The first calculation we will do with the observations is to find the difference in time between the first and second observations and the second and third observations, respectively: Dt_{21} = t_{2} - t_{1 } Dt_{32} = t_{3} - t_{2 } Dt_{31} = t_{3} - t_{1} Dt_{21}
= 328.22 seconds The values of Dt_{21}, Dt_{32} and Dt_{31 } will now be used to find the first values that we will require to find the second geocentric range of the satellite (at time t_{2}): t_{1}
= Dt_{32}
/ Dt_{31} t_{1}
= 0.5101194 |
|||||||||||||
SITE MAP | ||
Step 2: Time Values Was Last Modified On September 23, 2013 |