{"product_id":"deep-space-optical-communications-11-jpl-deepspace-communications-and-navigation-series-9780470040027","title":"Deep Space Optical Communications 11 JPL","description":"\u003cb\u003eBook Synopsis\u003c\/b\u003e\u003cbr\u003eThis is the first book that specifically addresses Optical Communications from planetary distances.   There are specific technologies and requirements that are unique to deep-space links and differ from either Earth-orbit to Earth, or terrestrial, optical communication links.\u003cbr\u003e\u003cbr\u003e\u003cb\u003eTable of Contents\u003c\/b\u003e\u003cbr\u003eForeword.  \u003cp\u003ePreface.\u003c\/p\u003e \u003cp\u003eAcknowledgments.\u003c\/p\u003e \u003cp\u003eContributors.\u003c\/p\u003e \u003cp\u003eChapter 1 : Introduction (James R . Lesh).\u003c\/p\u003e \u003cp\u003e1.1 Motivation for Increased Communications.\u003c\/p\u003e \u003cp\u003e1.2 History of JPL Optical Communications Activities.\u003c\/p\u003e \u003cp\u003e1.3 ComponentlSubsystem Technologies.\u003c\/p\u003e \u003cp\u003e1.3.1 Laser Transmitters.\u003c\/p\u003e \u003cp\u003e1.3.2 Spacecraft Telescopes.\u003c\/p\u003e \u003cp\u003e1.3.3 Acquisition, Tracking. and Pointing.\u003c\/p\u003e \u003cp\u003e1.3.4 Detectors.\u003c\/p\u003e \u003cp\u003e1.3.5 Filters.\u003c\/p\u003e \u003cp\u003e1.3.6 Error Correction Coding.\u003c\/p\u003e \u003cp\u003e1.4 Flight Terminal Developments.\u003c\/p\u003e \u003cp\u003e1.4.1 Optical Transceiver Package (OPTRANSPAC).\u003c\/p\u003e \u003cp\u003e1.4.2 Optical Communications Demonstrator (OCD).\u003c\/p\u003e \u003cp\u003e1.4.3 Lasercom Test and Evaluation Station (LTES).\u003c\/p\u003e \u003cp\u003e1.4.4 X2000 Flight Terminal.\u003c\/p\u003e \u003cp\u003e1.4.5 International Space Station Flight Terminal.\u003c\/p\u003e \u003cp\u003e1.5 Reception System and Network Studies.\u003c\/p\u003e \u003cp\u003e1.5.1 Ground Telescope Cost Model.\u003c\/p\u003e \u003cp\u003e1.5.2 Deep Space Optical Reception Antenna (DSORA).\u003c\/p\u003e \u003cp\u003e1.5.3 Deep Space Relay Satellite System (DSRSS) Studies.\u003c\/p\u003e \u003cp\u003e1.5.4 Ground-Based Antenna Technology Study (GBATS).\u003c\/p\u003e \u003cp\u003e1.5.5 Advanced Communications Benefits Study (ACBS).\u003c\/p\u003e \u003cp\u003e1.5.6 Earth Orbit Optical Reception Terminal (EOORT) Study.\u003c\/p\u003e \u003cp\u003e1.5 .7 EOORT Hybrid Study.\u003c\/p\u003e \u003cp\u003e1.5.8 Spherical Primary Ground Telescope.\u003c\/p\u003e \u003cp\u003e1.5.9 Space-Based versus Ground-Based Reception Trades.\u003c\/p\u003e \u003cp\u003e1.6 Atmospheric Transmission.\u003c\/p\u003e \u003cp\u003e1.7 Background Studies.\u003c\/p\u003e \u003cp\u003e1.8 Analysis Tools.\u003c\/p\u003e \u003cp\u003e1.\u003ci\u003e9 System-Level Studies.\u003c\/i\u003e\u003c\/p\u003e \u003cp\u003e1.9.1 Venus Radar Mapping (VRM) Mission Study.\u003c\/p\u003e \u003cp\u003e1.9.2 Synthetic Aperture Radar-C (SIR-C) Freeflyer.\u003c\/p\u003e \u003cp\u003e1.9.3 ER-2 to Ground Study.\u003c\/p\u003e \u003cp\u003e1.9.4 Thousand Astronomical Unit (TAU) Mission and Interstellar Mission Studies.\u003c\/p\u003e \u003cp\u003e1.1 0 System-Level Demonstrations.\u003c\/p\u003e \u003cp\u003e1 .1 0. 