Interaction between tidal terms and GPS orbits
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1 Interaction between tidal terms and GPS orbits Natalia Panafidina, Manuela Seitz, Urs Hugentobler Deutsches Geodätisches Forschungsinstitut (DGFI) Centrum für Geodätische Erdsystemforschung (CGE) München TU München EGU 2013, Vienna, Austria, 7-12 April 2013
2 Introduction Subdaily Earth Rotation model: IERS2010 (+ libration) Kept fixed in the processing Errors up to ~20% Empirical tidal models from GPS & VLBI: Big corrections (more than 10 µas in PM) for some tidal terms: K1(23.93h), S1 (24h), M2(12.42h), S2(12h), K2(11.97h) IERS2010+libration: K1 correction ~30 µas
3 Introduction Subdaily Earth Rotation model: IERS2010 (+ libration) Kept fixed in the processing Errors up to ~20% Empirical tidal models from GPS & VLBI: Big corrections (more than 10 µas in PM) for some tidal terms: K1(23.93h), S1 (24h), M2(12.42h), S2(12h), K2(11.97h) IERS2010+libration: K1 correction ~30 µas Influence of a wrong subdaily model on the orbits, coordinates, ERPs Are there draconitic signatures caused by a wrong subdaily model?
4 Data and solutions Data: Daily NEQs ( ): station coordinates, 1h-ERPs, GPS orbits IERS2000 subdaily model used in processing What we do: Daily solutions, transformation 1h-ERPs tidal terms change apriori values for tidal terms + fix tidal terms change subdaily model Daily estimates: GPS orbits, station coordinates, geocenter (NNR+NNT), 24h ERPs
5 Data and solutions Influence of subdaily tidal model: change 1 tide in PM by ~100 µas Daily solutions standard subdaily model changed subdaily model Time series of differences: GPS orbits ERPs Station coordinates Spectra
6 Data and solutions Influence of subdaily tidal model: change 1 tide in PM by ~100 µas Daily solutions standard subdaily model changed subdaily model Time series of differences: GPS orbits ERPs Station coordinates Spectra
7 GPS satellites and tidal variations in Earth rotation Prograde K1 period: 23h56min in terrestrial reference frame (~1 cpd) 11h58min in inertial reference frame (~2 cpd) Orbital period of GPS satellites: 11h58min K1 CIP After half a period: CIP
8 GPS satellites and tidal variations in Earth rotation Prograde K1 period: 23h56min in terrestrial reference frame (~1 cpd) 11h58min in inertial reference frame (~2 cpd) Orbital period of GPS satellites: 11h58min K1 CIP After half a period: CIP K1 is seen as a constant shift
9 GPS satellites and tidal variations in Earth rotation Prograde K1 period: 23h56min in terrestrial reference frame (~1 cpd) 11h58min in inertial reference frame (~2 cpd) Orbital period of GPS satellites: 11h58min K1 CIP After half a period: CIP K1 is seen as a constant shift Beat periods: Close periods are seen as slow rotation
10 GPS satellites and tidal variations in Earth rotation Prograde K1 period: 23h56min in terrestrial reference frame (~1 cpd) 11h58min in inertial reference frame (~2 cpd) Orbital period of GPS satellites: 11h58min Diurnal tides have periods in CRF ~12 hours Beat periods: Φ1(23.80h) ~185d Ψ1(23.87h) ~380d K1(23.93h) ~shift S1(24.00h) ~352d P1(24.07h) ~179d
11 GPS satellites and tidal variations in Earth rotation Prograde K1 period: 23h56min in terrestrial reference frame (~1 cpd) 11h58min in inertial reference frame (~2 cpd) Orbital period of GPS satellites: 11h58min Diurnal tides have periods in CRF ~12 hours Beat periods: Φ1(23.80h) ~185d Ψ1(23.87h) ~380d K1(23.93h) ~shift S1(24.00h) ~352d P1(24.07h) ~179d Semi-diurnal tides have periods in CRF ~8 hours Beat periods: M2(12.42h) ~25.82h S2(12.00h) ~24.07h K2(11.67h) ~23.94h
12 Test solutions Daily solutions standard subdaily model changed subdaily model Changed tidal terms: S1(24.00h), beat period ~352d P1(24.07h), beat period ~180d O1(25.82h), beat period ~14d Spectra of time series of differences: GPS orbits: 6 Kepler elements, CODE Radiation Pressure Parameters
13 Influence of tidal model on the orbit: Kepler elements and radiation pressure parameters S1(24.00h), beat period ~352d S1(24.00h), beat period ~352d P1(24.07h), beat period ~180d P1(24.07h), beat period ~180d O1(25.82h), beat period ~14d O1(25.82h), beat period ~14d O1
14 Influence of tidal model on the orbit: noise increase Aposteriori RMS: Standard solution minus test solution changed S1 (24.00h) Standard solution minus test solution changed M2r (12.42h)
15 Influence of tidal model on the orbit Can we see tidal contribution in time series of real orbital parameters? Test: K1 change of 100 µas ~1.5cm change in semi-major axis, ~0.4 nm/sec**2 in RPR Realistic changes for main tides ~0.6cm change in semi-major axis, ~0.1 nm/sec**2 in RPR
16 Influence of tidal model on the orbit Can we see tidal contribution in time series of real orbital parameters? Test: K1 change of 100 µas ~1.5cm change in semi-major axis, ~0.4 nm/sec**2 in RPR Realistic changes for main tides ~0.6cm change in semi-major axis, ~0.1 nm/sec**2 in RPR Spectra of daily estimates of orbital parameters from standard solution
17 Conclusions Errors in subdaily tidal model lead to periodic signals in the GPS orbits with beat periods of the tides (+ aliasing if sampled e.g. 24h) Beat periods of ~350 days can contribute to observed signals with draconitic periods Diurnal tides are better absorbed by the orbits because their periods in CRF are close to those of GPS satellites Semi-diurnal tides increase the residuals more than diurnal tides Periodic signals in the orbits caused by wrong tides are very small, but still can be seen by spectral anslysis
18 Thank you!
19 Influence of tidal model on the station coordinates YELL, CHUR (Canada): tide S1 KOKB, MKEA (Hawaii): tide S1 HUR
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