UNIT 4: ANTENNAS AND WAVE PROPAGATION - SHORT NOTES
1. FOUNDATIONAL ANTENNA THEORY & RADIATION MECHANISMS
Retarded Potential
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Concept: Accounts for finite propagation speed ($c$) of EM waves. The potential at point $P$ at time $t$ depends on source values at an earlier retarded time $$\displaystyle t_r = t - R/c $$, where $R$ is distance from source to $P$.
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Derivation for Sinusoidal Sources: For a current element $$\displaystyle I(z')e^{j\omega t} $$ along $z'$, vector potential $\mathbf{A}$ is:
$$\mathbf{A}(z,t) = \frac{\mu}{4\pi} \int \frac{I(z') e^{j\omega (t - R/c)}}{R} \,dz' \, \mathbf{\hat{z}}$$
where $R \approx r - z'\cos\theta$ for $r \gg$ element length. This leads to radiation fields.
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Significance: Fundamental to solving radiation problems; separates near-field (quasi-static) and radiation-field terms.
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Approaches to Solve Radiation Problems:
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Retarded Potential Method: Direct integration.
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Vector Potential + Wave Equation: Solve Helmholtz equation.
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Huygens' Principle: Aperture integration.
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[!TIP] Exam Focus: Retarded potential is the bridge between static fields and radiation. Be ready to derive $\mathbf{A}$ for a short dipole and identify the $1/r$ term as the radiation term.
Oscillating Electric Dipole / Current Element
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Model: Infinitesimal dipole (Hertzian dipole): length $dl \ll \lambda$, carrying uniform current $$\displaystyle I_0 $$.
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Radiated Fields (in spherical coordinates, $\theta$-polarized):
$$E_\theta = j\frac{\eta I_0 (\beta l)}{4\pi r} \sin\theta \, e^{-j\beta r} \left[1 + \frac{j}{\beta r}\right]$$
$$H_\phi = j\frac{I_0 (\beta l)}{4\pi r} \sin\theta \, e^{-j\beta r} \left[1 + \frac{j}{\beta r}\right]$$
where $$\displaystyle \beta = 2\pi/\lambda $$, $$\displaystyle \eta = \sqrt{\mu/\varepsilon} $$.
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Far-field ($r \gg \lambda$): Terms in $1/(\beta r)$ vanish → $$\displaystyle E_\theta \propto 1/r $$, $$\displaystyle H_\phi \propto 1/r $$.
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Power Radiation:
$$P_{rad} = \frac{I_0^2 (\beta l)^2}{12\pi\eta} \quad \text{(for } \beta l \ll 1\text{)}$$
Power $$\displaystyle \propto (I_0 f)^2 $$ (since $$\displaystyle \beta = 2\pi f/c $$).
- Radiation Resistance:
$$R_r = \frac{2P_{rad}}{I_0^2} = \frac{80\pi^2 (dl/\lambda)^2}{}$$
\boxed{R_r \approx 80\pi^2 (dl/\lambda)^2 , \Omega}
[!TIP] Common Pitfall: The $$\displaystyle 1/r^2 $$ and $$\displaystyle 1/r^3 $$ terms are reactive (store energy), not radiative. Only the $1/r$ terms carry time-average power to infinity.
Near-field and Far-field Regions
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Definitions (for antenna of max dimension $D$):
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Reactive Near-field ($$\displaystyle r < 0.62\sqrt{D^3/\lambda} $$): Reactive fields dominate ($$\displaystyle E \propto 1/r^3 $$, $$\displaystyle 1/r^2 $$). Field pattern not well-defined.
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Fresnel (Radiation) Near-field ($$\displaystyle 0.62\sqrt{D^3/\lambda} < r < 2D^2/\lambda $$): Both reactive and radiative fields present. Field structure complex, varies with $r$.
