Satellite-to-Ground Radiowave Propagation (2nd Edition)
This book is a follow-up to the award-winning first edition and is written as a comprehensive guide for those who need to obtain a working knowledge of radiowave propagation on satellite-to-ground links at frequencies above 1 GHz and as a reference book for experts in the field. To accomplish this, expanded sections of explanatory text, copiously illustrated, enable an undergraduate or non-specialist to grasp the fundamentals involved. An extensive reference list permits the expert to go to the source material should the level of enquiry go beyond the level of this book. The book is broken down into chapters that deal with the major propagation phenomena classes. After a broad introductory chapter, there are extensively updated chapters on ionospheric effects, clear air effects, attenuation effects and depolarisation effects. New chapters on mobile communications effects and optical communications effects are followed by a chapter on restoration of performance during impairments.
Inspec keywords: satellite communication; optical communication; radiowave propagation; ionospheric electromagnetic wave propagation
Other keywords: mobile satellite service propagation effects; depolarization effects; satellite-to-ground radiowave propagation; signal impairments; clear air effects; performance restoration; attenuation effects; radiowave Earth-space communications; optical communications propagation effects
Subjects: Optical communication; Radiowave propagation; Satellite communication systems
- Book DOI: 10.1049/PBEW054E
- Chapter DOI: 10.1049/PBEW054E
- ISBN: 9781849191500
- e-ISBN: 9781849191180
- Page count: 696
- Format: PDF
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Front Matter
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1 Radiowave Earth-space communications
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This chapter considers topics including artificial Earth satellites; orbits; antenna choice; frequency choice; polarisation choice, tracking choice; service choice; atmospheric characteristics and system planning.
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2 Ionospheric effects
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This chapter discusses ionospheric effects. The ionosphere is a region of ionized plasma that extends from roughly 50 to 2,000 km above the surface of the Earth. The boundary of the Earth's magnetic field within the solar wind is known as the magnetopause; between the magnetopause and the ionosphere is the magnetosphere. The magnetosphere extends about 10 Earth radii in the direction of the Sun, acting as a 'bow wave' against the solar wind. On the other side of the Earth, the magneto sphere streams backwards for about 60 Earth radii.
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3 Clear-air effects
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A radio signal that is transmitted approximately horizontally will consist of two basic components, a space wave (or direct wave) and a ground wave (or reflected wave). The constructive and destructive interference of these two signals continue alternately with distance from the antenna, giving rise to a rippling pattern of amplitude fluctuations centred about the inverse square loss value. At the optical range from the transmitter, where grazing incidence occurs, some components of the signal will be diffracted. The smooth ripple pattern is destroyed, and the loss in signal strength starts to exceed the inverse square law loss. At further distances still, scattering of the signal energy occurs from the non-uniform structure or turbulence of the atmosphere. This phenomenon is called tropospheric scatter and is of little direct relevance to satellite-to-ground propagation except for elevation angles below about 1°. The chapter gives a schematic of the three propagation ranges. As well as the scattering phenomenon, which was invoked to explain the reliable reception of radiowaves at distances well beyond the horizon, it was apparent that the radiowaves were bent, or refracted, as they passed through the atmosphere. The development of transmitting devices in the gigahertz range also highlighted the absorptive effect of the atmosphere, both in rain and in apparently clear-sky conditions. Later chapters will deal with the effect of rain and other particulates on radiowaves. In this chapter, only the effects of an apparently clear atmosphere on radiowave propagation are discussed.
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4 Attenuation effects
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There are a lot of atmospheric particles and possible weather effects that can exist on the path from a satellite to an earth station. We have seen that the clear-sky level of a signal from a satellite measured at an earth station can change appreciably over a day, a season and a year. So what baseline is set for the measurement of the signal attenuation? There are several measures for the change in signal level along the path. In absolute terms, the total attenuation along the path is the difference between the signal level at the earth station that would exist if there were a vacuum along the path from the satellite to the earth station and the signal level that is measured at the earth station. Total attenuation is the sum of every attenuating mechanism along the path. Excess attenuation is normally taken as the dif ference between the clear-sky level (which generally includes some clouds, gaseous attenuation and possibly low-level tropospheric scintillation) and the signal level in a significant attenuating event. If the cloud, gaseous attenuation and other low-level loss components can be assumed to be constant over the attenuating event, then the excess attenuation measures only the contribution due to significant tropospheric scintillation and rain effects. The excess attenuation of a radiowave passing through the atmosphere is made up of two principal components: absorption and scattering. Absorption takes place when the incident radiowave energy is transformed essentially into mechanical energy, thereby heating up the absorbing material. A radiowave is said to be scattered when its energy is redirected from the original propagation direction without losing any substantial energy to the scattering particle, or particles.
