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Construction of the Non-Rigid Earth Rotation Series

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1 Construction of the Non-Rigid Earth Rotation Series
V.V. Pashkevich Central (Pulkovo) Astronomical Observatory of the Russian Academy of Science St.Petersburg Space Research Centre of the Polish Academy of Sciences Warszawa 2007

2 The last years a lot of attempts to derive a high-precision theory of the non-rigid Earth rotation was carried out. For these purposes used the different transfer functions, which usually applied to the nutation in longitude and in obliquity of the rigid Earth rotation with respect to the ecliptic of date. Aim: Construction of a new high-precision non-rigid Earth rotation series (SN9000), dynamically adequate to the DE404/LE404 ephemeris over 2000 years, which is expressed as a function of the three Euler angles with respect to the fixed ecliptic plane and equinox J

3 S T E P S: The high-precision numerical solution of the rigid Earth rotation have been constructed (V.V.Pashkevich, G.I.Eroshkin and A.Brzezinski, 2004), (V.V.Pashkevich and G.I.Eroshkin, Proceedings of “Journees 2004”). The initial conditions have been calculated from SMART97 (P.Bretagnon, G.Francou, P.Rocher, J.L.Simon,1998). The discrepancies between the numerical solution and the semi-analytical solution SMART97 were obtained in Euler angles over 2000 years with one-day spacing.

4 S T E P - 1: Numerical integration of the differential equations Discrepancies: numerical solution minus SMART97 Initial conditions from SMART97

5 Problem expressed by the Rodrigues – Hamilton parameters:
S T E P - 1: Numerical integration of the differential equations Discrepancies: numerical solution minus SMART97 Initial conditions from SMART97 LAGRANGE DIFFERENTIAL EQUATIONS OF THE SECOND KIND: VECTOR OF THE GEODETIC ROTATION: Problem expressed by the Rodrigues – Hamilton parameters:

6 Fig.1 Numerical solution for Rigid Earth rotation minus solution SMART97 in the longitude of the ascending node of the Earth equator. Kinematical (relativistic) case Dynamical (Newtonian) case Secular terms of… Secular terms of… smart97 (as) d (as) smart97(as) 7.00 6.89 T T T T T2 T2 T2 T2 T3 T3 T3 T3 T4 T4 T4 T4 T5 T5 T5 T5 T6 T6

7 Fig.2 Numerical solution for Rigid Earth rotation minus solution SMART97 in the angle of the proper rotation of the Earth. Kinematical (relativistic) case Dynamical (Newtonian) case Secular terms of… Secular terms of… smart97 (as) d(as) d (as) 6.58 6.53 T T T T2 T2 T2 T2 T3 T3 T3 T3 T4 T4 T4 T4 T5 T5 T5 T5 T6 T6

8 Fig.3 Numerical solution for Rigid Earth rotation minus solution SMART97 in the inclination angle.
Kinematical (relativistic) case Dynamical (Newtonian) case Secular terms of… Secular terms of…  smart97(as) d(as) 1.42 1.39 T T T T T2 T2 T2 T2 T3 T3 T3 T3 T4 T4 T4 T4 T5 T5 T5 T5 T6 T6

9 S T E P S: The high-precision numerical solution of the rigid Earth rotation have been constructed (V.V.Pashkevich, G.I.Eroshkin and A.Brzezinski, 2004), (V.V.Pashkevich and G.I.Eroshkin, Proceedings of “Journees 2004”). The initial conditions have been calculated from SMART97 (P.Bretagnon, G.Francou, P.Rocher, J.L.Simon,1998). The discrepancies between the numerical solution and the semi-analytical solution SMART97 were obtained in Euler angles over 2000 years with one-day spacing.

10 S T E P S: The high-precision numerical solution of the rigid Earth rotation have been constructed (V.V.Pashkevich, G.I.Eroshkin and A.Brzezinski, 2004), (V.V.Pashkevich and G.I.Eroshkin, Proceedings of “Journees 2004”). The initial conditions have been calculated from SMART97 (P.Bretagnon, G.Francou, P.Rocher, J.L.Simon,1998). The discrepancies between the numerical solution and the semi-analytical solution SMART97 were obtained in Euler angles over 2000 years with one-day spacing. Investigation of the discrepancies is carried out by the least squares (LSQ) and by the spectral analysis (SA) algorithms (V.V.Pashkevich and G.I.Eroshkin, Proceedings of “Journees 2005”, 2005). The high-precision rigid Earth rotation series S9000 is determined (V.V.Pashkevich and G.I.Eroshkin, 2005 ).

