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SPS Effects on Optical and Radio Astronomy
Cover
1
Title Page
3
Table of Contents
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Introduction and Summary
11
Workshop Opening Statement
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Introduction
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Background
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Organization of the Workshop
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Organization of the Report
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Basic Conclusions of the Workshop
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SPS Briefing Document - Radio and Optical Astronomy Effects
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Introduction
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General Characteristics of the SPS Reference System
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Satellite Optical Effects
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A. Diffuse Reflection
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B. Specular Reflction
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C. Diffuse Sky Brightness
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D. Satellite Thermal Infrared Emission
41
E. Ionosperic Infrared and Optical Emissions
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Radio Effects
43
A. Satellite Main Power Bean
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B. Satellite Harmonic Radiation
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C. Satellite Noise Radiation
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D. Rectenna Powre Beam Scattering
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E. Rectenna Harmonic Radiation
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F. Rectenna Noise Radiation
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Appendix: TIme-Varying Brightness of the Solar Collecting Array
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Invited Presentations of SPS Effects on Optical Astronomy
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Limitations of the Briefing Document's Characterization of the SPS Reference System
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Comments of the Effects of Increased Diffuse SKy Brightness of Fint Object Astronomical Observations
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Effects of the SPS on Ground-Based Astronomical Telescopes
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Infrared Astronomy
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Possible Impacts of the SPS on the Space Telescope
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Report of the Optical Astronomy Working Group
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The Nature of Astronomical Observations
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The Origin of SPS Effects on Optical Astronomy
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Impact Thresholds of the SPS on Optical Astronomy
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Effects on Optical Astronomy
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Recommendations and Remedies
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Report on SPS Effects on Aeronomy
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Introduction
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Effects on Aeronomy Observations
109
Invited Presentations on SPS Effects on Radio Astronomy
119
Microwave Power Transmission System
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SPS Noise and Harmonics
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SPS-Generated Field Strengths at 2.45Ghz, Typical Effects
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Interference Effects on Radio Astronomy Equipment
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Possible Overeload and Physical Damge of a Radio Astronomy Receiver Caused by the SPS
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Potential Impact of Out-Of-Band Radiation from the SPS At Arecibo Observatory
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THe Effects of te Proposed SPS on the VLA
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SPS Effects on Very-Long Baseline Interferometry
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Considerations Regarding Deep Space Communication and the SPS
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Report of the Radio Astronomy Working Group
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Summary Statement
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Actual Properties of the Microwave Power Transmission System
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Assignment of SPS Harmonic Frequencies
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Time-Variability of SPS Off-Axis Radiation and Intrinsic Multiple Satellite Effects
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The "Rusty Bolt" Effect
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Interference Rejection Properties Peculiar to Synthesis Arrays (as the VLA)
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Siting Considerations
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On Moving Radio Astronomy to the Lunar Far Side
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Appendix A: CCIR Reports on Radio Astronomy (Reports 223-4 and 224-4)
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A Note on CCIR Report 224-4 AND THE FUTURE
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A 10 TO 20 Year Protection
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223-4: Line Frequencies Arising From Natural Phenomena of Interest to Radioastronomy and Related Sciences
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Annex I The Neutral Hydrogen Line
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Annex II Th OH Lines in Radioastronomy
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Annex III Water Vapour Line at 22.235 GHz
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Annex IV The Formaldehyde Lines
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Annex V The Carbon Monoxide Lines
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Report 224-6 Charactertics on the Radioastronomy Services and Interference Protection Criteria
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Annex I Radio-frequency Lines of the Greatest Importance to Radioastronomy
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Appendix B: CCIR Reports on Deep-Space Research (Reports 365-3 and 685)
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Recommendation 365-3 Frequncies, Bndwidth and Protection Critieria for Manned And Unmanned Deep-Space Research
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Recommendation 364-3 Telecommunication Links for Manned and Unmanndd Near-Earth Research Satellites
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Report 685 Protection Criteria and Sharing Considerations Relating to Deep-Space Research
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Appendix C. Effect of SPS Transmissions on Radio Astronomical Resaerch
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Chairman's Note
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Effect of Solar Power Satellite transmissions on radio astronomical research
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1. Introduction
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2. The present proposals for a Solar Power Satellite System (SPS)
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3. Interference with radio telescopes
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4. Operational circumstances
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5. Filtering requirements
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6. Discussion
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7. Conclusions
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References and Notes
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Appendix D. National Academy of Sciences Report on SPS Effects
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Solar Power Satellite - Assessment of Potential for Interference to Radio Astronomy Observations
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Appendix E. Environmental Consideration for the Microwave Beam from a SPS
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Environmental Considerations for the Microwave Beam from a SPS
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Acknowledgments
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