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Fraunhofer (Far-field) ($$\displaystyle r > 2D^2/\lambda $$): Pure radiative field ($E,H \propto 1/r$). Angular field distribution independent of $r$. Pattern measurement region.
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Key Difference: Near-field has significant $E$- and $H$-phase difference and $E/H$ ratio ≠ $\eta$; Far-field has $E \perp H$, $$\displaystyle |E|/|H| = \eta $$, in-phase.
[!TIP] Rule of Thumb: Far-field starts at $$\displaystyle r_{ff} = \frac{2D^2}{\lambda} $$. For $$\displaystyle D = 1\,m $$, $$\displaystyle \lambda=0.1\,m $$, $$\displaystyle r_{ff} = 20\,m $$.
Far-field Approximation
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Significance: Simplifies antenna analysis. In far-field:
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$R \approx r$ in denominator.
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$$\displaystyle e^{-j\beta R} \approx e^{-j\beta r} e^{j\beta \hat{\mathbf{r}}\cdot\mathbf{r}'} $$ (phase approximation).
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$\mathbf{\hat{R}} \approx \mathbf{\hat{r}}$ (direction approximation).
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Conditions: $r \gg \lambda$ and $$\displaystyle r \gg D^2/\lambda $$. Enables pattern multiplication and array factor concepts.
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Simplifications: Radiated fields transverse ($$\displaystyle E_\theta, H_\phi $$ only for z-axis dipole). Power flow radial ($\mathbf{S} \propto \mathbf{\hat{r}}$).
Reciprocity Theorem
- Statement: If a current $$\displaystyle I_1 $$ at antenna 1 produces field $$\displaystyle E_2 $$ at antenna 2, then same current $$\displaystyle I_1 $$ at antenna 2 produces same field $$\displaystyle E_1 $$ at antenna 1. Mathematically:
$$\oint_S (\mathbf{E}_1 \times \mathbf{H}_2 - \mathbf{E}_2 \times \mathbf{H}_1) \cdot d\mathbf{S} = 0$$
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Implication for Antennas: Transmitting and receiving patterns are identical for same antenna. Also, mutual impedance $$\displaystyle Z_{12} = Z_{21} $$.
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Proof Sketch: Apply vector identity $$\displaystyle \nabla \cdot (\mathbf{E}_1 \times \mathbf{H}_2 - \mathbf{E}_2 \times \mathbf{H}_1) = \mathbf{H}_2 \cdot (\nabla \times \mathbf{E}_1) - \mathbf{E}_1 \cdot (\nabla \times \mathbf{H}_2) - (\mathbf{E}_1 \leftrightarrow \mathbf{E}_2) $$. Use Maxwell's equations and integrate over closed surface; surface integral → 0 if sources enclosed or fields vanish at infinity.
Antenna Parameters & Definitions
| Parameter | Definition | Key Formula/Note |
|---|---|---|
| Radiation Pattern | 3D/2D plot of radiated power/field vs direction. | E-plane (cut with $E$-field), H-plane (cut with $H$-field). |
| Directivity $D$ | Ratio of radiation intensity in direction $(\theta,\phi)$ to average intensity. | $$\displaystyle D = \frac{4\pi U(\theta,\phi)}{P_{rad}} $$; $$\displaystyle D_{max} = \frac{4\pi}{P_{rad}} \int_0^{2\pi}\int_0^\pi U(\theta,\phi) \sin\theta d\theta d\phi $$ |
| Beamwidth | Angular width between half-power points (HPBW). | $$\displaystyle \text{HPBW} \approx \frac{58^\circ \lambda}{D} $$ (for broadside aperture). |
| Gain $G$ | Directivity × efficiency. Absolute or dB ($$\displaystyle G_{dBi} = 10\log_{10}G $$). | $$\displaystyle G = \eta_e D $$, $$\displaystyle \eta_e = \frac{R_r}{R_r + R_{loss}} $$ |
| Radiation Resistance $$\displaystyle R_r $$ | Equivalent resistance dissipating $$\displaystyle P_{rad} $$ for given $$\displaystyle I_0 $$. | $$\displaystyle P_{rad} = \frac{1}{2} I_0^2 R_r $$ |
| Effective Length $$\displaystyle h_e $$ | Ratio of open-circuit voltage to incident $E$-field. | $$\displaystyle V_{oc} = h_e E^{inc} $$; for short dipole, $$\displaystyle h_e \approx \frac{\eta l}{2\pi} $$ |
| Effective Aperture $$\displaystyle A_e $$ | Area capturing power from incident wave. | $$\displaystyle A_e = \frac{G \lambda^2}{4\pi} $$ \boxed{A_e = \frac{G \lambda^2}{4\pi}} |
| Gain–Aperture Relation | Links gain to physical size. | $$\displaystyle G = \eta_a \frac{4\pi A_{phys}}{\lambda^2} $$, $$\displaystyle \eta_a $$ = aperture efficiency. |
[!TIP] Directivity vs Gain: Directivity is theoretical max; Gain is real (includes losses). For lossless antenna, $$\displaystyle G = D $$.
