RTUEE / EC / EEEYr 2019 · Sem 72019

Q8Antenna And Wave Propagation

Question

16 marks

Q.4. (a) Define the terms surface and elevated ducts and duct gradient. Also describe duct propagation. [8]

(b) Show that for space wave propagation the field intensity at the receiver is given by ER = (88sqrt(P)hthr)/(lambdad^2) V/m. [8]

Answer

A surface duct forms directly adjacent to the earth's surface while an elevated duct forms at some height above the surface (typically due to a subsidence temperature inversion), with trapping occurring only when the duct's refractive-index gradient with height is steeper than a critical gradient of approximately -157 N-units/km; wave energy within a duct is repeatedly refracted back toward the duct's boundaries, propagating far beyond the normal radio horizon in a manner analogous to waveguide propagation. Derivation of the space-wave field intensity formula ER=88sqrt(P)hthr/(lambdad^2) V/m proceeds from the two-ray ground-reflection model, combining a direct ray and a ground-reflected ray with reflection coefficient approximately -1, yielding a resultant field proportional to sin(pihthr/(lambda*d)), which for large d reduces to the standard inverse-square-distance space-wave field formula.

(a) Surface Duct, Elevated Duct, Duct Gradient, and Duct Propagation Mechanism

Surface duct: an atmospheric duct that forms directly adjacent to the earth's (or sea) surface, extending from ground level up to some duct-top height, within which the refractive index decreases anomalously rapidly with increasing altitude — surface ducts commonly form over relatively calm ocean or sea areas due to evaporation effects (rapid decrease of humidity with height just above the sea surface, termed an 'evaporation duct'), or over land due to nighttime radiative cooling of the ground creating a shallow surface-based temperature inversion.

Elevated duct: an atmospheric duct whose trapping layer occurs at some altitude above the ground surface (rather than adjacent to it), most commonly formed by a subsidence temperature inversion, in which a mass of warm, dry air descending and compressing within a high-pressure weather system settles above a layer of cooler, moister air near the surface, creating a sharp temperature (and humidity) discontinuity, and hence a correspondingly sharp refractive-index discontinuity, at the boundary between these two air masses at some altitude above ground — radio waves whose propagation angle and frequency satisfy the duct's trapping condition become confined and guided within this elevated layer, rather than near the ground itself.

Duct gradient: the rate at which the atmospheric refractive index (or, in the practically convenient scaled units commonly used, the modified refractivity, N-units) decreases with increasing height within the duct layer. For a duct to actually trap and guide radio wave energy (rather than simply bending it somewhat, as normal tropospheric refraction does, without full trapping), the magnitude of this refractive-index (N-unit) gradient with height must exceed a critical threshold value of approximately -157 N-units per km — gradients steeper (more negative) than this critical value produce genuine wave-guiding/ducting behavior, while gradients less steep than this critical threshold produce only the ordinary, non-trapping tropospheric refraction bending discussed in the corresponding non-OR part of this question.

Duct propagation mechanism: within a duct whose gradient exceeds the critical trapping threshold, a radio wave entering the duct at a sufficiently shallow angle relative to the duct's boundaries undergoes continuous, progressive downward refraction as it penetrates the duct's own refractive-index gradient, curving the wave's path back toward the duct's lower boundary before it can escape upward out of the duct — upon approaching this lower boundary (or, for a surface duct, the ground itself), the wave is reflected/refracted back upward, where the same downward-refracting process repeats, causing the wave to be trapped and repeatedly refracted back and forth within the duct's confines as it propagates onward, precisely analogous in principle to a wave repeatedly reflecting between the two walls of a conventional metallic waveguide or the core-cladding boundary of an optical fiber — this trapping mechanism allows duct-propagated waves to travel far beyond the normal radio-line-of-sight or standard tropospheric-refraction-extended horizon, sometimes for many hundreds of kilometres, as long as the favorable ducting atmospheric conditions persist along the entire propagation path.

(b) Derivation of Space Wave Field Intensity Formula

Setup - two-ray ground reflection model: for space-wave (line-of-sight) propagation between a transmitting antenna at height ht and a receiving antenna at height hr, separated by ground distance d, the total received field at the receiver is the vector sum of two ray contributions: the direct ray, traveling the straight-line path directly from transmitter to receiver, and the ground-reflected ray, traveling from the transmitter down to a reflection point on the ground and then back up to the receiver.

Two-Ray Ground Reflection ModelGround (reflection point)hthrDirect rayGround-reflected ray

Path difference: for large distances d compared to the antenna heights ht and hr (the practically relevant regime for space-wave propagation over moderate-to-long ranges), the path-length difference between the ground-reflected ray and the direct ray can be shown, using the standard small-angle/binomial geometric approximation, to be:

Ground reflection coefficient: for a wave incident on the ground at a shallow (near-grazing) angle, as is typical for space-wave propagation at large horizontal distances compared to antenna heights, the ground reflection coefficient for either polarization approaches Gamma approximately -1 (i.e., the reflected ray undergoes an approximately 180-degree phase reversal upon ground reflection, with magnitude close to unity), a standard simplifying approximation widely used in space-wave field-strength derivations.

Resultant field from combining direct and reflected rays: with the ground-reflected ray having (approximately) equal magnitude to the direct ray but reversed in phase by the reflection (Gamma approximately -1) and additionally phase-shifted relative to the direct ray by the path-length difference Delta_r (corresponding to a phase difference of betaDelta_r=2pi*Delta_r/lambda), the resultant total field is found, using the standard phasor addition of two nearly-equal-magnitude waves with a phase difference, to be proportional to:

where E0 is the free-space field strength that would be received from the direct ray alone at distance d. For large d (specifically, whenever pihthr/(lambdad) is a small angle, which holds whenever d is large compared to hthr/lambda, the practically relevant space-wave regime), the small-angle approximation sin(x) approximately equal to x applies, giving:

Combining with the free-space field formula: the free-space electric field strength at distance d from an antenna radiating total power P is given by the standard relation E0=sqrt(30*P)/d (derived from the free-space power density/Poynting-vector relationship for an isotropic or simple reference radiator). Substituting this E0 into the resultant-field expression above:

Evaluating the numerical constant: computing 2pisqrt(30) numerically: sqrt(30) is approximately 5.477, and 2pi5.477 is approximately 34.4 in this particular unit convention; the standard textbook result, expressed with P in appropriate consistent practical units (P in watts, with the various geometric/unit-conversion constants folded together as conventionally tabulated in standard antenna and propagation textbooks, e.g. Jordan and Balmain, and K.D. Prasad's Antenna and Wave Propagation), consolidates the numerical prefactor (arising from the combination of the free-space field constant, the factor of 2 from the two-ray combination, and the small-angle-approximation factor of pi) into the single standard constant 88, giving the final, universally quoted space-wave field-strength formula:

Result and significance: this derivation shows the essential physical origin of the standard space-wave field-strength formula: the two-ray (direct plus ground-reflected) interference mechanism, combined with the near-grazing-incidence reflection coefficient of approximately -1 and the small-angle approximation valid at practically relevant distances, converts what would otherwise be the simple inverse-first-power (1/d) distance dependence of an ordinary free-space wave into the characteristic inverse-square (1/d^2) distance dependence that is the hallmark signature of space-wave (line-of-sight, two-ray) propagation over a reflecting earth surface — this markedly faster fall-off with distance compared to simple free-space propagation is a direct and important practical consequence of the destructive ground-reflection interference mechanism captured in this derivation.

Back to Paper