Path: news.ccsf.jp!tomockey.ddo.jp!border1.nntp.dca.giganews.com!nntp.giganews.com!newsfeed00.sul.t-online.de!t-online.de!feeder.news-service.com!newsfeed.xs4all.nl!newsfeed5.news.xs4all.nl!xs4all!post.news.xs4all.nl!not-for-mail Date: Tue, 24 Feb 2009 05:16:45 +0100 From: "\\frac{1}{R}\\sqrt{\\frac{L}{C}}" User-Agent: Thunderbird 2.0.0.19 (Windows/20081209) MIME-Version: 1.0 Newsgroups: alt.math,japan.sci.math,sci.math,sci.physics,sci.physics.relativity Subject: Re: GPS question References: <1faf92f1-847e-41c9-b6eb-09556cdeb0bc@t3g2000yqa.googlegroups.com> <3ca62bde-fb58-49a6-bd99-9614b9fbe589@a12g2000yqm.googlegroups.com> In-Reply-To: <3ca62bde-fb58-49a6-bd99-9614b9fbe589@a12g2000yqm.googlegroups.com> Content-Type: text/plain; charset=windows-1252 Content-Transfer-Encoding: 8bit Lines: 58 Message-ID: <49a37493$0$192$e4fe514c@news.xs4all.nl> NNTP-Posting-Host: 80.100.69.254 X-Trace: 1235448979 news.xs4all.nl 192 [::ffff:80.100.69.254]:34674 X-Complaints-To: abuse@xs4all.nl Xref: news.ccsf.jp japan.sci.math:207 koobee.wublee@gmail.com wrote: > On Feb 23, 11:09 am, PD wrote: >> On Feb 23, 12:49 pm, koobee.wub...@gmail.com wrote: > >>> You need four satellites where each satellite should know its time and >>> position. Time can just be a counter with all the satellites >>> synchronized to within a count of each other. Each satellite then >>> just broadcast its time and position information as almanac signal to >>> whoever wants to receive it. >>> Since the distance is traveled by light with a known speed, you can >>> then easily form a set of four equations with four unknowns. The four >>> unknowns are your time (relative to the counter in each satellite) and >>> position. >>> ** c^2 (t1 – t)^2 = (x1 – x)^2 + (y1 – y)^2 + (z1 – z)^2 >>> ** c^2 (t2 – t)^2 = (x2 – x)^2 + (y2 – y)^2 + (z2 – z)^2 >>> ** c^2 (t3 – t)^2 = (x3 – x)^2 + (y3 – y)^2 + (z3 – z)^2 >>> ** c^2 (t4 – t)^2 = (x4 – x)^2 + (y4 – y)^2 + (z4 – z)^2 >>> Where >>> ** (t1, x1, y1, z1) = Time and position of satellite 1 >>> ** (t2, x2, y2, z2) = Time and position of satellite 2 >>> ** (t3, x3, y3, z3) = Time and position of satellite 3 >>> ** (t4, x4, y4, z4) = Time and position of satellite 4 >>> ** (t, x, y, z) = Time and position of the receiver >>> Notice that relativistic effect is never needed. >> Except that t1, t2, t3, and t4 are Earth-referenced times, not the >> native time of the clocks on the satellites, which are t1', t2', t3', >> t4'. To get from t1', t2', t3', t4' to t1, t2, t3, t4, the satellites >> have programmed in a correction that comes from understanding >> relativistic effects. > > There are two ways to synchronize t1, t2, t3, and t4. Ground- > satellite synchronization introduces much more errors than satellite- > satellite synchronization. The latter does not have the ionosphere > and other atmospheric anomalies to consider. That latter also does > not have high speed to worry about since all satellites are either at > rest or moving very slowly relative to each other. > > For precision GPS design, one must use the satellite-satellite > synchronization. In doing so, there is no relativistic correction > needed in the design. > > You don't need satellite to satellite synchronization in GPS, although the newer satellites have this capability (block III i think they are called, these guys could operate independently for a while) Since the 70's any single GPS satellite in orbit is tracked with a few stations on ground forming a ground segment. In this way you get the orbit of the satellite, a master oscillator at just one tracking station is good enough to synchronize all satellite clocks to the same time system. Q -- CO2 at 390 ppm and counting, put a tiger in your tank -- ESSO commercial