fourth measurement will decide between two points Fourth measurement will only go through one of the two points Questions from Last Week ) GPS Time Correction? ) Small time Errors cause huge positioning errors because electromagnetic signals move so fast. ) Pathfinder pocket (+-2 to 5 meters) ) Or 0.0000000067 seconds! Dealing with Clock Errors Suppose that there were 1 second errors in your receiver's clock - position calculation would be way off 5 seconds wrong time 7 seconds wrong time Our true position This diagram is a 2D analogy - GPS really works in a 3D world Bad position - receiver clock is off by one second =186,000 miles Dealing with Clock Errors ) With the addition of a third measurement the receiver recognizes the timing problem ) The receiver figures the error offset, sets its internal clock to the correct time (very near atomic accuracy) and calculates its true position ) In real world 3-D, this means using a 4th satellite to solve for clock errors. The clock error is the same for each satellite. Error Budget ) y y y y y ) Error Typical observed errors satellite clocks ephemeris error receiver errors atmospheric/iono S/A Total (rt sq sum) y y y y .8 m .8 m 1.2 m 4m 30 m 2 ft 2 feet 4 ft 12 ft 100 ft 5-7 m 15-30 ft Then multiply by GDOP (usu. 4-6) that gives a total error of: typical good receiver 20-50M 60-100 ft worst case 65 M 200 feet with S/A 120 M 350 feet S/A Atmos/Ionos Receiver Ephemeris Sat Clocks Feet Meters 0 0 50 100 17 33 More Geometry ) Satellite geometry matters ) Accuracy is best when SV’s are spread out overhead, not bunched together or down on the horizon Good Bad DOP ) Dilution of Precision ) A controllable source of error ) Can be predicted ) Two things influence DOP y Number of satellites in view (line of sight) y 3- dimensional Arrangements of satellites ) Has become less of a problem since more satellites have been placed in orbit Graphic from http://www.geosun.sjsu.edu/paula/137/pdf/lecture15.pdf DOP ) Different types of DOP y HDOP horizontal Dilution of Precision y VDOP is vertical dilution of Precision y PDOP Position dilution of Precision (combines HDOP and VDOP) y TDOP Time Dilution of Precision y GDOP geometric DOP is a combination of PDOP and TDOP Measured from high to low- we will come back to this! Low = 1 high = 8 Selective Availability ) ) ) As hard as it may be to believe, the same government that spent $12 billion to develop the most accurate navigation system in the world used to intentionally degrading its accuracy. The policy was called "Selective Availability" or "SA" DoD want to make sure that no hostile force or terrorist group can use GPS to make accurate weapons. Selective Availability ) ) ) DoD introduces some "noise" into the satellite's clock data which, in turn, adds noise (or inaccuracy) into position calculations DoD may also be sending slightly erroneous orbital data to the satellites which they transmit back to receivers on the ground as part of a status message. Together these factors used to make SA the biggest single source of inaccuracy in the system Selective Availability ) Military receivers use a separate signal on a different frequency along with a decryption key to remove the SA errors and so they're much more accurate (ten time more accurate) Selective Availability • Turned on in late March, 1990 (without notice) • Turned off on 10 Aug., 1990 for the Gulf war *not enough P-code receivers yet in U.S. military • Turned on again on 1 July, 1990war over. Turned off again for Panama, Grenada, and Haiti SA turned off ) President Clinton ordered Selective Availability turned off in July, 2000 ) Now even low-end units have much greater accuracy. ) The Federal Government now degrades GPS locally instead of globally using jamming technology.