Book description
Explore the development and state-of-the-art in deep space exploration using radio science techniques
In Radio Science Techniques for Deep Space Exploration, accomplished NASA/JPL researcher and manager Sami Asmar delivers a multi-disciplinary exploration of the science, technology, engineering, mission operations, and signal processing relevant to deep space radio science. The book discusses basic principles before moving on to more advanced topics that include a wide variety of graphical illustrations and useful references to publications by experts in their respective fields.
Complete explanations of changes in the characteristics of electromagnetic waves and the instrumentation and technology used in scientific experiments are examined.
Radio Science Techniques for Deep Space Exploration offers answers to the question of how to explore the solar system with radio links and better understand the interior structures, atmospheres, rings, and surfaces of other planets. The author also includes:
- Thorough introductions to radio science techniques and systems needed to investigate planetary atmospheres, rings, and surfaces
- Comprehensive explorations of planetary gravity and interior structures, as well as relativistic and solar studies
- Practical discussions of instrumentation, technologies, and future directions in radio science techniques
Perfect for students and professors of physics, astronomy, planetary science, aerospace engineering, and communications engineering, Radio Science Techniques for Deep Space Exploration will also earn a place in the libraries of engineers and scientists in the aerospace industry.
Table of contents
- Cover
- Serious page
- Title page
- Copyright
- Foreword
- Preface
- Acknowledgments
- Author and Contributors
-
1 Investigations and Techniques
- 1.0 Introduction
- 1.1 Historical Background
- 1.1.1 The Field of Radio Science
- 1.2 Fundamental Concepts
- 1.2.1 Categories of RS Investigations
- 1.2.2 Related Fields
- 1.3 Historical Development
- 1.4 Overview of the Radio Science Instrumentation System
- 1.4.1 Flight System
- 1.4.2 Ground System
- 1.4.3 Other Ground Stations
- 1.5 Noise, Error Sources, and Calibrations
- 1.6 Experiment Implementation, Data Archiving, and Critical Mission Support
- 1.7 Radio Science at Home
- 1.8 Future Directions
- 1.9 Summary and Remaining Chapters
- Appendix 1A Selected Accomplishments and Planned Observations in Spacecraft Radio Science
- 1A.1 Selected Accomplishments in Radio Science
- 1A.2 Planned Observations in the Near-Term
- 1A.3 Planned Observations in the Long Term
-
2 Planetary Atmospheres, Rings, and Surfaces
- 2.1 Overview of Radio Occultations
- 2.2 Neutral Atmospheres
- 2.2.1 Abel Inversion
- 2.3 Ionospheres
- 2.4 Rings
- 2.4.1 Ring Occultation Observables
- 2.4.2 Ring Occultation Analysis
- 2.4.3 Ring Diffraction Correction
- 2.4.4 Data Decimation and Profile Resolution
- 2.4.5 Signal-to-noise Ratio-resolution Tradeoff
- 2.5 Surface Scattering
-
3 Gravity Science and Planetary Interiors
- 3.1 Overview
- 3.2 Gravity Observables and Formulations
- 3.2.1 Alternative Basis and Methods
- 3.2.2 Tidal Forces and Time Variable Gravity
- 3.2.3 Covariance Analysis
- 3.3 Earth and Moon Gravity Measurements and the Development of Crosslinks
- 3.4 Shape and Topography Data for Interpretation of Gravity Measurements