2. WIRE ANTENNAS
Dipole Antennas
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Half-wave Dipole ($$\displaystyle l = \lambda/2 $$):
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Current Distribution: $$\displaystyle I(z) = I_0 \cos(\beta z) $$ (sinusoidal, zero at ends).
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Radiation Pattern: Figure-8 in E-plane ($$\displaystyle \phi=0 $$ cut), omnidirectional in H-plane. Max at $$\displaystyle \theta=90^\circ $$.
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Directivity: $D \approx 1.64$ (2.15 dBi). $$\displaystyle R_r \approx 73\,\Omega $$.
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Length Influence: As $l$ increases beyond $\lambda/2$, main beam splits, grating lobes appear. For $l \approx 1.2\lambda$, back lobe develops.
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Short Dipole ($l \ll \lambda$): Same pattern as infinitesimal dipole (sin²θ). $$\displaystyle R_r \propto (l/\lambda)^2 $$.
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Infinitesimal Dipole: Theoretical limit; $$\displaystyle R_r \approx 80\pi^2 (dl/\lambda)^2\,\Omega $$.
[!TIP] Pattern Shape: Dipole E-plane pattern $\propto \sin\theta$. Half-wave is standard reference.
Quarter-wave Monopole
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Working Principle: Half dipole over perfect ground plane. Uses image theory: ground plane replaced by image monopole (current opposite phase) → full $\lambda/2$ dipole in free space.
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Radiation Pattern: Same as half-wave dipole but only above ground plane (hemispherical). Ground plane must be large ($$\displaystyle > \lambda $$).
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Power Radiated: Half of $\lambda/2$ dipole → $$\displaystyle P_{rad} = \frac{I_0^2 \cdot 73}{2} \Omega $$ (if $$\displaystyle R_r $$ same).
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Applications: Vehicle antennas, mast radiators for AM broadcast.
[!TIP] Impedance: Monopole over perfect ground: $$\displaystyle R_r \approx 36.5\,\Omega $$ (half of dipole). Over real ground, $$\displaystyle R_r $$ decreases due to losses.
Folded Dipole
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Construction: Two parallel $\lambda/2$ dipoles connected at ends; fed at center of one.
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Current Distribution: $$\displaystyle I_1 $$ (feed arm), $$\displaystyle I_2 $$ (other arm). For symmetric case, $$\displaystyle I_1 = I_0 $$, $$\displaystyle I_2 = -I_0 $$ → balanced.
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Impedance: $$\displaystyle R_{in} \approx 4 \times R_{r,dipole} \approx 292\,\Omega $$ (for lossless, equal arms). High impedance useful for matching to twin-lead (300 $\Omega$).
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Bandwidth: Slightly wider than simple dipole due to increased thickness effect.