1 Galileo Optical Experiment (GOPEX).\u003c\/p\u003e \u003cp\u003e1.10.2 Compensated Earth-Moon-Earth Retro-Reflector Laser Link (CEMERLL).\u003c\/p\u003e \u003cp\u003e1.1 0.3 Groundlorbiter Lasercomm Demonstration (GOLD).\u003c\/p\u003e \u003cp\u003e1.10 .4 Ground-Ground Demonstrations.\u003c\/p\u003e \u003cp\u003e1.11 Other Telecommunication Functions.\u003c\/p\u003e \u003cp\u003e1.11.1 Opto-Metric Navigation.\u003c\/p\u003e \u003cp\u003e1.11.2 Light Science.\u003c\/p\u003e \u003cp\u003e1.12 The Future.\u003c\/p\u003e \u003cp\u003e1.12.1 Optical Communications Telescope Facility (OCTL).\u003c\/p\u003e \u003cp\u003e1.12.2 Unmanned Aria1 Vehicle (UAVFGround Demonstration.\u003c\/p\u003e \u003cp\u003e1.12.3 Adaptive Optics.\u003c\/p\u003e \u003cp\u003e1.12.4 Optical Receiver and Dynamic Detector Array.\u003c\/p\u003e \u003cp\u003e1.1 2.5 Alternate Ground-Reception Systems.\u003c\/p\u003e \u003cp\u003e1.13 Mars Laser Communication Demonstration.\u003c\/p\u003e \u003cp\u003e1.14 Summary of Following Chapters.\u003c\/p\u003e \u003cp\u003eReferences.\u003c\/p\u003e \u003cp\u003eChapter 2: Link and System Design (Chien-Chung Chen).\u003c\/p\u003e \u003cp\u003e2.1 Overview of Deep-Space Lasercom Link.\u003c\/p\u003e \u003cp\u003e2.2 Communications Link Design.\u003c\/p\u003e \u003cp\u003e2.2.1 Link Equation and Receive Signal Power.\u003c\/p\u003e \u003cp\u003e2.2.2 Optical-Receiver Sensitivity.\u003c\/p\u003e \u003cp\u003e2.2.2.1 Photon Detection Sensitivity.\u003c\/p\u003e \u003cp\u003e2.2.2.2 Modulation Format.\u003c\/p\u003e \u003cp\u003e2.2.2.3 Background Noise Control.\u003c\/p\u003e \u003cp\u003e2.2.3 Link Design Trades.\u003c\/p\u003e \u003cp\u003e2.2.3.1 Operating Wavelength.\u003c\/p\u003e \u003cp\u003e2.2.3.2 Transmit Power and Size of Transmit and Receive Apertures.\u003c\/p\u003e \u003cp\u003e2.2.3.3 Receiver Optical Bandwidth and Field of View versus Signal Throughput.\u003c\/p\u003e \u003cp\u003e2.2.3.4 Modulation and Coding.\u003c\/p\u003e \u003cp\u003e2.2.4 Communications Link Budget.\u003c\/p\u003e \u003cp\u003e2.2.5 Link Availability Considerations.\u003c\/p\u003e \u003cp\u003e2.2.5.1 Short-Term Data Outages.\u003c\/p\u003e \u003cp\u003e2.2.5.2 Weather-Induced Outages.\u003c\/p\u003e \u003cp\u003e2.2.5.3 Other Long-Term Outages.\u003c\/p\u003e \u003cp\u003e2.2.5.4 Critical-Mission-Phase Coverage.\u003c\/p\u003e \u003cp\u003e2.3 Beam Pointing and Tracking.\u003c\/p\u003e \u003cp\u003e2.3.1 Downlink Beam Pointing.\u003c\/p\u003e \u003cp\u003e2.3.1.1 Jitter Isolation and Rejection.\u003c\/p\u003e \u003cp\u003e2.3.1.2 Precision Beam Pointing and Point Ahead.\u003c\/p\u003e \u003cp\u003e2.3.2 Uplink Beam Pointing.\u003c\/p\u003e \u003cp\u003e2.3.3 Pointing Acquisition.\u003c\/p\u003e \u003cp\u003e2.4 Other Design Drivers and Considerations.\u003c\/p\u003e \u003cp\u003e2.4.1 System Mass and Power.\u003c\/p\u003e \u003cp\u003e2.4.2 Impact on Spacecraft Design.\u003c\/p\u003e \u003cp\u003e2.4.3 Laser Safety.\u003c\/p\u003e \u003cp\u003e2.5 Summary.\u003c\/p\u003e \u003cp\u003eReferences.\u003c\/p\u003e \u003cp\u003eChapter 3: The Atmospheric Channel (Abhijit Biswas and Sabino Piazzolla).\u003c\/p\u003e \u003cp\u003e3.1 Cloud Coverage Statistics.