11 S T E P - 1: Numerical integration of the differential equations Discrepancies: numerical solution minus SMART97 Initial conditions from SMART97 S T E P - 2

12 S T E P S - 1 and 2: Numerical integration of the differential equations Discrepancies: numerical solution minus SMART97 Initial conditions from SMART97 Precession and GMST terms of SMART97 Calculation of the secular terms by the LSQ method Set of nutation terms of SMART97 Computation of the new precession and GMST parameters Removal of the secular trends from the discreapancies Calculation of the periodical terms by the SA method High-precision series S9000 Construction of the new nutation series

13 Fig.4. The numerical solution of the rigid Earth rotation minus S9000 after formal removal of the secular trends in the proper rotation angle. Kinematical case Dynamical case

14 Fig.5. Differences between S9000 and SMART97.
Kinematical case Dynamical case

15 S T E P S: The high-precision numerical solution of the rigid Earth rotation have been constructed (V.V.Pashkevich, G.I.Eroshkin and A.Brzezinski, 2004), (V.V.Pashkevich and G.I.Eroshkin, Proceedings of “Journees 2004”). The initial conditions have been calculated from SMART97 (P.Bretagnon, G.Francou, P.Rocher, J.L.Simon,1998). The discrepancies between the numerical solution and the semi-analytical solution SMART97 were obtained in Euler angles over 2000 years with one-day spacing. Investigation of the discrepancies is carried out by the least squares (LSQ) and by the spectral analysis (SA) algorithms (V.V.Pashkevich and G.I.Eroshkin, Proceedings of “Journees 2005”, 2005). The high-precision rigid Earth rotation series S9000 is determined (V.V.Pashkevich and G.I.Eroshkin, 2005 ).

16 S T E P S: The high-precision numerical solution of the rigid Earth rotation have been constructed (V.V.Pashkevich, G.I.Eroshkin and A.Brzezinski, 2004), (V.V.Pashkevich and G.I.Eroshkin, Proceedings of “Journees 2004”). The initial conditions have been calculated from SMART97 (P.Bretagnon, G.Francou, P.Rocher, J.L.Simon,1998). The discrepancies between the numerical solution and the semi-analytical solution SMART97 were obtained in Euler angles over 2000 years with one-day spacing. Investigation of the discrepancies is carried out by the least squares (LSQ) and by the spectral analysis (SA) algorithms (V.V.Pashkevich and G.I.Eroshkin, Proceedings of “Journees 2005”, 2005). The high-precision rigid Earth rotation series S9000 is determined (V.V.Pashkevich and G.I.Eroshkin, 2005 ). The new high-precision non-rigid Earth rotation series (SN9000), which expressed in the function of the three Euler angles, is constructed by using the method (P.Bretagnon, P.M.Mathews, J.-L.Simon: 1999) and the transfer function (Mathews, P. M., Herring, T. A., and Buffett B. A., 2002).

17 Expressions for Euler angles:
S T E P - 3: Expressions for Euler angles:

18 Classical A l g o r i t h m

19 Classical A l g o r i t h m Expressions for the non-rigid Earth nutations in longitude and obliquity:

20 TRANSFER FUNCTIONS J.M.Wahr ,1981; V. Dehant and P. Defraigne, 1997: T. Shirai and T. Fukushima, 2001:

21 TRANSFER FUNCTIONS P.Bretagnon, P.M. Mathews, J.-L. Simon,1999: P.M. Mathews, T.A. Herring, B.A. Buffett, 2002:

22 P.M. Mathews, T.A. Herring, B.A. Buffett, 2002:
TRANSFER FUNCTIONS P.M. Mathews, T.A. Herring, B.A. Buffett, 2002: Geophisical model includes : The effects Electromagnetic coupling The Ocean effects Mantle inelasticity effects Atmospheric effects Change in the global Earth dynamical flattening and in the core flattening

23 Algorithm of Bretagnon et al. 1999
1.The rigid Earth angular velocity vector:

24 Expressions for the Earth’s angular velocity vector:
The coefficients of the developments of p, q in case of the rigid Earth:

25 The components of the Rigid Earth angular velocity vector:

26 The components of the coefficients of the developments of p, q
in case of the rigid Earth:

27 The amplitudes of the prograde and retrograde components:
Complex transformation of the componets of the angular velocity vector:

28 Algorithm of Bretagnon et al. 1999
1.The rigid Earth angular velocity vector: 2.The non-rigid Earth angular velocity vector is obtained by:

29 The components of the coefficients of the developments of p, q
in case of the non-rigid Earth:

30 The prograde and retrograde components of the coefficients
of the developments of p in case of the non-rigid Earth:

31 The prograde and retrograde components of the coefficients
of the developments of q in case of the non-rigid Earth:

32 The sin coefficients of the developments
for the non-rigid Earth angular velocity vector:

33 The cos coefficients of the developments
for the non-rigid Earth angular velocity vector:

34 Algorithm of Bretagnon et al. 1999
1.The rigid Earth angular velocity vector: 2.The non-rigid Earth angular velocity vector is obtained by: 3.The derivatives of Euler angles for the non-rigid Earth rotation:

35 Common form of the periodic part of Euler angles:
Cascade method:

36 Iterative solution of the algorithm of Bretagnon et al. 1999
Details: Iterative solution of the algorithm of Bretagnon et al. 1999 1 iteration

37 Iterative solution of the algorithm of Bretagnon et al. 1999
Details: Iterative solution of the algorithm of Bretagnon et al. 1999 n iteration Iterations are repeated until the absolute value of the difference between iterations K-1 and K exceedes some DEFINITE values 

38 DD- Dehant and Defraigne, 1997; BMS- Bretagnon et al., 1999;
Results: Table 1. Comparison of different solutions Argument (λ3 +D-F ) with a 18.6 year period Solution Ψ(sin) μas Ψ(cos) θ (sin) θ (cos) φ (sin) φ (cos) S9000+Wahr 1981 -431 35 -395 S9000+DD -396 S9000+SF -2701 -1269 -2479 S9000+BMS -3351 -1486 -3075 S9000+MHB -3386 -1505 -3106 DD- Dehant and Defraigne, 1997; BMS- Bretagnon et al., 1999; SF-Shirai and Fukushima, 2001; MHB- Mathews et al., 2002.

39 DD- Dehant and Defraigne, 1997; BMS- Bretagnon et al., 1999;
Results: Table 1. Comparison of different solutions Argument (λ3 +D-F ) with a 18.6 year period Solution Ψ(sin) μas Ψ(cos) θ (sin) θ (cos) φ (sin) φ (cos) SMART97+Wahr 1981 -431 35 -395 SMART97+DD -396 SMART97+SF -2701 -1269 -2479 SMART97+BMS -3351 -1486 -3075 SMART97+MHB -3386 -1505 -3106 DD- Dehant and Defraigne, 1997; BMS- Bretagnon et al., 1999; SF-Shirai and Fukushima, 2001; MHB- Mathews et al., 2002.

40 Table 2. Comparison of different solutions For some arguments
Argu-ment, Period (days) Ψ(sin) μas Ψ(cos) θ (sin) θ (cos) φ (sin) φ (cos) SMN SN9000 λ3 +D-F 2λ3 182.62 2λ3+2D 13.66 2λ3 +2D-2F λ3 365.24 3λ3 121.75 SMN=SMART97+MHB; SN9000=S9000+MHB; MHB- Mathews et al., 2002.

41 Fig.6. The differences between SN9000 and SMN after removal of the secular terms. (non-rigid Earth rotation) Dynamical case μas Δφ Δθ Δψ YEARS

42 Fig.7. The differences between S9000 and SMART after removal of the secular terms. (rigid Earth rotation) Dynamical case μas Δφ Δθ Δψ YEARS

43 Fig.8. The differences between SN9000 and SMN after removal of the secular terms. (non-rigid Earth rotation) Kinematical case μas Δφ Δθ Δψ YEARS

44 Fig.9. The differences between S9000 and SMART after removal of the secular terms. (rigid Earth rotation) Kinematical case μas Δφ Δθ Δψ YEARS

45 Fig.10. The differences between S9000 and SN9000.
Dynamical case μas Δφ Δθ Δψ YEARS

46 Fig.11. The differences between S9000 and SN9000.
Kinematical case μas Δφ Δθ Δψ YEARS

47 Fig.12. The differences between SMART97 and SMN.
Dynamical case μas Δφ Δθ Δψ YEARS

48 Fig.13. The differences between SMART97 and SMN.
Kinematical case μas Δφ Δθ Δψ YEARS

49 Fig.14. The discrepancies between S9000 and SN9000 minus discrepancies between SMART97 and SMN.
Dynamical case μas Δφ Δθ Δψ YEARS

