I. FUNDAMENTAL ANTENNA THEORY
Retarded Potentials
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Concept: Generalization of static potentials to time-varying sources, accounting for finite propagation speed \(c\).
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Derivation for sinusoidal sources: For current density \(\mathbf{J}(\mathbf{r}', t) = \mathbf{J}(\mathbf{r}') e^{j\omega t}\), the vector potential is
$$\mathbf{A}(\mathbf{r}, t) = \frac{\mu_0}{4\pi} \int \frac{\mathbf{J}(\mathbf{r}') e^{j\omega (t - |\mathbf{r}-\mathbf{r}'|/c)}}{|\mathbf{r}-\mathbf{r}'|} dV'$$
Similarly for scalar potential \(\phi\) with charge density.
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Significance: Enables calculation of radiated fields from arbitrary current distributions; essential for antenna analysis.
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Comparison with static potential: Static potentials assume instantaneous action at a distance (\(e^{j\omega t}\) factor only), while retarded potentials include delay \(|\mathbf{r}-\mathbf{r}'|/c\).
[!TIP] Retarded potentials are the foundation for deriving fields from any antenna; always use \(t_r = t - R/c\) with \(R = |\mathbf{r}-\mathbf{r}'|\).
Radiation from Elementary Sources
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Oscillating electric dipole (Hertzian dipole): Infinitesimal antenna of length \(dl \ll \lambda\) carrying current \(I_0\).
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Field components (far-field):
$$E_\theta = j \frac{\eta I_0 dl k}{4\pi r} \sin\theta \, e^{-jkr}$$
$$H_\phi = j \frac{I_0 dl k}{4\pi r} \sin\theta \, e^{-jkr}$$
where \(\eta = \sqrt{\mu_0/\varepsilon_0}\), \(k = 2\pi/\lambda\), \(r\) is distance.
- Power radiated:
$$P_{rad} = \frac{\pi \eta I_0^2 (dl)^2}{3 \lambda^2} = \frac{I_0^2 (dl)^2}{6\pi \eta} \left(\frac{2\pi}{\lambda}\right)^2$$
- Dependence: \(P_{rad} \propto (dl/\lambda)^2\); for fixed current, higher frequency (smaller \(\lambda\)) increases radiation.
[!TIP] Hertzian dipole fields are transverse in far-field; \(E_\theta\) and \(H_\phi\) are in phase and related by \(\eta\).
Antenna Parameters
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Radiation pattern: 3D plot of field/power vs direction. Cuts: E-plane (contains \(\mathbf{E}\) and \(\mathbf{r}\)), H-plane (contains \(\mathbf{H}\) and \(\mathbf{r}\)).
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Beamwidth: Half-power beamwidth (HPBW) or first-null beamwidth (FNBW).
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Directivity:
$$D = \frac{4\pi}{\Omega_A}$$
where \(\Omega_A\) = beam solid angle. For narrow beams, \(D \approx \frac{4\pi}{\theta_{BP} \phi_{BP}}\) (radians).
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Gain: \(G = \epsilon D\), where \(\epsilon\) = efficiency. In dB: \(G_{dBi} = 10 \log_{10} G\).
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Efficiency: \(\epsilon = \frac{R_{rad}}{R_{rad} + R_{loss}}\).
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Effective area: \(A_e = \frac{G \lambda^2}{4\pi}\).
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Effective length: \(h_e = \frac{V_{oc}}{E_{inc}}\) for open-circuit voltage.
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Relation: \(G = \frac{4\pi A_e}{\lambda^2}\).
[!TIP] Directivity is theoretical max; gain accounts for losses. Effective area relates receiving to transmitting gain.
Field Regions
| Region | Distance | Field Characteristics | Pattern Behavior |
|---|---|---|---|
| Reactive Near-field | \(r \ll \lambda\) | \(E\) and \(H\) out of phase, reactive dominance | Not established |
| Radiating Near-field (Fresnel) | \(0.62\sqrt{l^3/\lambda} < r < 2l^2/\lambda\) | Radiating, angular dependence varies with \(r\) | Varies with \(r\) |
| Far-field (Fraunhofer) | \(r > \frac{2l^2}{\lambda}\) | Plane waves, \(E \perp H \perp r\), in phase | Independent of \(r\) |
- Fraunhofer distance: \(\boxed{R = \frac{2l^2}{\lambda}}\) where \(l\) = largest antenna dimension.