\u003c\/p\u003e \u003cp\u003e3.1.1 National Climatic Data Center Data Set.\u003c\/p\u003e \u003cp\u003e3.1.2 Single-Site and Two-Site Diversity Statistics.\u003c\/p\u003e \u003cp\u003e3.1.3 Three-Site Diversity.\u003c\/p\u003e \u003cp\u003e3.1.4 NCDC Analysis Conclusion.\u003c\/p\u003e \u003cp\u003e3.1.5 Cloud Coverage Statistics by Satellite Data Observation.\u003c\/p\u003e \u003cp\u003e3.2 Atmospheric Transmittance and Sky Radiance.\u003c\/p\u003e \u003cp\u003e3.2.1 Atmospheric Transmittance.\u003c\/p\u003e \u003cp\u003e3.2.2 Molecular Absorption and Scattering.\u003c\/p\u003e \u003cp\u003e3.2.3 Aerosol Absorption and Scattering.\u003c\/p\u003e \u003cp\u003e3.2.3.1 Atmospheric Attenuation Statistics.\u003c\/p\u003e \u003cp\u003e3.2.4 Sky Radiance.\u003c\/p\u003e \u003cp\u003e3.2.4.1 Sky Radiance Statistics.\u003c\/p\u003e \u003cp\u003e3.2.5 Point Sources of Background Radiation.\u003c\/p\u003e \u003cp\u003e3.3 Atmospheric Issues on Ground Telescope Site Selection for an Optical Deep Space Network.\u003c\/p\u003e \u003cp\u003e3.3.1 Optical Deep Space Network.\u003c\/p\u003e \u003cp\u003e3.3.2 Data RateJBER of a Mission.\u003c\/p\u003e \u003cp\u003e3.3.3 Telescope Site Location.\u003c\/p\u003e \u003cp\u003e3.3.4 Network Continuity and Peaks.\u003c\/p\u003e \u003cp\u003e3.4 Laser Propagation Through the Turbulent Atmosphere.\u003c\/p\u003e \u003cp\u003e3.4.1 Atmospheric Turbulence.\u003c\/p\u003e \u003cp\u003e3.4.2 Atmospheric \"Seeing\" Effects.\u003c\/p\u003e \u003cp\u003e3.4.3 Optical Scintillation or Irradiance Fluctuations.\u003c\/p\u003e \u003cp\u003e3.4.4 Atmospheric Turbulence Induced Angle of Arrival.\u003c\/p\u003e \u003cp\u003eReferences.\u003c\/p\u003e \u003cp\u003eChapter 4: Optical Modulation and Coding (Samuel J . Dolinar. Jon Hamkins. Bruce E . Moision and Victor A . Vilnrotter).\u003c\/p\u003e \u003cp\u003e4.1 Introduction.\u003c\/p\u003e \u003cp\u003e4.2 Statistical Models for the Detected Optical Field.\u003c\/p\u003e \u003cp\u003e4.2.1 Quantum Models of the Optical Field.\u003c\/p\u003e \u003cp\u003e4.2.1.1 Quantization of the Electric Field.\u003c\/p\u003e \u003cp\u003e4.2.1.2 The Coherent State Representation of a Single Field Mode.\u003c\/p\u003e \u003cp\u003e4.2.1.3 Quantum Representation of Thermal Noise.\u003c\/p\u003e \u003cp\u003e4.2.1.4 Quantum Representation of Signal Plus Thermal Noise.\u003c\/p\u003e \u003cp\u003e4.2.2 Statistical Models for Direct Detection.\u003c\/p\u003e \u003cp\u003e4.2.2.1 The Poisson Channel Model for Ideal Photodetectors or Ideal PMTs.\u003c\/p\u003e \u003cp\u003e4.2.2.2 The McIntyre-Conradi Model for APD Detectors.\u003c\/p\u003e \u003cp\u003e4.2.2.3 The Webb, McIntyre, and Conradi Approximation to the McIntyre-Conradi Model.\u003c\/p\u003e \u003cp\u003e4.2.2.4 The WMC Plus Gaussian Approximation.\u003c\/p\u003e \u003cp\u003e4.2.2.5 Additive White Gaussian Noise Approximation.\u003c\/p\u003e \u003cp\u003e4.2.3 Summary of Statistical Models.\u003c\/p\u003e \u003cp\u003e4.3 Modulation Formats.\u003c\/p\u003e \u003cp\u003e4.3.1 On-Off Keying (OOK).\u003c\/p\u003e \u003cp\u003e4.3.2 Pulse-Position Modulation (PPM).\u003c\/p\u003e \u003cp\u003e4.3.3 Differential PPM (DPPM).