50 Fig.15. The discrepancies between S9000 and SN9000 minus discrepancies between SMART97 and SMN.
Kinematical case μas Δφ Δθ Δψ YEARS

51 Kinematical solution of the rigid Earth rotation= Dynamical solution of the rigid Earth rotation + Geodetics corrections Dynamical solution of the non-rigid Earth rotation= Dynamical solution of the rigid Earth rotation + TRANSFER FUNCTIONS Original Kinematical solution of the non-rigid Earth rotation= Dynamical solution of the rigid Earth rotation + TRANSFER FUNCTIONS + Geodetics corrections Kinematical solution of the non-rigid Earth rotation= Kinematical solution of the rigid Earth rotation + TRANSFER FUNCTIONS

52 CONCLUSION The exact expressions for the algorithm of Bretagnon et al. (1999) are obtained. The new semi-analytical solution of the non-rigid Earth rotation SMN (SMART97+MHB2002) is derived. The high-precision non-rigid Earth rotation series SN9000, which is expressed as a function of the three Euler angles and is dynamically adequate to the ephemerides DE404/LE404 over 2000 years, has been constructed.

53 R E F E R E N C E S P.Bretagnon and G.Francou. Planetary theories in rectangular and spherical variables // Astronomy and Astrophys., 202, 1988, pp. 309–-315. P.Bretagnon, G.Francou, P.Rocher, J.L.Simon. SMART97: A new solution for the rotation of the rigid Earth // Astron. Astrophys. , 1998, 329, pp P.Bretagnon,P.M.Mathews,J.-L.Simon. Non Rigid Earth Rotation // in Proc. Journees 1999: Motion of Celestial Bodies, Astrometry and Astronomical Reference Frames Les Journees 1999 \& IX. Lohrmann - Kolloquium, (Dresden, September 1999), p V.A..Brumberg, P.Bretagnon. Kinematical Relativistic Corrections for Earth’s Rotation Parameters // in Proc. of IAU Colloquium 180, eds. K.Johnston, D. McCarthy, B. Luzum and G. Kaplan, U.S. Naval Observatory, 2000, pp. 293–302. V.Dehant and P.Defraigne. New transfer functions for nutations of a non-rigid Earth // J. Geophys. Res., 1997,102, pp Mathews, P. M., Herring, T. A., and Buffett B. A.. Modeling of nutation and precession: New nutation series for nonrigid Earth and insights into the Earth's Interior // J. Geophys. Res., 2002, 107, B4, /2001JB V.V.Pashkevich, G.I.Eroshkin and A. Brzezinski. Numerical analysis of the rigid Earth rotation with the quadruple precision // Artificial Satellites, Vol. 39, No. 4, Warszawa, 2004, pp. 291–304. V. V. Pashkevich and G. I. Eroshkin. Spectral analysis of the numerical theory of the rigid Earth rotation // in Proc. of “Journees 2004”, Fundamental Astronomy: New concepts and models for high accuracy observations» (Observatoire de Paris, September 2004.), pp V.V.Pashkevich and G.I.Eroshkin. Choice of the optimal spectral analysis scheme for the investigation of the Earth rotation problem // in Proc. of “Journees 2005”, Earth dynamics and reference systems: five years after the adoption of the IAU 2000 Resolutions (Space Research Centre of Polish Academy of Sciences, Warsaw, Poland, September 2005), pp V.V.Pashkevich and G.I.Eroshkin. Application of the spectral analysis for the mathematical modelling of the rigid Earth rotation // Artificial Satellites, Vol. 40, No. 4, Warszawa, 2005, pp. 251–260. T.Shirai and T.Fukushima. Construction of a new forced nutation theory of the nonrigid Earth // The Astron. Journal, 121, 2001, pp J.M.Wahr. The forced nutationsof an elliptical, rotating, elastic and oceanless Earth // Geophys. J. R. Astron. Soc., 1981, 64, pp

54 A C K N O W L E D G M E N T S The investigation was carried out at the Central (Pulkovo) Astronomical Observatory of the Russian Academy of Sciences and the Space Research Centre of the Polish Academy of Sciences, under a financial support of the agreement cooperation between the Polish and Russian Academies of Sciences, Theme No 31.


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