Long Wire Antenna / Traveling Wave Antennas
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Radiation from Wire of Length $l$: Current is traveling wave (not standing wave). $$\displaystyle I(z) = I_0 e^{-j\beta z} $$ (for $$\displaystyle z>0 $$).
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Pattern Characteristics:
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Pattern Function: $$\displaystyle F(\theta) \propto \frac{\cos(\frac{\beta l}{2} \cos\theta) - \cos(\frac{\beta l}{2})}{\sin\theta} $$
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For $l \gg \lambda$, main lobe at $$\displaystyle \theta \approx 90^\circ $$ (broadside) with cardioid shape if terminated in matched load.
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End-fire if open-circuited (standing wave component).
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Length Influence:
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$$\displaystyle l = n\lambda/2 $$: Resonant, high $$\displaystyle R_r $$, but pattern multi-lobed.
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$l \approx \lambda$ to $2\lambda$: Good end-fire gain (5–8 dBi).
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$l \gg \lambda$: Narrow beam, high directivity, but inefficient feed.
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V-Antenna: Two long wires at angle $\alpha$; pattern tilted by $\alpha/2$.
[!TIP] Long Wire vs Dipole: Long wire has traveling wave → unidirectional pattern; dipole has standing wave → bidirectional.
Rhombic Antenna (Short Notes)
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Structure: Four long wires in diamond shape, terminated with resistors.
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Operation: Traveling wave along each leg; main lobe along rhombus axis.
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Advantages: High gain (15–20 dBi), wide bandwidth, unidirectional.
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Disadvantages: Low efficiency (termination loss), large size.
Turnstile Antenna
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Construction: Two orthogonal half-wave dipoles fed $$\displaystyle 90^\circ $$ out-of-phase.
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Radiation: Circularly polarized (CP) when axes crossed at $$\displaystyle 90^\circ $$ and fed in quadrature. Omnidirectional in horizontal plane for CP.
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Applications: FM broadcasting, satellite communication (CP reception).
3. APERTURE & REFLECTOR ANTENAS
Horn Antennas
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Types:
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E-plane horn: Flared in E-plane.
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H-plane horn: Flared in H-plane.
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Pyramidal horn: Flared in both planes (most common).
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Gain Calculation:
$$G = \frac{4\pi A_e}{\lambda^2} = \eta_a \frac{4\pi A_{phys}}{\lambda^2}$$
where $$\displaystyle A_{phys} = a \times b $$ (aperture dimensions), $$\displaystyle \eta_a $$ = efficiency (0.5–0.7).
For pyramidal horn, $$\displaystyle \eta_a \approx 0.51 $$ (approx).
- Aperture Efficiency: $$\displaystyle \eta_a = \eta_{illum} \cdot \eta_{spill} \cdot \eta_{block} $$ (illumination, spillover, blockage).
Parabolic Reflector Antenna
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Principle: Parallel rays from feed reflect off paraboloid → converge at focus (reverse for transmitting). Phase equality along aperture.
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Feed Mechanisms:
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Axial feed: Feed at focus; simple but blocks aperture.
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Offset feed: Feed off-axis; no blockage, lower sidelobes.
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Cassegrain: Subreflector (hyperbolic) reflects to feed behind dish.
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Design Considerations:
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Illumination Taper: Edge illumination ~ -10 dB to -15 dB for good efficiency/sidelobe trade-off.
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Spillover: Feed radiation missing reflector → increases noise, reduces efficiency.
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Aperture Blockage: Feed/support structures shadow aperture → reduces gain, increases sidelobes.
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Gain: $$\displaystyle G \approx \eta_a \left(\frac{\pi D}{\lambda}\right)^2 $$ (for circular dish, $D$ diameter).
[!TIP] Blockage Effect: Central blockage reduces gain by factor $$\displaystyle \left(1 - (d/D)^2\right)^2 $$ (d = blockage diameter) and raises sidelobes.