\u003c\/p\u003e \u003cp\u003e4.3.4 Overlapping PPM (OPPM).\u003c\/p\u003e \u003cp\u003e4.3.5 Wavelength Shift Keying (WSK).\u003c\/p\u003e \u003cp\u003e4.3.6 Combined PPM and WSK.\u003c\/p\u003e \u003cp\u003e4.4 Rate Limits Imposed by Constraints on Modulation.\u003c\/p\u003e \u003cp\u003e4.4.1 Shannon Capacity.\u003c\/p\u003e \u003cp\u003e4.4.1.1 Characterizing Capacity: Fixed Duration Edges.\u003c\/p\u003e \u003cp\u003e4.4.1.2 Characterizing Capacity: Variable Duration Edges.\u003c\/p\u003e \u003cp\u003e4.4.1.3 Characterizing Capacity: Probabilistic Characterization.\u003c\/p\u003e \u003cp\u003e4.4.1.4 Characterizing Capacity: Energy Efficiency.\u003c\/p\u003e \u003cp\u003e4.4.2 Constraints.\u003c\/p\u003e \u003cp\u003e4.4.2.1 Dead Time.\u003c\/p\u003e \u003cp\u003e4.4.2.2 Runlength.\u003c\/p\u003e \u003cp\u003e4.4.3 Modulation Codes.\u003c\/p\u003e \u003cp\u003e4.4.3.1 M-ary PPM with Deadtime.\u003c\/p\u003e \u003cp\u003e4.4.3.2 M-ary DPPM with Deadtime.\u003c\/p\u003e \u003cp\u003e4.4.3.3 Synchronous Variable-Length Codes.\u003c\/p\u003e \u003cp\u003e4.5 Performance of Uncoded Optical Modulations.\u003c\/p\u003e \u003cp\u003e4.5.1 Direct Detection of OOK on the Poisson Channel.\u003c\/p\u003e \u003cp\u003e4.5.2 Direct Detection of PPM.\u003c\/p\u003e \u003cp\u003e4.5.2.1 Poisson Channel.\u003c\/p\u003e \u003cp\u003e4.5.2.2 AWGN Channel.\u003c\/p\u003e \u003cp\u003e4.5.3 Direct Detection of Combined PPM and WSK.\u003c\/p\u003e \u003cp\u003e4.5.4 Performance of Modulations Using Receivers Based on Quantum Detection Theory.\u003c\/p\u003e \u003cp\u003e4.5.4.1 Receivers Based on Quantum Detection Theory.\u003c\/p\u003e \u003cp\u003e4.5.4.2 Performance of Representative Modulations.\u003c\/p\u003e \u003cp\u003e4.6 Optical Channel Capacity.\u003c\/p\u003e \u003cp\u003e4.6.1 Capacity of the PPM Channel: General Formulas.\u003c\/p\u003e \u003cp\u003e4.6.2 Capacity of Soft-Decision PPM: Specific Channel Models.\u003c\/p\u003e \u003cp\u003e4.6.2.1 Poisson Channel.\u003c\/p\u003e \u003cp\u003e4.6.2.2 AWGN Channel.\u003c\/p\u003e \u003cp\u003e4.6.3 Hard-Decision Versus Soft-Decision Capacity.\u003c\/p\u003e \u003cp\u003e4.6.4 Losses Due to Using PPM.\u003c\/p\u003e \u003cp\u003e4.6.5 Capacity of the Binary Channel with Quantum Detection.\u003c\/p\u003e \u003cp\u003e4.7 Channel Codes for Optical Modulations.\u003c\/p\u003e \u003cp\u003e4.7.1 Reed-Solomon Codes.\u003c\/p\u003e \u003cp\u003e4.7.2 Turbo and Turbo-Like Codes for Optical Modulations.\u003c\/p\u003e \u003cp\u003e4.7.2.1 Parallel Concatenated (Turbo) Codes.\u003c\/p\u003e \u003cp\u003e4.7.2.2 Serially Concatenated Codes with Iterative Decoding.\u003c\/p\u003e \u003cp\u003e4.8 Performance of Coded Optical Modulations.\u003c\/p\u003e \u003cp\u003e4.8.1 Parameter Selection.\u003c\/p\u003e \u003cp\u003e4.8.2 Estimating Performance.\u003c\/p\u003e \u003cp\u003e4.8.2.1 Reed-Solomon Codes.\u003c\/p\u003e \u003cp\u003e4.8.2.2 Iterative Codes.\u003c\/p\u003e \u003cp\u003e4.8.3 Achievable Data Rates Versus Average Signal Power.\u003c\/p\u003e \u003cp\u003eReferences.\u003c\/p\u003e \u003cp\u003eChapter 5: Flight Transceiver (Hamid Hemmati. Gerardo G . Ortiz. William T . Roberts, Malcolm W . Wright, and Shinhak Lee)\u003c\/p\u003e \u003cp\u003e5.1 Optomechanical Subsystem (Hamid Hemmati).