[!TIP] For pattern measurements, ensure \(r > R\); near-field scanners require transformation to far-field.
Far-Field Approximation
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Conditions: \(r \gg \lambda\) and \(r \gg l^2/\lambda\); also angular extent small.
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Assumptions:
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\(1/r\) dependence,
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Transverse fields (\(E_r, H_r \approx 0\)),
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Wave impedance \(\eta\).
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Importance: Simplifies field expressions; pattern depends only on angle, not \(r\). Basis for array theory and gain measurements.
[!TIP] Far-field fields are spherical waves locally plane; used in Friis transmission equation.
Ground Effects on Antennas
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Impact of ground: Conductivity \(\sigma\) and permittivity \(\varepsilon_r\) determine reflection coefficient.
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Reflection coefficients (for plane wave at angle \(\theta\) from normal):
- Vertical polarization (E in plane of incidence):
$$\Gamma_v = \frac{\varepsilon_r \sin\theta - \sqrt{\varepsilon_r - \cos^2\theta}}{\varepsilon_r \sin\theta + \sqrt{\varepsilon_r - \cos^2\theta}}$$
- Horizontal polarization:
$$\Gamma_h = \frac{\sin\theta - \sqrt{\varepsilon_r - \cos^2\theta}}{\sin\theta + \sqrt{\varepsilon_r - \cos^2\theta}}$$
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Image theory: For perfect electric conductor (PEC), ground replaced by image antenna.
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Vertical antenna: image in-phase (current same direction).
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Horizontal antenna: image out-of-phase (current opposite).
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Effect on vertical patterns: For vertical antennas, ground reflection can enhance low-angle radiation (constructive interference) or cause nulls (destructive), depending on height and ground properties.
[!TIP] For AM broadcast (vertical monopoles), ground conductivity critical for low-angle radiation; poor ground increases losses.
II. WIRE ANTENNAS
Half-Wave Dipole
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Current distribution: \(I(z) = I_0 \cos(\beta z)\) for \(|z| \leq \lambda/4\), where \(\beta = 2\pi/\lambda\).
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Radiation pattern:
$$E_\theta \propto \frac{\cos\left(\frac{\pi}{2} \cos\theta\right)}{\sin\theta}$$
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E-plane: figure-8 (doughnut), H-plane: circle.
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Input impedance: \(Z_{in} \approx 73 + j42.5\ \Omega\) at resonance.
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Radiation resistance: \(R_{rad} \approx 73\ \Omega\).
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Influence of length:
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Slightly longer: higher resistance, capacitive reactance.
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Slightly shorter: lower resistance, inductive reactance.
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Directional properties: as length increases, pattern splits into multiple lobes (e.g., 1.5λ dipole has 4 lobes).
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[!TIP] Half-wave dipole is reference for gain (2.15 dBi); length tolerance ±5% acceptable.
Quarter-Wave Monopole
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Operation over ground plane: Uses image theory; equivalent to half-wave dipole in upper hemisphere.
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Radiation pattern: Same as half-wave dipole but only above ground; power radiated half of dipole.
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Fields: For perfect ground, \(E_\theta\) same as dipole for \(\theta \leq 90^\circ\), zero below.
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Input impedance: \(Z_{in} \approx 36.5 + j21.25\ \Omega\) (half of dipole).
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Applications: Mobile phones, FM broadcast (with ground plane).
[!TIP] Monopole gain is 2.15 dBi relative to isotropic; relative to dipole, gain is 0 dBD.
Long Wire Antennas (Traveling Wave)
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Construction: Wire length \(l \gg \lambda\), terminated with resistance \(R_T \approx 300-800\ \Omega\).
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Current distribution: Traveling wave, \(I(z) = I_0 e^{-j\beta z}\) (decaying if matched).