Slot Antennas
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Concept: Aperture in conducting plane. Radiates from slot edges.
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Babinet's Principle: Fields of complementary structures (slot vs dipole) related:
$$\mathbf{E}_{slot} \propto \mathbf{H}_{dipole}, \quad \mathbf{H}_{slot} \propto -\mathbf{E}_{dipole}$$
Impedances: $$\displaystyle Z_{slot} Z_{dipole} = \eta^2/4 $$.
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Rectangular Slot in Infinite Ground Plane:
- Radiation Pattern: Same as dipole orthogonal to slot. For $a \times b$ slot ($a$ along $x$, $b$ along $y$), E-plane cut ($$\displaystyle \phi=0 $$) pattern:
$$E_\theta \propto \frac{\sin\left(\frac{\beta a}{2} \sin\theta\right)}{\frac{\beta a}{2} \sin\theta} \cdot \cos\left(\frac{\beta b}{2} \cos\theta\right)$$
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Directivity: $$\displaystyle D \approx \frac{4ab}{\lambda^2} $$ (for $a,b \gg \lambda$).
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Applications: Slotted waveguide arrays (radar), aircraft wing slots.
Lens Antennas (Definitions)
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Principle: Dielectric lens (or metal-plate lens) focuses radiation from feed like optical lens.
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Types: Dielectric lens (Luneburg, hemispherical), metal-plate lens (E-plane, H-plane).
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Advantages: Low loss, good scan capability.
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Disadvantages: Heavy, bulky, frequency-sensitive (dielectric constant dispersion).
Tapered Apertures vs Uniform Apertures
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Uniform Aperture: Constant amplitude across aperture → high gain but high sidelobes (~ -13.2 dB for rectangular).
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Tapered Aperture: Amplitude tapers to edges (e.g., Taylor, binomial, cosine).
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Advantages: Reduces sidelobes significantly (Taylor: -20 to -30 dB).
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Disadvantages: Slightly lower gain, wider main beam.
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Tapering Functions:
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Binomial: $A(x) \propto \binom{N}{k}$; sidelobes eliminated, but wide beam.
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Taylor: Optimized for specified sidelobe level; near-optimum gain for given sidelobe.
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[!TIP] Trade-off: Sidelobe reduction always costs gain and beamwidth. Taylor distribution is popular for radar (low clutter).
4. ARRAY ANTENNAS & PATTERN SYNTHESIS
Antenna Arrays Fundamentals
- Pattern Multiplication Theorem: Total pattern = element pattern × array factor.
$$F_{total}(\theta,\phi) = f_{element}(\theta,\phi) \cdot F_{array}(\theta,\phi)$$
- Array Factor for $N$ identical elements:
$$F_{array} = \sum_{n=1}^N I_n e^{j \psi_n}$$
where $$\displaystyle \psi_n = \beta \mathbf{\hat{r}} \cdot \mathbf{d}_n + \alpha_n $$ (phase due to position $$\displaystyle d_n $$ and excitation phase $$\displaystyle \alpha_n $$).
Linear Array Design
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Broadside Array: Maxima at $$\displaystyle \theta = 90^\circ $$ (perpendicular to array axis).
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Condition: All elements in phase ($$\displaystyle \alpha_n = 0 $$) and uniform spacing $d$.
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Array Factor: $$\displaystyle F \propto \frac{\sin(N \psi/2)}{\sin(\psi/2)} $$, $$\displaystyle \psi = \beta d \cos\theta $$.
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End-fire Array: Maxima at $$\displaystyle \theta = 0^\circ $$ or $$\displaystyle 180^\circ $$ (along array axis).
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Condition: Progressive phase $$\displaystyle \alpha = -\beta d $$ (or $+\beta d$) to steer beam along axis.
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Array Factor: $$\displaystyle F \propto \frac{\sin(N (\psi+\beta d)/2)}{\sin((\psi+\beta d)/2)} $$.
