Page 92 - Satellite Communications, Fourth Edition
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72   Chapter Two

                              2.12.  Explain what is meant by the ascending and descending nodes. In what
                              units would these be measured, and in general, would you expect them to change
                              with time?
                              2.13.  Explain what is meant by (a) line of apsides and (b) line of nodes. Is it
                              possible for these two lines to be coincident?

                              2.14.  With the aid of a neat sketch, explain what is meant by each of the
                              angles: inclination; argument of perigee; right ascension of the ascending node.
                              Which of these angles would you expect, in general, to change with time?

                              2.15. The inclination of an orbit is 67°. What is the greatest latitude, north and
                              south, reached by the subsatellite point? Is this orbit retrograde or prograde?
                              2.16.  Describe briefly the main effects of the earth’s equatorial bulge on a
                              satellite orbit. Given that a satellite is in a circular equatorial orbit for which
                              the semimajor axis is equal to 42,165 km, calculate (a) the mean motion, (b) the
                              rate of regression of the nodes, and (c) the rate of rotation of argument of perigee.

                              2.17.  A satellite in polar orbit has a perigee height of 600 km and an apogee
                              height of 1200 km. Calculate (a) the mean motion, (b) the rate of regression of
                              the nodes, and (c) the rate of rotation of the line of apsides. The mean radius of
                              the earth may be assumed equal to 6371 km.

                              2.18. What is the fundamental unit of universal coordinated time? Express the
                              following times in (a) days and (b) degrees: 0 h, 5 min, 24 s; 6 h, 35 min, 20 s;
                              your present time.

                              2.19.  Determine the Julian days for the following dates and times: midnight
                              March 10, 1999; noon, February 23, 2000; 16:30 h, March 1, 2003; 3  P.M.,
                              July 4, 2010.

                              2.20. Find, for the times and dates given in Prob. 2.19, (a) T  in Julian centuries
                              and (b) the corresponding GST in degrees.

                              2.21.  Find the month, day, and UT for the following epochs: (a) day 3.00, year
                              1999; (b) day 186.125, year 2000; (c) day 300.12157650, year 2001; (d) day
                              3.29441845, year 2004; (e) day 31.1015, year 2010.

                              2.22.  Find the GST corresponding to the epochs given in Prob. 2.21.
                              2.23. The Molnya 3-(25) satellite has the following parameters specified: perigee
                              height 462 km; apogee height 40,850 km; period 736 min; inclination 62.8°.
                              Using an average value of 6371 km for the earth’s radius, calculate (a) the
                              semimajor axis and (b) the eccentricity. (c) Calculate the nominal mean motion
                              n 0 . (d) Calculate the mean motion. (e) Using the calculated value for a, calculate
                              the anomalistic period and compare with the specified value. Calculate (f ) the
                              rate of regression of the nodes, and (g) the rate of rotation of the line of apsides.
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