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Radiation pattern: End-fire along wire direction; maximum at angle \(\theta \approx \arccos(\lambda/l)\) for \(l \gg \lambda\).
- Beverage antenna: long wire above ground, unidirectional, low angle radiation.
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Influence of length: Longer wire → narrower beam, higher gain (up to ~10 dBi for \(l \approx 10\lambda\)).
[!TIP] Long wire antennas are unidirectional due to termination; avoid reflections for pure traveling wave.
Folded Dipole
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Structure: Two parallel dipoles connected at ends; fed at center of one.
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Feed impedance transformation: Input impedance ≈ \(4 \times\) single dipole impedance (for equal diameters). So ~300 Ω for half-wave.
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Current distribution: Equal currents in both arms; voltage across feed point doubled.
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Applications: Broadband feed for Yagi-Uda, FM reception (300 Ω balanced line).
[!TIP] Folded dipole bandwidth ~15% wider than simple dipole due to increased impedance.
Other Wire Antennas
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Turnstile antenna: Two crossed dipoles, 90° phase shift → circular polarization.
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Rhombic antenna: Four-wire diamond, traveling wave with termination; broadside pattern, gain ~15 dBi.
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V-antenna: V-shaped wire, angle ~90°; broadside pattern, moderate gain.
III. ANTENNA ARRAYS
Array Fundamentals
- Array factor (AF): For \(N\) elements with currents \(I_n\), positions \(\mathbf{d}_n\), phases \(\beta_n\):
$$AF(\theta,\phi) = \sum_{n=1}^N I_n e^{j(k \mathbf{\hat{r}} \cdot \mathbf{d}_n + \beta_n)}$$
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Pattern multiplication theorem: Total pattern = element pattern × array factor (if elements identical and similarly oriented).
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Element patterns vs. array factor: Element pattern accounts for single antenna radiation; array factor accounts for spatial arrangement.
Linear Arrays
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Broadside: Maximum radiation perpendicular to array axis; phase progression \(\alpha = 0\).
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End-fire: Maximum radiation along array axis; phase progression \(\alpha = \mp k d\) (for forward/backward).
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Phased arrays: Steer beam by progressive phase \(\alpha = -k d \cos\theta_0\) (for array along \(z\), broadside at \(\theta_0=90^\circ\)).
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Element spacing \(d\):
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\(d \leq \lambda\) avoids grating lobes (multiple maxima).
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Grating lobes appear if \(d > \lambda\) and \(|\alpha| < k d\).
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[!TIP] For scanning, maximum scan angle \(\theta_{max}\) without grating lobes: \(d \leq \frac{\lambda}{1 + |\sin\theta_0|}\).
Array Synthesis Methods
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Binomial array: Amplitude coefficients from binomial expansion \((1+x)^{N-1}\); no side lobes but wide main beam.
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Taylor distribution: Continuous approximation to reduce side lobes; parameter \(\bar{n}\) controls lobe level.
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Schelkunoff unit circle method: Place zeros of AF on unit circle in complex plane; nulls at \(\Phi = kd\cos\theta + \alpha\). Example: zeros at \(\Phi = 90^\circ,180^\circ,270^\circ\) → array coefficients from polynomial.
Yagi-Uda Antenna
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Construction: Driven element (half-wave dipole), reflector (longer, ~5% longer), directors (shorter, ~5% shorter).
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Pattern formation: Reflector induces reverse current, reinforcing forward wave; directors phase-advance waves, enhancing forward gain.
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Design parameters:
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Reflector length: \(0.5\lambda\) to \(0.52\lambda\)
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Director lengths: decreasing from driven element.
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Spacing: reflector ~0.15–0.2λ, directors ~0.3–0.4λ.
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Gain: 7–15 dBi depending on number of directors.
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Applications: TV reception, point-to-point links.
[!TIP] Yagi gain increases with directors but with diminishing returns; typically 10–12 directors for ~15 dBi.
Log-Periodic Antenna
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Structure: Toothed elements of varying lengths, fed transverely along boom. Scale factor \(\tau = \frac{L_{n+1}}{L_n} < 1\), angle \(\alpha\).