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Beam Scanning (off broadside by $$\displaystyle \theta_0 $$):
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Required phase progression: $$\displaystyle \alpha = -\beta d \cos\theta_0 $$.
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Example: Scan to $$\displaystyle 30^\circ $$ off broadside, $$\displaystyle d = 3\,cm $$, $$\displaystyle f=64\,kHz $$ → $$\displaystyle \lambda = c/f \approx 4687\,m $$, $\beta d \approx 0.00004$ rad → $\alpha \approx 0$ (nearly broadside). Note: For HF, $d \ll \lambda$ so scanning limited.
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Directivity vs Array Length: $$\displaystyle D \approx \frac{2L}{\lambda} $$ for broadside (end-fire: $$\displaystyle D \approx \frac{4L}{\lambda} $$), where $$\displaystyle L = Nd $$.
[!TIP] Grating Lobes: Occur when $$\displaystyle d > \lambda $$ and scanning. Condition to avoid: $$\displaystyle d \leq \frac{\lambda}{1+|\sin\theta_0|} $$.
Schelkunoff Unit Circle Method
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Polynomial Representation: Array factor $$\displaystyle F(z) = \sum_{n=0}^{N-1} I_n z^n $$, where $$\displaystyle z = e^{j\psi} $$.
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Root Placement: Zeros of $F(z)$ on unit circle correspond to null directions.
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Design Example: For $$\displaystyle N=4 $$, zeros at $$\displaystyle \psi = 90^\circ, 180^\circ, 270^\circ $$ → $$\displaystyle z = j, -1, -j $$. Solve polynomial → excitation coefficients.
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Advantage: Graphical synthesis; ensures nulls at specified angles.
Binomial Array
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Excitation Coefficients: Binomial coefficients (Pascal's triangle): $$\displaystyle I_n = \binom{N-1}{n} $$.
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Pattern: No sidelobes (except main lobe), but wide main beam.
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Application: When sidelobe suppression is critical (e.g., low interference).
Taylor Synthesis
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For Sum Patterns: Approximate ideal pattern with specified sidelobe level.
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Method: Start with continuous distribution $$\displaystyle I(x) = I_0 \frac{\sin(\pi x)}{\pi x} \prod_{n=1}^{\bar{n}-1} \frac{1 - (x/n)^2}{1 - (x/\bar{n})^2} $$, where $\bar{n}$ controls sidelobe level.
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Discrete Approximation: Sample continuous distribution for array elements.
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Result: Near-optimum gain for given sidelobe level; first $\bar{n}-1$ sidelobes equal, rest decay.
Planar Arrays
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Configuration: Elements on 2D grid (rectangular, circular).
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Pattern: $$\displaystyle F(\theta,\phi) = f_{element}(\theta,\phi) \cdot F_x(\theta,\phi) \cdot F_y(\theta,\phi) $$ (separable).
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Requirements: Control both azimuth and elevation patterns; spacing $$\displaystyle d_x, d_y \leq \lambda/2 $$ to avoid grating lobes in both planes.
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Applications: Phased array radars, base station antennas.
5. WIDEBAND & SPECIAL ANTENNAS
Log-Periodic Antenna
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Structure: Series of driven and parasitic elements (toothed) along boom; lengths and spacings follow $$\displaystyle \tau = \frac{L_{n+1}}{L_n} < 1 $$, $$\displaystyle \sigma = \frac{s_n}{2L_n} \approx 0.05–0.2 $$.
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Frequency-Independent Principle: Input impedance and radiation pattern repeat every $\log f$ cycle. Self-similar structure.
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Operation: At any frequency, elements near $\lambda/2$ are active; others are too long/short → broadband.
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Bandwidth: Limited by smallest/largest elements; can exceed 10:1.
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Applications: TV reception, EMC testing, wideband communication.
