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CEP to ITRF
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Fundamentals | |
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Title | CEP to ITRF |
Author(s) | J. Sanz Subirana, J.M. Juan Zornoza and M. Hernández-Pajares, Technical University of Catalonia, Spain. |
Level | Advanced |
Year of Publication | 2011 |
To transform the coordinates from CEP to ITRF it is necessary to correct the polar motion and the sidereal time (because CEP is a non-rotating system while ITRF is tied to the earth's rotation). Therefore the basic formula to apply is:
In this case, the computation is easier, Figure 1 shows the needed steps to change from CEP to ITRF.
- Diurnal rotation matrix:
- This matrix defines a rotation around the CEP pole of angle . That is:
- where is the Greenwich Apparent (=true) Sidereal Time (GAST) ^{[footnotes 1]} of date, which is given by:
- where is the Greenwich Mean Sidereal Time ^{[footnotes 2]} (GMST) and is the equinox equation at the observation time , where ^{[footnotes 3]}:
- being the GMST at UT1:
- with expressed in centuries of Julian UT1 date:
- The is the difference between the hour angle of the true equinox () of date and the mean equinox () of date ^{[footnotes 4]}, difference which is due to the nutation of earth and can be computed from:
- where is the component of the row and column of the Nutation Matrix (8) (see ICRF to CEP). Note that the sidereal time (GAST or GMST) is always measured from true Greenwich meridian.
- Polar Motion Matrix:
- This matrix is given by two elemental rotations, and around the and axis, respectively. With these rotations the CEP pole is matched into the CTP pole:
- where and define the position of the CEP with respect to the CTP (see figure 2, at right side).
- The , pole displacements between 1961 and 1964 are shown in figure 2, at left side.
- Because of the polar movement is quite unpredictable the , displacements are estimated from observations and provided by the IERS as mentioned before. These values can be obtained the from the Earth Rotation Parameters files provided by the IERS or JPL.
Figure 2: Polar Motion measurements from 2002 to 2008 (left) and polar coordinates (right)
Speed Transformation
According to the previous explanations it follows:
The transformation for the velocity is found differentiating the equation (10) respect to time:
Where is the earth revolution rate:
Notes
- ^ That is, the hour angle of the true equinox, from Greenwich meridian (see Sidereal Time).
- ^ The hour angle of the mean equinox of date, from Greenwich meridian.
- ^ The ratio of universal to sidereal times 1.002737909350795 can be approximately computed as the ratio between and . A very accurate value is .
- ^ That is, between the GAST and GMST. This difference is called Equation of Equinoxes.