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Frequency-independent principle: Geometry self-similar; input impedance and pattern repeat every decade.
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Wideband characteristics: Operates over 2:1 or more bandwidth; gain ~7–10 dBi.
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Applications: Wideband TV reception, EMC measurements.
[!TIP] LPDA feed at apex; active region where element length ≈ λ/2 shifts with frequency.
IV. APERTURE ANTENNAS
Horn Antennas
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Types: Pyramidal (rectangular), conical, sectoral (E-plane or H-plane).
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Gain calculation:
$$G = \frac{4\pi A_e}{\lambda^2} = \eta \left(\frac{\pi D}{\lambda}\right)^2$$
for circular aperture; for rectangular, \(A_e = a b\). Efficiency \(\eta \approx 0.5–0.6\).
- Feeding: Waveguide, coax-to-waveguide transition.
[!TIP] Horn gain measured by comparison method; directivity from aperture field distribution.
Slot Antennas
- Babinet’s principle: Complementary antennas (slot in infinite ground vs. dipole) have identical \(E\) and \(H\) fields interchanged, with
$$\mathbf{E}_{slot} = \frac{\lambda^2}{4\pi} \mathbf{H}_{dipole}, \quad \mathbf{H}_{slot} = -\frac{\lambda^2}{4\pi} \mathbf{E}_{dipole}$$
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Rectangular slot in infinite ground: Slot dimensions \(a \times b\); fed by probe or waveguide.
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Radiation pattern: Similar to dipole but with H- and E-planes swapped.
$$E_\phi \propto \frac{\sin\left(\frac{\pi a}{\lambda} \sin\theta \cos\phi\right)}{\frac{\pi a}{\lambda} \sin\theta \cos\phi} \cdot \frac{\sin\left(\frac{\pi b}{\lambda} \sin\theta \sin\phi\right)}{\frac{\pi b}{\lambda} \sin\theta \sin\phi}$$
[!TIP] Slot antennas are used in arrays and aircraft (flush-mounted).
Parabolic Reflector Antennas
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Geometry: Paraboloid of revolution; focal point \(f = D^2/(16C)\) where \(C\) = depth.
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Focusing principle: Parallel rays reflect to feed (prime focus) or to secondary (Cassegrain).
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Feed mechanisms:
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Prime focus: feed at focal point.
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Cassegrain: subreflector (hyperbolic) reflects to feed behind vertex.
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Aperture efficiency: \(\eta = \eta_{spillover} \times \eta_{taper} \times \eta_{blockage}\).
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Tapered apertures: Aperture illumination tapered (e.g., cosine) reduces side lobes at cost of gain.
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Aperture blockage: Feed and subreflector block part of aperture, reducing gain and increasing side lobes.
[!TIP] Typical efficiency 50–70%; Cassegrain reduces spillover but adds blockage.
Lens Antennas
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Types: Dielectric lens (Luneburg, hemispherical), zoned lens (reduces thickness).
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Operation: Refracts plane wave to feed or vice versa; focal length \(f = \frac{R}{2(\sqrt{\varepsilon_r}-1)}\) for hemispherical.
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Applications: Microwave systems, radar, where reflectors impractical.
Flat Sheet and Corner Reflectors
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Flat sheet: Flat conducting plate; acts as aperture when fed by dipole; pattern bidirectional.
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Corner reflector: Two flat plates at 90°; unidirectional pattern, gain ~10–12 dBi.
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Directivity: Increases with size; edge effects cause diffraction.
V. PRINTED AND PLANAR ANTENNAS
Microstrip (Patch) Antennas
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Rectangular patch design:
- Width \(W\):
$$W = \frac{c}{2f_r} \sqrt{\frac{2}{\varepsilon_r + 1}}$$
- Effective dielectric constant:
$$\varepsilon_{eff} = \frac{\varepsilon_r + 1}{2} + \frac{\varepsilon_r - 1}{2} \left(1 + 12\frac{h}{W}\right)^{-1/2}$$
- Length \(L\) (for resonance):
$$L = \frac{c}{2f_r \sqrt{\varepsilon_{eff}}} - 2\Delta L$$
where \(\Delta L \approx 0.412h \frac{(\varepsilon_{eff}+0.3)(W/h+0.264)}{(\varepsilon_{eff}-0.258)(W/h+0.8)}\).