- 3.4.1 Imagery
- 3.4.2 Altimetry
- 3.4.3 Space-based Radar
- 3.4.4 Radio Occultations
- 3.4.5 Ground-based Radar
- 3.4.6 Examples of Results of Gravity–Topography Analysis
- 3.5 Application to Solar System Bodies
- 3.5.1 Moon
- 3.5.2 Mercury
- 3.5.3 Venus
- 3.5.4 Mars
- 3.5.5 Jupiter
- 3.5.6 Saturn
- 3.5.7 Uranus
- 3.5.8 Neptune
- 3.5.9 Pluto
- 3.5.10 Asteroids and Comets
- 3.5.11 Pioneer and Earth Flyby Anomalies
- 3.6 A User’s Guide
- 3.6.1 Calculation of Observables and Partials
- 3.6.2 Estimation Filter
- 3.6.3 Solution Analysis
- Appendix 3A Planetary Geodesy
- 3A.1 Planetary Geodesy: Gravitational Potentials and Fields
- 3A.2 Gravity Determination Technique
- 3A.3 Dynamical Integration
- 3A.4 Processing of Observations
- 3A.5 Filtering of Observations
-
4 Solar and Fundamental Physics
- 4.1 Principles of Heliospheric Observations
- 4.2 Inner Heliospheric Electron Density
- 4.3 Density Power Spectrum
- 4.4 Intermittency, Nonstationarity, and Events
- 4.5 Faraday Rotation
- 4.6 Spaced-receiver Measurements
- 4.7 Space-time Localization of Plasma Irregularities
- 4.8 Utility for Telecommunications Engineering
- 4.9 Precision Tests of Relativistic Gravity
- 4.10 Scientific Goals and Objectives
- 4.10.1 Determine γ to an Accuracy of 2 ×10−6
- 4.10.2 Determine β to an Accuracy of ~3 ×10−5
- 4.10.3 Determine η to an Accuracy of at Least 4.4 ×10−4
- 4.10.4 Determine α1 to an Accuracy of 7.8 ×10−6
- 4.10.5 Determine the Solar Oblateness to an Accuracy of 4.8 ×10−9
- 4.10.6 Test Any Time Variation of the Gravitational Constant, G, to an Accuracy of 3 10×−13 Per Year
- 4.10.7 Characterize the Solar Corona
- 4.11 Comparison with Other Experiments
- 4.11.1 Cassini
- 4.11.2 Gravity Probe B
- 4.11.3 Messenger
- 4.11.4 Lunar Laser Ranging
- 4.11.5 Gaia
- 4.12 MORE Summary
- 4.13 Anomalous Motion of Pioneers 10 and 11
- Appendix 4A Solar Corona Observation Methodology Illustrated by Mars Express
- 4A.1 Formulation
- 4A.2 Total Electron Content from Ranging Data
- 4A.3 Change in Total Electron Content from Doppler Data
- 4A.4 Electron Density
- 4A.5 Coronal Mass Ejections
- 4A.6 Separation of Uplink and Downlink Effects from Plasma
- 4A.7 Earth Atmospheric Correction
- 4A.8 Example Data
- Appendix 4B Faraday Rotation Methodology Illustrated by Magellan Observations
- 4B.1 Formulation
- 4B.2 Coronal Radio Sounding
- 4B.3 The Faraday Rotation Effect
- 4B.4 Measurement of the Total Electron Content
- 4B.5 Combining the Faraday Rotation and Total Electron Content
- 4B.6 Instrument Overview: The Magellan Spacecraft
- 4B.7 Instrument Overview: The Deep Space Network
- 4B.8 Data Processing and Results
- 4B.9 Conclusion
- Appendix 4C Precision Doppler Tracking of Deep Space Probes and the Search for Low-frequency Gravitational Radiation
- 4C.1 Background
- 4C.2 Response of Spacecraft Doppler Tracking to Gravitational Waves
- 4C.3 Noise in Doppler GW Observations and Their Transfer Functions
- 4C.4 Detector Performance
- 4C.4.1 Periodic and Quasi-periodic Waves
- 4C.4.2 Burst Waves
- 4C.4.3 Stochastic Waves
- 4C.5 Sensitivity Improvements in Future Doppler GW Observations
-
5 Technologies, Instrumentation, and Operations
- 5.1 Overview
- 5.1.1 End-to-End Instrumentation Overview
- 5.1.2 Experiment Error Budgets
- 5.2 Key Concepts and Terminology
- 5.2.1 The Allan Deviation for Frequency and Timing Standards
- 5.2.2 Signal Operational Modes