[!TIP] Key Parameter: $\tau$ (scale factor) determines bandwidth: $$\displaystyle \text{BW} = \frac{f_{max}}{f_{min}} = \tau^{-(N-1)} $$, $N$ = number of elements.
Helical Antenna
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Normal Mode ($D \ll \lambda$, $C \approx \lambda$):
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Radiation Pattern: Figure-8 along helix axis (like dipole).
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Applications: HF communications (broadside radiation).
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Axial Mode ($D \approx \lambda/3$, $C \approx \lambda$, $L \approx n\lambda$):
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Radiation: Circularly polarized wave along helix axis (right-hand or left-hand CP).
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Gain: $$\displaystyle G \approx 15 \left(\frac{C}{\lambda}\right)^2 n $$ (approx). For $$\displaystyle C=\lambda $$, $$\displaystyle n=10 $$, $G \approx 15$ (11.8 dBi).
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Half-power beamwidth: $$\displaystyle \text{HPBW} \approx \frac{52^\circ \lambda^{3/2}}{C \sqrt{n}} $$ (narrower with more turns).
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Dimensions: $$\displaystyle C = \pi D \approx \lambda $$, $L \approx n\lambda$, pitch angle $$\displaystyle \alpha \approx 12^\circ–14^\circ $$.
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Microstrip Antennas
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Construction: Patch (conducting), substrate (dielectric), ground plane.
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Radiation Mechanism: Fringing fields at patch edges; patch acts as $\lambda/2$ resonator.
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Feeding Techniques: Microstrip line, coaxial probe, aperture coupling, proximity coupling.
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Rectangular Patch Design Equations (for $$\displaystyle W > h $$):
- Width $W$:
$$W = \frac{c}{2f_r} \sqrt{\frac{2}{\varepsilon_r + 1}}$$
\boxed{W = \frac{c}{2f_r} \sqrt{\frac{2}{\varepsilon_r + 1}}}
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Effective dielectric constant: $$\displaystyle \varepsilon_{eff} = \frac{\varepsilon_r + 1}{2} + \frac{\varepsilon_r - 1}{2}\left(1 + 12\frac{h}{W}\right)^{-1/2} $$
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Length $L$:
$$L = \frac{c}{2f_r \sqrt{\varepsilon_{eff}}} - 2\Delta L$$
where $$\displaystyle \Delta L \approx 0.412h \frac{(\varepsilon_{eff}+0.3)(W/h+0.264)}{(\varepsilon_{eff}-0.258)(W/h+0.8)} $$
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Advantages: Low profile, conformal, lightweight, low cost, easy integration with circuits.
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Limitations: Narrow bandwidth (1–5%), low efficiency (due to dielectric/surface wave losses), low gain (6–8 dBi), spurious feed radiation.
[!TIP] Bandwidth Limitation: Primarily due to high $Q$ of cavity. Thicker substrate ($h \uparrow$) and lower $$\displaystyle \varepsilon_r $$ increase bandwidth.
Yagi-Uda Antenna
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Construction:
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Driven element: $\lambda/2$ dipole (or folded dipole).
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Reflector: $\lambda/2$ dipole, ~5% longer than driven, placed $\lambda/4$ behind, passive (short-circuited).
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Directors: $\lambda/2$ dipoles, ~5% shorter than driven, spaced $\lambda/3$–$\lambda/4$ apart, passive.
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Boom: Non-conductive support.
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Role of Reflector: Reflects forward radiation, increases forward gain, reduces backward radiation.
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Role of Directors: Phase acceleration; each director re-radiates with phase leading driven element → constructive interference in forward direction.
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Design Example (6 elements, 12 dB gain at 200 MHz):
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$$\displaystyle f=200\,\text{MHz} \Rightarrow \lambda = 1.5\,m $$.
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Driven: $$\displaystyle 0.5\lambda = 0.75\,m $$.
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Reflector: $$\displaystyle 0.51\lambda = 0.765\,m $$, spacing $$\displaystyle 0.15\lambda = 0.225\,m $$.