\u003c\/p\u003e \u003cp\u003e5.1 . 1 Introduction.\u003c\/p\u003e \u003cp\u003e5.1.2 Optical Beam Paths.\u003c\/p\u003e \u003cp\u003e5.1.3 Optical Design Requirements, Design Drivers, and Challenges.\u003c\/p\u003e \u003cp\u003e5.1.4 Optical Design Drivers and Approaches.\u003c\/p\u003e \u003cp\u003e5.1.5 Transmit-Receive-Isolation.\u003c\/p\u003e \u003cp\u003e5.1.6 Stray-Light Control.\u003c\/p\u003e \u003cp\u003e5.1.6.1 Operation at Small Sun Angles.\u003c\/p\u003e \u003cp\u003e5.1.6.2 Surface Cleanliness Requirements.\u003c\/p\u003e \u003cp\u003e5.1.7 Transmission, Alignment, and Wavefront Quality Budgets.\u003c\/p\u003e \u003cp\u003e5.1.8 Efficient Coupling of Lasers to Obscured Telescopes.\u003c\/p\u003e \u003cp\u003e5.1.8.1 Axicon Optical Element.\u003c\/p\u003e \u003cp\u003e5.1.8.2 Sub-Aperture Illumination.\u003c\/p\u003e \u003cp\u003e5.1.8.3 Prism Beam Slicer.\u003c\/p\u003e \u003cp\u003e5.1.8.4 Beam Splitter\/Combiner.\u003c\/p\u003e \u003cp\u003e5.1.9 Structure, Materials, and Structural Analysis.\u003c\/p\u003e \u003cp\u003e5.1.10 Use of Fiber Optics.\u003c\/p\u003e \u003cp\u003e5.1.1 1 Star-Tracker Optics for Acquisition and Tracking.\u003c\/p\u003e \u003cp\u003e5.1 . 12 Thermal Management.\u003c\/p\u003e \u003cp\u003e5.1.13 Optical System Design Example.\u003c\/p\u003e \u003cp\u003e5.1.13.1 Afocal Fore-Optics.\u003c\/p\u003e \u003cp\u003e5.1.13.2 Receiver Channel.\u003c\/p\u003e \u003cp\u003e5.1.13.3 Stellar Reference Channel.\u003c\/p\u003e \u003cp\u003e5.1.13.4 Align and Transmit Channels.\u003c\/p\u003e \u003cp\u003e5.1.13.5 Folded Layouts.\u003c\/p\u003e \u003cp\u003e5.1.13.6 Tolerance Sensitivity Analysis.\u003c\/p\u003e \u003cp\u003e5.1.13.7 Thermal Soak Sensitivity Analysis.\u003c\/p\u003e \u003cp\u003e5.1.13.8 Solid Model of System.\u003c\/p\u003e \u003cp\u003e5.2 Laser Transmitter (Hamid Hemmati).\u003c\/p\u003e \u003cp\u003e5.2.1 Introduction.\u003c\/p\u003e \u003cp\u003e5.2.2 Requirements and Challenges.\u003c\/p\u003e \u003cp\u003e5.2.3 Candidate Laser Transmitter Sources.\u003c\/p\u003e \u003cp\u003e5.2.3.1 Pulsed Laser Transmitters.\u003c\/p\u003e \u003cp\u003e5.2.3.2 Fiber- Waveguide Amplifiers.\u003c\/p\u003e \u003cp\u003e5.2.3.3 Bulk-Crystal Amplifiers.\u003c\/p\u003e \u003cp\u003e5.2.3.4 Semiconductor Optical Amplifiers.\u003c\/p\u003e \u003cp\u003e5.2.4 Lasers for Coherent Communications.\u003c\/p\u003e \u003cp\u003e5.2.5 Laser Modulators.\u003c\/p\u003e \u003cp\u003e5.2.6 Efficiency.\u003c\/p\u003e \u003cp\u003e5.2.7 Laser Timing Jitter Control.\u003c\/p\u003e \u003cp\u003e5.2.7.1 Jitter Control Options.\u003c\/p\u003e \u003cp\u003e5.2.8 Redundancy.\u003c\/p\u003e \u003cp\u003e5.2.9 Thermal Management.\u003c\/p\u003e \u003cp\u003e5.3 Deep-Space Acquisition, Tracking, and Pointing (Gerardo G . Ortiz and Shinhak Lee).\u003c\/p\u003e \u003cp\u003e5.3.1 Unique Challenges of Deep Space Optical Beam Pointing.\u003c\/p\u003e \u003cp\u003e5.3.1.1 State-of-the-Art ATP Performance.\u003c\/p\u003e \u003cp\u003e5.3.2 Link Overview and System Requirements.\u003c\/p\u003e \u003cp\u003e5.3.2.1 Pointing Requirement.\u003c\/p\u003e \u003cp\u003e5.3.2.2 Pointing-Error Budget Allocations.