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Argos. 2005. General information to info@argosinc.com Customer support to DUS, at www.argosinc.com/documents. From the menu list select sysdesc.pdf Brown, M. P., Jr. (Ed.). 1981. Compendium of Communication and Broadcast Satellites 1958 to 1980. IEEE Press, New York. Cospas-Sarsat, at http://www.cospas-sarsat.org/ Cospas-Sarsat, at http://www.cospas-sarsat.org/Beacons/406Bcns.htm Cospas-Sarsat, at http://www.cospas-sarsat.org/Status/spaceSegmentStatus.htm Cospas-Sarsat, at http://www.equipped.com/cospas-sarsat_overview.htm Cospas-Sarsat. 1994a. System Data No. 17, February. Cospas-Sarsat. 1994b. Information Bulletin No. 8, February. Cospas-Sarsat. 2004. Information Bulletin No.17, November, at http://www.cospassarsat.org FCC. 1983. Licensing of Space Stations in the Domestic Fixed-Satellite Service and Related Revisions of Part 25 of the Rules and Regulations, Report 83-184 33206, CC Docket 81-184. Federal Communications Commission, Washington, DC. FCC. 1997 Assignment of Orbital Locations to Space Stations in the Ka-Band. Adopted May 8, 1997, released May 9, at http://www.fcc.gov/Bureaus/International/ Orders/1997/da970967.txt FCC. 1996. Orbital Assignment Plan, at http://www.fcc.gov/Bureaus/International/ Orders/1996/da960713.txt Government of Canada. 1983. Direct-to-Home Satellite Broadcasting for Canada. IEEE Spectrum, March. Information Services, Department of Communications. Intelsat, at http://www.intelsat.com/ Lilly, C. J. 1990. INTELSAT s New Generation. IEE Review, Vol. 36, No. 3, March. NOAA, at http://www.ipo.noaa.gov/
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Pritchard, W. L. 1984. The History and Future of Commercial Satellite Communications. IEEE Commun. Mag., Vol. 22, No. 5, May, pp. 22 37. Reinhart, E. E. 1990. Satellite Broadcasting and Distribution in the United States. Telecommun. J., Vol. 57, No. V1, June, pp. 407 418. Sachdev, D. K., P. Nadkarni, P. Neyret, L. R. Dest, K. Betaharon, and W. J. English. 1990. INTELSAT V11: A Flexible Spacecraft for the 1990s and Beyond. Proc. IEEE, Vol. 78, No. 7, July, pp. 1057 1074. Scales, W. C., and R. Swanson. 1984. Air and Sea Rescue via Satellite Systems. IEEE Spectrum, March, pp. 48 52.
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2.1 Introduction Satellites (spacecraft) orbiting the earth follow the same laws that govern the motion of the planets around the sun. From early times much has been learned about planetary motion through careful observations. Johannes Kepler (1571 1630) was able to derive empirically three laws describing planetary motion. Later, in 1665, Sir Isaac Newton (1642 1727) derived Kepler s laws from his own laws of mechanics and developed the theory of gravitation [for very readable accounts of much of the work of these two great men, see Arons (1965) and Bate et al. (1971)]. Kepler s laws apply quite generally to any two bodies in space which interact through gravitation. The more massive of the two bodies is referred to as the primary, the other, the secondary or satellite. 2.2 Kepler s First Law Kepler s first law states that the path followed by a satellite around the primary will be an ellipse. An ellipse has two focal points shown as F1 and F2 in Fig. 2.1. The center of mass of the two-body system, termed the barycenter, is always centered on one of the foci. In our specific case, because of the enormous difference between the masses of the earth and the satellite, the center of mass coincides with the center of the earth, which is therefore always at one of the foci. The semimajor axis of the ellipse is denoted by a, and the semiminor axis, by b. The eccentricity e is given by e 2a2 a b2 (2.1)
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Figure 2.1 The foci F1 and F2, the semimajor axis a, and the semiminor axis b of an ellipse.
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The eccentricity and the semimajor axis are two of the orbital parameters specified for satellites (spacecraft) orbiting the earth. For an elliptical orbit, 0 e 1. When e 0, the orbit becomes circular. The geometrical significance of eccentricity, along with some of the other geometrical properties of the ellipse, is developed in App. B.
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2.3 Kepler s Second Law Kepler s second law states that, for equal time intervals, a satellite will sweep out equal areas in its orbital plane, focused at the barycenter. Referring to Fig. 2.2, assuming the satellite travels distances S1 and S2 meters in 1 s, then the areas A1 and A2 will be equal. The average velocity in each case is S1 and S2 m/s, and because of the equal area law, it follows that the velocity at S2 is less than that at S1. An important
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