- 5.2.3 Reception Modes
- 5.2.4 Signal Carrier Modulation Modes
- 5.3 Radio Science Technologies
- 5.3.1 Spacecraft Ultrastable Oscillator
- 5.3.2 Spacecraft Ka-band Translator
- 5.3.3 Spacecraft Open-loop Receiver
- 5.3.4 Spacecraft Radio Science Beacon
- 5.3.5 Ground Water Vapor Radiometer
- 5.3.6 Ground Advanced Ranging Instrument
- 5.3.7 Ground Bethe Hole Coupler
- 5.3.8 Ground Advanced Pointing Techniques
- 5.4 Operations and Experiment Planning
- 5.5 Data Products
- 5.5.1 Range Rate
- 5.5.2 Range
- 5.5.3 Delta Differential One-way Ranging (Delta-DOR)
- 5.5.4 Differenced Range Versus Integrated Doppler
- 5.5.5 Open-loop Receiver (Radio Science Receiver)
- 5.5.6 Media Calibration
- 5.5.7 Spacecraft Trajectory
- 5.5.8 Calibration Data Sets
- Appendix 5A Spacecraft Telecommunications System and Radio Science Flight Instrument for Several Deep Space Missions
-
6 Future Directions in Radio Science Investigations and Technologies
- 6.1 Fundamental Questions toward a Future Exploration Roadmap
- 6.1.1 Fundamental Questions about the Utility of RS Techniques
- 6.1.2 Possible Triggers for Specific Innovations for Future Investigations
- 6.1.3 Possible Synergies with Other Fields
- 6.1.4 Examining Relevant Methodologies
- 6.2 Science-Enabling Technologies: Constellations of Small Spacecraft
- 6.2.1 Constellations for Investigations of Atmospheric Structure and Dynamics
- 6.2.2 Constellations for Investigations of Interior Structure and Dynamics
- 6.2.3 Constellations for Simultaneous and Differential Measurements
- 6.2.4 Constellations of Entry Probes and Atmospheric Vehicles
- 6.2.5 Constellations for Investigations of Planetary Surface
- 6.3 Science-enabling via Optical Links
- 6.4 Science-enabling Calibration Techniques
- 6.4.1 Earth’s Troposphere Water Vapor Radiometry
- 6.4.2 Antenna Mechanical Noise
- 6.4.3 Advanced Ranging
- 6.5 Summary
- Appendix 6A The National Academies Planetary Science Decadal Survey, Radio Science Contribution, 2009: Planetary Radio Science: Investigations of Interiors, Surfaces, Atmospheres, Rings, and Environments
- 6A.1 Summary
- 6A.2 Background
- 6A.3 Historical Opportunities and Discoveries
- 6A.4 Recent Opportunities and Discoveries
- 6A.5 Future Opportunities
- 6A.6 Technological Advances in Flight Instrumentation
- 6A.7 The Future of Flight Instrumentation
- 6A.7.1 Crosslink Radio Science
- 6A.7.2 Ka-band Transponders and Other Instrumentation
- 6A.8 Ground Instrumentation
- 6A.8.1 NASA’s Deep Space Network
- 6A.8.2 Other Facilities
- 6A.9 New Communications Architectures: Arrays and Optical Links
- 6A.10 Conclusion and Goals
- Appendix 6B The National Academies Planetary Science Decadal Survey, Radio Science Contribution: Solar System Interiors, Atmospheres, and Surfaces Investigations via Radio Links: Goals for the Next Decade
- 6B.1 Summary
- 6B.2 Current Status of RS Investigations
- 6B.3 Key Science Goals for the Next Decade
- 6B.4 Radio Science Techniques for Achieving the Science Goals of the Next Decade
- 6B.5 Technology Development Needed in the Next Decade
- References
- Acronyms and Abbreviations
- Index
- End User License Agreement
Product information
- Title: Radio Science Techniques for Deep Space Exploration
- Author(s):
- Release date: March 2022
- Publisher(s): Wiley
- ISBN: 9781119734147
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