\u003c\/p\u003e \u003cp\u003e5.3.3 ATP System.\u003c\/p\u003e \u003cp\u003e5.3.3.1 Pointing Knowledge Reference Sources.\u003c\/p\u003e \u003cp\u003e5.3.3.2 Pointing System Architecture.\u003c\/p\u003e \u003cp\u003e5.3.3.3 Design Considerations.\u003c\/p\u003e \u003cp\u003e5.3.4 Cooperative Beacon (Ground Laser) Tracking.\u003c\/p\u003e \u003cp\u003e5.3.5 Noncooperative Beacon Tracking.\u003c\/p\u003e \u003cp\u003e5.3.5.1 Earth Tracker-Visible Spectrum.\u003c\/p\u003e \u003cp\u003e5.3.5.2 Star Tracker.\u003c\/p\u003e \u003cp\u003e5.3.5.3 Earth Tracker-Long Wavelength Infrared Band.\u003c\/p\u003e \u003cp\u003e5.3.6 ATP Technology Demonstrations.\u003c\/p\u003e \u003cp\u003e5.3.6.1 Reduced Complexity ATP Architecture.\u003c\/p\u003e \u003cp\u003e5.3.6.2 Centroiding Algorithms-Spot Model Method.\u003c\/p\u003e \u003cp\u003e5.3.6.3 High Bandwidth, Windowing, CCD-Based Camera.\u003c\/p\u003e \u003cp\u003e5.3.6.4 Accelerometer-Assisted Beacon Tracking.\u003c\/p\u003e \u003cp\u003e5.4 Flight Qualification (Hamid Hemmati, William T . Roberts, and Malcolm W . Wright).\u003c\/p\u003e \u003cp\u003e5.4.1 Introduction.\u003c\/p\u003e \u003cp\u003e5.4.2 Approaches to Flight Qualification.\u003c\/p\u003e \u003cp\u003e5.4.3 Flight Qualification of Electronics and Opto-Electronic Subsystem.\u003c\/p\u003e \u003cp\u003e5.4.3.1 MIL-PRF-19500.\u003c\/p\u003e \u003cp\u003e5.4.3.2 MIL STD 750.\u003c\/p\u003e \u003cp\u003e5.4.3.3 MIL STD 883.\u003c\/p\u003e \u003cp\u003e5.4.3.4 Telcordia.\u003c\/p\u003e \u003cp\u003e5.4.3.5 NASA Electronics Parts and Packaging (NEPP).\u003c\/p\u003e \u003cp\u003e5.4.4 Number of Test Units.\u003c\/p\u003e \u003cp\u003e5.4.5 Space Environments.\u003c\/p\u003e \u003cp\u003e5.4.5.1 Environmental Requirements.\u003c\/p\u003e \u003cp\u003e5.4.5.2 Ionizing Radiation.\u003c\/p\u003e \u003cp\u003e5.4.5.3 Vibration Environment.\u003c\/p\u003e \u003cp\u003e5.4.5.4 Mechanical, Thermal, and Pyro Shock Environment.\u003c\/p\u003e \u003cp\u003e5.4.5.5 Thermal Gradients Environment.\u003c\/p\u003e \u003cp\u003e5.4.5.6 Depressurization Environment.\u003c\/p\u003e \u003cp\u003e5.4.5.7 Electric and Magnetic Field Environment.\u003c\/p\u003e \u003cp\u003e5.4.5.8 Outgassing.\u003c\/p\u003e \u003cp\u003e5.4.6 Flight Qualification of Detectors.\u003c\/p\u003e \u003cp\u003e5.4.6.1 Flight Qualification Procedures.\u003c\/p\u003e \u003cp\u003e5.4.6.2 Detector Radiation Testing.\u003c\/p\u003e \u003cp\u003e5.4.7 Flight Qualification of Laser Systems.\u003c\/p\u003e \u003cp\u003e5.4.7.1 Past Laser Systems Flown in Space.\u003c\/p\u003e \u003cp\u003e5.4.7.2 Design of Semiconductor Lasers for High Reliability Applications.\u003c\/p\u003e \u003cp\u003e5.4.7.3 Degradation Mechanisms.\u003c\/p\u003e \u003cp\u003e5.4.7.4 Qualification Process for Lasers.\u003c\/p\u003e \u003cp\u003e5.4.8 Flight Qualification of Optics.\u003c\/p\u003e \u003cp\u003eReferences.\u003c\/p\u003e \u003cp\u003eChapter 6: Earth Terminal Architectures (Keith E . Wilson, Abhijit Biswas, Andrew A . Gray, Victor A . Vilnrotter, Chi-Wung Lau. Mera Srinivasan, and William H . Farr).\u003c\/p\u003e \u003cp\u003e6.1 Introduction (Keith E . Wilson).