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xiii | |
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xvi | |
Preface |
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xvii | |
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The Usual Decomposition |
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xviii | |
The Decomposition Using Trace-Less Parts |
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xix | |
Decomposition Into Two Parts |
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xix | |
Decomposition Into Divergence-Free Parts |
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xx | |
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1 | (26) |
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3 | (10) |
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The Experimental Basis of General Relativity |
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3 | (1) |
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4 | (3) |
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The Gravitomagnetic Field in Astrophysical Scenarios |
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4 | (1) |
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The Gravitomagnetic Field of the Earth |
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4 | (3) |
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The Gravitomagnetic Fields of the Sun and of Mars |
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7 | (1) |
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7 | (2) |
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7 | (2) |
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9 | (1) |
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Is It Really Necessary to Perform Experiments to Directly Measure Gravitomagnetism? |
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9 | (2) |
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11 | (1) |
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11 | (2) |
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13 | (14) |
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13 | (1) |
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14 | (6) |
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Mach's Principle and General Relativity |
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20 | (1) |
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21 | (2) |
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Tact of the Natural Investigator |
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23 | (1) |
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Quantum Theory and Inertia |
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24 | (1) |
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25 | (2) |
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27 | (74) |
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Gravitoelectromagnetism: A Brief Review |
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29 | (12) |
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29 | (1) |
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Linear Perturbation Approach to GEM |
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30 | (2) |
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Gravitational Larmor Theorem |
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32 | (2) |
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Spacetime Curvature Approach to GEM |
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34 | (3) |
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Spin-Rotation-Gravity Coupling |
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37 | (4) |
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Analogies and Differences between Gravito-Electromagnetism and Electro-magnetism |
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41 | (10) |
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41 | (1) |
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Direct Deduction of the Gravito-Electromagnetic Faraday-Henry Law |
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42 | (3) |
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Is There a Gravito-Magnetic Meissner Effect? |
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45 | (2) |
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Inconsistencies of the Gravito-Electromagnetic Analogy |
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47 | (1) |
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Discussion and Conclusions |
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48 | (3) |
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Quasi-Inertial Coordinates |
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51 | (22) |
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51 | (1) |
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Fermi-Walker Transport of a Tetrad |
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52 | (3) |
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55 | (2) |
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Geodetic Precession of Freely-Falling Gyroscope |
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57 | (1) |
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Construction of Quasi-Inertial Coordinates |
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58 | (6) |
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61 | (1) |
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Coordinate Transformations |
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61 | (1) |
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Metric in Quasi-Inertial Frame |
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62 | (2) |
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Spin Precession in the Quasi-Inertial Frame |
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64 | (1) |
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65 | (2) |
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Two Sources-Sun and Earth |
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67 | (2) |
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Local Inertial Frame of Earth |
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69 | (2) |
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71 | (2) |
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The Lense-Thirring Effect on the Orbit of a Test Particle |
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73 | (14) |
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The Orbit of a Test Particle in Space |
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73 | (3) |
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The Derivation of the Lense-Thirring Effect on the Orbit of a Test Particle: the Lagrangian Approach |
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76 | (4) |
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The Derivation of the Lense-Thirring Effect on the Orbit of a Test Particle: the Gaussian Approach |
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80 | (4) |
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An Extension of the Gravitational Larmor Theorem |
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84 | (1) |
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The Gravitomagnetic Stern-Gerlach Force |
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85 | (2) |
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Post-Newtonian Orbital Perturbations |
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87 | (14) |
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87 | (1) |
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88 | (2) |
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90 | (1) |
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91 | (5) |
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Precession of the Pericenter |
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91 | (1) |
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Precession of the Orbital Plane |
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92 | (1) |
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The Change in the Mean Motion |
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93 | (3) |
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Time Difference Induced by Precession |
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96 | (1) |
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Time Difference due to Pericenter Precession |
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96 | (1) |
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Time Difference due to Orbital Precession |
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97 | (1) |
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The Sidereal Period and the Gravitomagnetic Clock Effect |
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97 | (2) |
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An Alternative Derivation of the Gravitomagnetic Sidereal Effect for Circular and Equatorial Orbits |
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99 | (2) |
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101 | (136) |
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Recent Developments in Testing Gravitomagnetism with Satellite Laser Ranging |
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103 | (34) |
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103 | (3) |
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The Gravitoelectric Effects |
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104 | (1) |
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The Gravitomagnetic Effects |
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104 | (2) |
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The Major Systematic Errors |
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106 | (6) |
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The Non-Gravitational Errors |
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106 | (1) |
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106 | (6) |
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Some New Observables for Measuring the Lense-Thirring Effect |
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112 | (2) |
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The Supplementary Orbital Planes Option |
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112 | (1) |
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113 | (1) |
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The Impact of the 1st Generation of Earth Gravity Models from Champ and Grace |
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114 | (4) |
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The Full-Range Even Zonal Harmonics Observables |
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114 | (1) |
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The Partial-Range Even Zonal Harmonics Observables |
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115 | (1) |
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Combinations With the Other Existing Geodetic Satellites |
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116 | (2) |
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The Use of Data from the Altimeter Satellite Jason-1 |
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118 | (6) |
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A Possible Combination of Nodes and the Gravitational Errors |