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Substrate parameters: \(\varepsilon_r\) and height \(h\) affect bandwidth (\(BW \propto h/\varepsilon_r\)) and efficiency.
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Feeding techniques:
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Microstrip line (impedance matching via inset).
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Coaxial probe (vertical feed).
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Aperture coupling (slot between ground and patch).
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Advantages: Low profile, conformal, inexpensive, easy to integrate.
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Limitations: Narrowband (typically 1–5%), low efficiency (due to surface waves, dielectric loss), spurious feed radiation.
[!TIP] Patch length ≈ \(\lambda_0/(2\sqrt{\varepsilon_{eff}})\); increase \(h\) for wider bandwidth but higher surface waves.
Planar Arrays
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Configuration: 2D grid of elements (rectangular, circular).
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Pattern synthesis: Separable into two linear arrays; control both azimuth and elevation patterns.
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Applications: Phased array radars, satellite communications, beam steering.
VI. WAVE PROPAGATION MECHANISMS
Ground Wave Propagation
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Components:
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Surface wave: Bound to ground, follows Earth’s curvature; dominant at low frequencies (MF, HF).
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Space wave: Direct + ground-reflected; dominant at VHF/UHF.
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Transition: At higher frequencies, space wave dominates; surface wave attenuates rapidly.
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Influence of terrain:
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Conductivity: higher \(\sigma\) → lower attenuation (sea water best).
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Curvature: limits range; horizon distance \(d \approx \sqrt{2h_t} + \sqrt{2h_r}\) (km) with heights in meters.
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Attenuation:
$$A \approx 8.7 \alpha \ d$$
(dB) where \(\alpha\) = attenuation constant (dB/km), depends on frequency and ground.
[!TIP] Ground wave used for AM broadcast; over seawater, range > 1000 km at 1 MHz.
Sky Wave Propagation (Ionospheric)
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Ionospheric layers: D (60–90 km), E (90–150 km), F (150–500 km, splits into F1/F2 daytime).
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Critical frequency:
$$f_c = 9\sqrt{N_{max}}\ \text{MHz}$$
where \(N_{max}\) = maximum electron density (electrons/m³).
- Maximum Usable Frequency (MUF):
$$\text{MUF} = \frac{f_c}{\cos\theta}$$
where \(\theta\) = angle of incidence at ionosphere.
- Skip distance: Minimum ground distance with no signal;
$$d_{skip} = 2(R + h) \sin\theta \approx 2\sqrt{2Rh}$$
for small \(\theta\), \(h\) = virtual height.
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Lowest Usable Frequency (LUF): Determined by D-layer absorption; increases with solar activity.
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Virtual height: Apparent reflection height from ionogram: \(h' = \frac{c \Delta t}{2}\).
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Derivation of MUF-skip relation:
From geometry: \(\sin\theta = \frac{d}{2(R+h)}\), and \(\cos\theta = \sqrt{1 - \sin^2\theta}\). MUF = \(f_c / \cos\theta\).
[!TIP] Optimum working frequency (OWF) ≈ 0.85 MUF to avoid fading.
Tropospheric Propagation
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Refraction: Standard atmosphere: refractive index \(n = 1 + 40.3 \times 10^{-6} N / f^2\)? Actually, for radio, \(n \approx 1 + \frac{79.5 P}{T} \times 10^{-6}\) (P in hPa, T in K). Gradient \(dn/dh \approx -4 \times 10^{-7}\)/m → Earth curvature equivalent radius \(R_e/(1+R_e dn/dh) \approx 4/3 R_e\).
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Super refraction: \(dn/dh\) more negative → ray curvature > Earth curvature; extends radio horizon.
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Subrefraction: \(dn/dh\) less negative or positive → ray curvature < Earth curvature; reduces horizon.
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Tropospheric scattering: Turbulence causes scattering; enables beyond-horizon reception (VHF/UHF).