\u003c\/p\u003e \u003cp\u003e6.1.1 Single-Station Downlink Reception and Uplink Transmission (Keith E . Wilson).\u003c\/p\u003e \u003cp\u003e6.1.1.1 Introduction.\u003c\/p\u003e \u003cp\u003e6.1.1.2 Deep-Space Optical Ground Receivers.\u003c\/p\u003e \u003cp\u003e6.1.1.3 Mitigating Cloud Cover and Sky Background Effects at the Receiver.\u003c\/p\u003e \u003cp\u003e6.1.1.4 Daytime Sky Background Effects.\u003c\/p\u003e \u003cp\u003e6.1.1.5 Earth-Orbiting and Airborne Receivers.\u003c\/p\u003e \u003cp\u003e6.1.1.6 Uplink Beacon and Command.\u003c\/p\u003e \u003cp\u003e6.1.1.7 Techniques for Mitigating Atmospheric Effects.\u003c\/p\u003e \u003cp\u003e6.1.1.8 Adaptive Optics.\u003c\/p\u003e \u003cp\u003e6.1.1.9 Multiple-Beam Propagation.\u003c\/p\u003e \u003cp\u003e6.1.1.10 Safe Laser Beam Propagation into Space.\u003c\/p\u003e \u003cp\u003e6.1.1. I 1 Concept Validation Experiments Supporting Future Deep-Space Optical links.\u003c\/p\u003e \u003cp\u003e6.1.1.12 Conclusion.\u003c\/p\u003e \u003cp\u003e6.1.2 Optical-Array Receivers for Deep-Space Communication (Victor A . Vilnrotter, Chi-Wung Lau, and Meera Srinivasan).\u003c\/p\u003e \u003cp\u003e6.1.2.1 Introduction.\u003c\/p\u003e \u003cp\u003e6.1.2.2 The Optical-Array Receiver Concept.\u003c\/p\u003e \u003cp\u003e6.1.2.3 Aperture-Plane Expansions.\u003c\/p\u003e \u003cp\u003e6.1.2.4 Array Receiver Performance.\u003c\/p\u003e \u003cp\u003e6.1.2.5 Conclusions.\u003c\/p\u003e \u003cp\u003e6.2 Photodetectors.\u003c\/p\u003e \u003cp\u003e6.2.1 Single-Element Detectors (Abhijit Biswas and William H . Farr).\u003c\/p\u003e \u003cp\u003e6.2.1.1 Deep-Space Detector Requirements and Challenges.\u003c\/p\u003e \u003cp\u003e6.2.1.2 Detector System Dependencies.\u003c\/p\u003e \u003cp\u003e6.2.1.3 Detectors for Deep-Space Communications.\u003c\/p\u003e \u003cp\u003e6.2.2 Focal-Plane Detector Arrays for Communication Through Turbulence (Victor A . Vilnrotter and Meera Srinivasan).\u003c\/p\u003e \u003cp\u003e6.2.2.1 Introduction.\u003c\/p\u003e \u003cp\u003e6.2.2.2 Optical Direct Detection with Focal-Plane Arrays.\u003c\/p\u003e \u003cp\u003e6.2.2.3 Numerical Results.\u003c\/p\u003e \u003cp\u003e6.2.2.4 Summary And Conclusions.\u003c\/p\u003e \u003cp\u003e6.3 Receiver Electronics (Andrew A . Gray, Victor A . Vilnrotter, and Meera Srinivasan).\u003c\/p\u003e \u003cp\u003e6.3.1 Introduction.\u003c\/p\u003e \u003cp\u003e6.3.2 Introduction to Discrete-Time Demodulator Architectures.\u003c\/p\u003e \u003cp\u003e6.3.3 Discrete-Time Synchronization and Post-Detection Filtering Overview.\u003c\/p\u003e \u003cp\u003e6.3.3.1 Discrete-Time Post-Detection Filtering.\u003c\/p\u003e \u003cp\u003e6.3.3.2 Slot and Symbol Synchronization and Decision Processing.\u003c\/p\u003e \u003cp\u003e6.3.4 Discrete-Time Demodulator Variations.\u003c\/p\u003e \u003cp\u003e6.3.5 Discrete-Time Demodulator with Time-Varying Post-Detection Filter.\u003c\/p\u003e \u003cp\u003e6.3.6 Parallel Discrete-Time Demodulator Architectures.\u003c\/p\u003e \u003cp\u003e6.3.7 Asynchronous Discrete-Time Processing.\u003c\/p\u003e \u003cp\u003e6.3.8 Parallel Discrete-Time Demodulator Architectures.\u003c\/p\u003e \u003cp\u003e6.3.8.1 Simple Example Architecture.