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5 Depolarization effects
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The rapid increase in the demand for telecommunications capacity, combined with the pressure to conserve the bandwidth used as much as possible, led to the concept of frequency reuse. On a satellite, this can be achieved in two ways: via spatial isolation or via polarization isolation. The polarization of a wave refers to the degree of non-randomness in the orientation of the electric vector. A completely unpolarized wave is one with no detectable preferred orientation sense of the electric vector. For frequency reuse with circular polarization, the two polarization senses are right hand circular polarization (RHCP) and left hand circular polarization (LHCP). A wave is RHCP if the sense of rotation of the electric field corresponds to the natural curl of the fingers of the right hand when the right thumb is pointed along the propagation direction. In essence, the electric field turns in the direction of rotation of a right-handed person opening a doorknob or screwing in a corkscrew into a bottle of wine. For LHCP, the same definition applies but with the left hand used instead of the right. For linear polarization, it is common to use vertical and horizontal as the two orthogonal reference axes.
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6 Mobile satellite service propagation effects
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Commercial global communications via satellite began with Intelsat in 1965, using large, fixed earth stations (~30 m in diameter) communicating with each other at C-band (6 GHz on the uplink and 4 GHz on the downlink) via spacecraft in geostationary orbit. The almost universal reach of geostationary satellites, coupled with the fact that the majority of the Earth's surface is water, made the move to offer telecommunications services to ships a logical progression. The original geostationary satellites were small and power limited, and there was clearly no way a 30-m diameter antenna could be located aboard even the largest ship. The solution reached was to offer services at L-band (between 1 and 2 GHz) rather than at C-band and to make the services narrowband (one equivalent voice channel) rather than attempting to provide broadband links.
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7 Optical communications propagation effects
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We will look at the differences between traditional microwave links and optical links, before moving on to review some of the parameters needed to calculate link impairments, and then present some calculation procedures for assessing optical link budgets.
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8 Restoration of performance during signal impairments
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The previous chapters have detailed the impact of various propagation impairment phenomena on the radiowave signals between earth stations (both fixed and mobile) and satellites. In each chapter, the system effects of the impairment in question were discussed and some means of reducing the impact of the impairment alluded to. This chapter will present in some detail the various schemes suggested and, in some cases, already implemented to restore performance during signal impairment.
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Appendix 1: Terms and definitions relating to space radiocommunications
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The information in this appendix was originally extracted from Report 204-6, of the same title, contained in Section 4A of Volume IV Part 1, Fixed Satellite Service and, more recently, updated with information from Recommendations 310-9 (Definitions of Terms Relating to Propagation in Non-Ionized Media) and 311-6 (Presentation of Data in Studies of Tropospheric-Wave Propagation), formerly in Volume V, 'Propagation in Non-Ionized Media', of the CCIR Green Books, and now in ITU-R Study Group 3 Recommendations.
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Appendix 2: Useful general equations
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This appendix considers equations that appear in the text or are referred to in the text of the book.
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Appendix 3: Glossary of terms and acronyms
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The list of definitions and acronyms of relevance to satellite-to-ground radiowave propagation has been collected over many conferences. It includes ITU-R standards applicable to VSAT systems and European technical standards (ETS) for VSAT systems.
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Appendix 4: ITU-R propagation series recommendations
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This appendix covers non-ionized media propagation, data acquisition, data analysis tropospheric propagation, radio links, ionospheric disturbance warnings, transmission loss, ground-wave propagation, microwave interference, ionospheric propagation, VHF propagation, UHF propagation, long-term ionospheric predictions, radio refractive index, and free-space attenuation.
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Back Matter
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