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119 | (1) |
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The Impact of the Observational Errors of Ajisai and Jason-1 |
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119 | (1) |
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The Impact of the Non-Gravitational Perturbations of Ajisai |
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119 | (2) |
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The Impact of the Non-Gravitational Perturbations on Jason-1 |
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121 | (3) |
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The 2nd Generation of the Grace-only Earth Gravity Models and the First Champ/Grace Combined Model |
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124 | (1) |
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124 | (1) |
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125 | (1) |
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125 | (1) |
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A Quantitative Assessment of the Impact of the Secular Variations of the Even Zonal Harmonics on the Performed Test with the Nodes of the Lageos Satellites |
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125 | (9) |
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127 | (4) |
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131 | (2) |
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133 | (1) |
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Discussion and Conclusions |
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134 | (3) |
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The Use of Ajisai and Jason-1 |
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134 | (1) |
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The Lageos-Lageos II Node-Node-Perigee Combination |
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135 | (1) |
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A New Dedicated Satellite? |
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135 | (2) |
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The Lageos Satellites: Non-Gravitational Perturbations and the Lense-Thirring Effect |
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137 | (20) |
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138 | (1) |
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The Osculating Orbital Elements and the Gaussian Perturbativc Equations |
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139 | (2) |
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The Non-Gravitational Perturbations: A Brief Review |
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141 | (10) |
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Visible Radiation Effects: Direct Solar Radiation Pressure |
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141 | (2) |
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Visible Radiation Effects: Earth Albedo |
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143 | (1) |
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The Lageos Satellites Spin-Axis Modeling |
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144 | (1) |
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145 | (5) |
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The Asymmetric Reflectivity Effect |
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150 | (1) |
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151 | (2) |
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The Lense-Thirring Effect Error Budget and the NGP |
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153 | (1) |
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154 | (3) |
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On the Impossibility of Using the Node of Nearly Polar Satellites for Measuring the Lense-Thirring Effect |
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157 | (8) |
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157 | (5) |
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The Static and Time-Varying Part of the Earth Gravitational Field |
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158 | (4) |
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On the (Im)possibility of Using a Polar Lares |
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162 | (1) |
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162 | (3) |
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Error Budget for the Gravitomagnetic Clock Effect |
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165 | (12) |
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165 | (1) |
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The Impact of the Orbital Injection Errors |
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166 | (9) |
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The Imperfect Cancellation of the Keplerian Periods |
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167 | (1) |
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The Imperfect Cancellation of the Post-Newtonian Periods |
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168 | (1) |
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The Impact of the Classical Gravitational Perturbations |
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169 | (4) |
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The Impact of the Errors in the Inclinations |
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173 | (1) |
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The N-Body Gravitational Perturbations |
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174 | (1) |
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The Impact of the Non-Gravitational Perturbations |
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175 | (1) |
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175 | (2) |
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Is it Possible to Measure the Lense-Thirring Effect in the Gravitational Fields of the Sun and of Mars? |
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177 | (12) |
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The Solar Gravitomagnetic Field |
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178 | (5) |
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Compatibility of the Estimated Extra-Precessions of Planetary Perihelia with the Lense-Thirring Effect |
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178 | (4) |
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Analysis of Other Independent Data |
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182 | (1) |
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Testing Gravitomagnetism with Mars Global Surveyor in the Field of Mars |
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183 | (3) |
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Discussion and Conclusions |
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186 | (3) |
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On the Detectability of the Earth's Gravitomagnetic Field in Laboratory Experiments |
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189 | (12) |
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189 | (2) |
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Proposed Earth Based Laboratory Experiments |
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191 | (9) |
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A Foucault Pendulum at South Pole |
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191 | (2) |
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A Magnetic-Gravitomagnetic Experiment |
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193 | (1) |
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A Michelson-Moreley-Type Experiment |
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194 | (2) |
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The Use of Ring Laser Gyroscopes |
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196 | (1) |
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A Terrestrial Version of the Gravitomagnetic Clock Effect |
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197 | (3) |
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Discussion and Conclusions |
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200 | (1) |
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Atom Interferometry and Gravitomagnetism |
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201 | (36) |
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201 | (2) |
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203 | (10) |
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The Sagnac Effect for Light |
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203 | (5) |
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The Operational Definition of Rotation |
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208 | (2) |
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The Sagnac Effect for Matter Waves |
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210 | (3) |
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Basics About Atomic Interferometry |
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213 | (11) |
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The Non-Relativistic Hamiltonian for Atoms |
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213 | (4) |
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The Hamiltonian for the Energy Levels |
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217 | (1) |
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The Center-of-Mass Hamiltonian |
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217 | (2) |
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219 | (1) |
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220 | (2) |
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222 | (1) |
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The Observed Interference Pattern |
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223 | (1) |
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The Phase Shift for Gravito-Inertial Effects |
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224 | (13) |
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224 | (7) |
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231 | (1) |
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232 | (2) |
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Comparison with Other Methods |
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234 | (3) |
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A. The Inclination Functions |
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237 | (2) |
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B. The Classical Orbital Precessions |
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239 | (8) |
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240 | (1) |
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The Pericenter Coefficients |
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241 | (6) |
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247 | (2) |
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References |
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249 | (22) |
Index |
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271 | |