\u003c\/p\u003e \u003cp\u003e6.3.8.2 Performance with a Simple Optical Channel Model.\u003c\/p\u003e \u003cp\u003e6.3.8.3 Evolved Parallel Architectures.\u003c\/p\u003e \u003cp\u003e6.3.9 Primary System Models and Parameters.\u003c\/p\u003e \u003cp\u003e6.3.10 Conclusion and Future Work.\u003c\/p\u003e \u003cp\u003eReferences.\u003c\/p\u003e \u003cp\u003eChapter 7: Future Prospects and Applications (Hamid Hemmati and Abhijit Biswas).\u003c\/p\u003e \u003cp\u003e7.1 Current and Upcoming Projects in the United States, Europe. and Japan.\u003c\/p\u003e \u003cp\u003e7.1.1 LUCE (Laser Utilizing Communications Experiment).\u003c\/p\u003e \u003cp\u003e7.1.2 Mars Laser-Communication Demonstrator (MLCD).\u003c\/p\u003e \u003cp\u003e7.2 Airborne and Spaceborne Receivers.\u003c\/p\u003e \u003cp\u003e7.2.1 Advantages of Airborne and Spaceborne Receivers.\u003c\/p\u003e \u003cp\u003e7.2.2 Disadvantages of Airborne and Spaceborne Receivers.\u003c\/p\u003e \u003cp\u003e7.2.3 Airborne Terminals.\u003c\/p\u003e \u003cp\u003e7.2.3.1 Balloons.\u003c\/p\u003e \u003cp\u003e7.2.3.2 Airships.\u003c\/p\u003e \u003cp\u003e7.2.3.3 Airplanes.\u003c\/p\u003e \u003cp\u003e7.2.4 Spaceborne Receiver Terminals.\u003c\/p\u003e \u003cp\u003e7.2.5 Alternative Receiver Sites.\u003c\/p\u003e \u003cp\u003e7.3 Light Science.\u003c\/p\u003e \u003cp\u003e7.3.1 Light-Propagation Experiments.\u003c\/p\u003e \u003cp\u003e7.3.2 Occultation Experiments to Probe Planetary Atmospheres, Rings. Ionospheres. Magnetic Fields. and the Interplanetary Medium.\u003c\/p\u003e \u003cp\u003e7.3.2.1 Atmospheric Occultations.\u003c\/p\u003e \u003cp\u003e7.3.2.2 Ring-Investigation Experiments.\u003c\/p\u003e \u003cp\u003e7.3.3 Enhanced Knowledge of Solar-System-Object Masses and Gravitational Fields. Sizes. Shapes. and Surface Features.\u003c\/p\u003e \u003cp\u003e7.3.3.1 Improved Knowledge of Solar-System Body Properties.\u003c\/p\u003e \u003cp\u003e7.3.3.2 Optical Reference-Frame Ties..\u003c\/p\u003e \u003cp\u003e7.3.4 Tests of the Fundamental Theories: General Relativity, Gravitational Waves, Unified Field Theories, Astrophysics, and Cosmology.\u003c\/p\u003e \u003cp\u003e7.3.4.1 Tests of General Relativity and Unified Field Theories, Astrophysics, and Cosmology.\u003c\/p\u003e \u003cp\u003e7.3.4.2 Effects of Charged Particles on Electromagnetic Wave Propagation, Including Test of I\/f Hypothesis.\u003c\/p\u003e \u003cp\u003e7.3.5 Enhanced Solar-System Ephemerides.\u003c\/p\u003e \u003cp\u003e7.3.5.1 Science Benefits of Remote Optical Tracking: Ephemeris Improvement.\u003c\/p\u003e \u003cp\u003e7.3.6 Applications of Coherent Laser Communications Technology.\u003c\/p\u003e \u003cp\u003e7.4 Conclusions.\u003c\/p\u003e \u003cp\u003eReferences.\u003c\/p\u003e","brand":"John Wiley \u0026 Sons Inc","offers":[{"title":"Default Title","offer_id":49402269434199,"sku":"9780470040027","price":188.06,"currency_code":"GBP","in_stock":true}],"thumbnail_url":"\/\/cdn.shopify.com\/s\/files\/1\/0817\/1739\/5799\/files\/9780470040027.jpg?v=1730479898","url":"https:\/\/bookcurl.com\/products\/deep-space-optical-communications-11-jpl-deepspace-communications-and-navigation-series-9780470040027","provider":"Book Curl","version":"1.0","type":"link"}