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Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography, Zdiby & CEDR Prague-Ondřejov

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Page 1: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

Astronomical Institute, Academy of Sciences

Ondřejov Observatory,Czech Republic

&Geodetic Observatory,

Research Inst. for Geodesy, Topography and Cartography,

Zdiby&

CEDR Prague-Ondřejov

Page 2: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

SATELLITE ORBIT GEOMETRY: DIVERSITY OF GROUND TRACKS,

APPLICATIONS FOR GRAVITY STUDIES, OCEANOGRAPHY, AND REMOTE SENSING

J. Klokočník, J. Kostelecký

LECTURE AT NRIAG HELWAN EGYPT November 2005

Jaroslav Klokočník
Doplněno v březnu 2005 pro přednášku v ASÚ AV ČR Ondřejov 4.dubna 2005
Page 3: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

Definitions Geometry of Satellite Groundtrack Patterns is dictated by the orbit inclination, semimajor axis, and eccentricity

Fundamental interval Longitudinal spacing between sequential orbit traces at the equator Equals to the nodal period of satellite motiont times the difference between the inertial rotation of the Earth and precessional rate of the line of orbit nodes

S = o α/β Density of ground tracks Longitudinal spacing of adjacent tracks at equator

D = o/β [km] where o=40075km=2π R Density also depends on latitude which is not described by this equation

• Geodetic Mission• Exact Repeat (Oceanography) Mission• Orbit maneouvres in semimajor axis to tune orbit for specific application

Example of ground tracks for a satellite with given orbit inclination and semimajor axis,

ascending and descending tracks,

prograde vs retrograde orbits

crossover points, turning points

Page 4: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 5: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 6: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 7: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 8: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

number of nodal revolutions per of synodic daysnumber of nodal revolutions per of synodic days

Page 9: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 10: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 11: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 12: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 13: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 14: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

Ground tracks for EgyptSat1 initial elements I= 98. 1 deg a = 7046. 14 km resonant orbits (ExactRepeat Missions): Kozai’s semimajor axes a(44/3) = 7048.60 km a(191/13) = 7040.45 km

Page 15: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 16: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 17: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

Examples of ground tracks density for EgyptSat1 theoretical orbit

• Density of ground tracks D =o/β [km], where o=40075km=2π R

• Geodetic Missions GM• Exact Repeat (Oceanography) Missions ERM• Orbit maneouvres in semimajor axis to tune orbit for specific application

Examples resonance β/α density of ground tracks [in km]---------------------------------------------------------------------------------------- 44/3 910 59/4 680 89/6 450 191/13 210 … 235/16 170 GM <20 **--------------------------------------------------------------------------------------

Page 18: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 19: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 20: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 21: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 22: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

GRACE around 61/4 resonance

Page 23: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 24: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 25: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 26: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,
Page 27: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

Conclusions

Orbit of a satellite can be tailored to the required application by a proper selection of orbital inclination and semimajor axis

(examples given for gravity missions and oceanography satellites)

Small changes of semimajor axis by the orbit maneouvre(s) (even without changing the other elements) result in different resonance regimes and in changes of the density of satellite ground tracks, and such changes may be dramatic

One satellite may offer several different orbits with diverse

density of ground tracks and thus may serve for different applications (different orbit scenarios)

(examples of orbit maneouvres of ERS 1,2, and also -- with another motivation -- semimajor axis increments for CHAMP)

Page 28: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

To get a copy

• Anonymous ftp: sunkl.asu.cas.cz• pub/jklokocn

file: PPT_GEOMETRY_EGYPT05.ppt

• For more information: Web: www.asu.cas.cz/~jklokocn • e-mail: [email protected][email protected]

Page 29: Astronomical Institute, Academy of Sciences Ondřejov Observatory, Czech Republic & Geodetic Observatory, Research Inst. for Geodesy, Topography and Cartography,

The END