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Duct propagation:
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Surface-based duct: \(dn/dh < -157 \times 10^{-6}\)/m (evaporation duct).
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Elevated duct: temperature inversion.
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Traps waves, low loss over hundreds of km (microwave).
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[!TIP] Ducting common over oceans; causes anomalous propagation for radar.
Environmental Effects
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Atmospheric conditions: Humidity, precipitation cause absorption (especially >10 GHz).
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Terrain and obstacles: Diffraction over hills, reflection from buildings → multipath fading.
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Fading:
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Fast fading (multipath, wavelength scale).
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Slow fading (shadowing, terrain scale).
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Impact: Signal strength fluctuations, delay spread, polarization changes.
VII. SPECIAL TOPICS & DESIGN TOOLS
Helical Antenna
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Normal mode: Circumference \(C \approx \lambda\), pitch \(S \ll \lambda\); broadside radiation, circular polarization.
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Axial mode: \(C \approx \lambda\), \(S \approx \lambda/4\); end-fire, high gain (10–15 dBi), circular polarization.
- Axial ratio: \(AR \approx \sqrt{1 + \left(\frac{2S}{\lambda}\right)^2}\) for \(C=\lambda\).
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Applications: Satellite communications (axial mode), VHF/UHF (normal mode).
Numerical Tools for Antenna Analysis
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HFSS: Finite element method (FEM); high-frequency structures.
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CST: Time domain solver; transient analysis.
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NEC: Method of Moments (MoM); wire antennas, ground planes.
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Applications: Design, optimization, near-to-far field transformation, impedance matching.
Reciprocity Theorem
- Statement: For two antennas A and B,
$$Z_{AB} = Z_{BA}$$
where \(Z_{AB}\) = open-circuit voltage at A due to current in B.
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Proof: From Lorentz reciprocity: \(\int_V (\mathbf{J}_1 \cdot \mathbf{E}_2 - \mathbf{J}_2 \cdot \mathbf{E}_1) dV = 0\).
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Implication: Transmitting pattern of antenna A equals receiving pattern of antenna A.
Antenna Gain and Effective Area
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Detailed derivation:
From Friis: \(P_r = P_t G_t G_r \left(\frac{\lambda}{4\pi R}\right)^2\).
For receiving, \(P_r = \frac{|V_{oc}|^2}{2R_{rad}}\) and \(V_{oc} = E_{inc} h_e\).
Also, \(G = \frac{4\pi A_e}{\lambda^2}\) from power conservation.
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Measurement techniques:
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Gain: comparison with standard horn, or using Friis with known distance.
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Effective area: measure gain, then compute.
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VIII. FREQUENTLY ASKED DERIVATIONS & SHORT NOTES
(Integrated in relevant sections above)
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Derivation of radiated fields from Hertzian dipole: In Radiation from Elementary Sources.
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Power radiated by quarter-wave monopole: In Quarter-Wave Monopole (half of half-wave dipole).
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Radiation pattern of rectangular slot: In Slot Antennas (Babinet’s principle).
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Relation between MUF and skip distance: In Sky Wave Propagation (geometry derivation).
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Pattern multiplication and earth’s effect on vertical patterns: In Array Fundamentals and Ground Effects.
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Taylor synthesis: In Array Synthesis Methods.
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Schelkunoff unit circle: In Array Synthesis Methods (null placement).
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Microstrip patch dimensions: In Microstrip Antennas (formulas).
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Horn antenna gain calculation: In Horn Antennas (aperture efficiency).
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Critical frequency, virtual height, maximum coverage: In Sky Wave Propagation (\(f_c = 9\sqrt{N_{max}}\), \(h' = c\Delta t/2\), \(d_{max} \approx 2\sqrt{2Rh}\)).
[!EXAM TIP] Past papers emphasize derivations: retarded potential, Hertzian dipole fields, monopole power, MUF-skip, slot pattern, array synthesis. Practice these step-by-step with clear assumptions (far-field, sinusoidal sources). For numerical problems, always state formulas first (e.g., \(G = 4\pi A_e/\lambda^2\), MUF = \(f_c/\cos\theta\)).