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Directors (4): lengths $0.48\lambda, 0.46\lambda, 0.44\lambda, 0.42\lambda$; spacings $0.15\lambda, 0.25\lambda, 0.35\lambda, 0.4\lambda$ (typical).
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Gain $\approx 10–12$ dBi.
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Applications: TV reception, point-to-point links, amateur radio.
[!TIP] Design Trend: More directors → higher gain but diminishing returns; spacing ~0.3λ optimal.
6. PROPAGATION MECHANISMS (WAVE PROPAGATION)
Ground Wave Propagation
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Transition: Surface wave (bound to earth) → space wave (refracted upward) as height increases.
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Effect of Ground:
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Conductivity $\sigma$: Higher $\sigma$ (sea water) → lower attenuation, longer range.
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Permittivity $$\displaystyle \varepsilon_r $$: Affects wave tilt and attenuation.
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Terrain: Smooth (water) → low loss; rough (hilly) → scattering, diffraction loss.
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Vertical Pattern Influence: Ground reflection creates wave tilt; for vertical polarization, ground wave stronger at low angles.
Sky Wave Propagation (Ionospheric)
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Ionosphere as Variable Refractive Index Medium: Plasma frequency $$\displaystyle f_p = 9\sqrt{N_e} $$ ($$\displaystyle N_e $$ = electron density). Refractive index $$\displaystyle n = \sqrt{1 - (f_p/f)^2} $$. Decreases with height → bends rays downward.
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Critical Frequency $$\displaystyle f_c $$: Max frequency reflected vertically ($$\displaystyle \theta_i=0 $$). $$\displaystyle f_c = 9\sqrt{N_{e,max}} $$ (for layer).
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Virtual Height $h'$: Apparent reflection height assuming straight-line propagation. $$\displaystyle h' > h_{true} $$ due to refraction.
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Maximum Usable Frequency (MUF):
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Definition: Highest frequency that can be reflected for given path and angle.
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Derivation: From Snell's law for ionosphere: $$\displaystyle n \sin\theta_i = \text{constant} $$. At reflection, $$\displaystyle n=0 $$ → $$\displaystyle \sin\theta_i = n_{0} = f_c/f $$.
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$$\boxed{f_{MUF} = \frac{f_c}{\cos\theta_i}}$$
where $$\displaystyle \theta_i $$ = angle of incidence at ionosphere.
- Relation to Skip Distance $d$:
$$\boxed{d = 2 h' \tan\theta_i = 2 h' \sqrt{\left(\frac{f_{MUF}}{f_c}\right)^2 - 1}}$$
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Lowest Usable Frequency (LUF): Lowest frequency that provides acceptable signal-to-noise ratio; limited by atmospheric noise and absorption.
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Multi-hop Propagation: Signal reflects multiple times (earth-ionosphere) → longer distances.
[!TIP] MUF Calculation: Given $$\displaystyle f_c $$ and $$\displaystyle \theta_i $$, $$\displaystyle f_{MUF} = f_c / \cos\theta_i $$. For $$\displaystyle \theta_i=60^\circ $$, $$\displaystyle f_{MUF}=2f_c $$. Skip distance increases with MUF.
Space Wave Propagation
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Line-of-sight (LOS): Direct path; limited by Earth's curvature.
- Radio Horizon: $$\displaystyle d \approx 4.12(\sqrt{h_t} + \sqrt{h_r}) $$ km ($h$ in meters).
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Beyond Horizon:
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Super Refraction (Ducting): Refractive index decreases rapidly with height → rays bend more than Earth's curvature. Can trap waves in ducts (evaporation ducts over sea, surface ducts). Enables propagation beyond LOS (up to 500–1000 km).
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Tropospheric Scattering: Turbulence in troposphere scatters energy; allows communication beyond horizon (up to 500 km). Scatter volume concept; requires high power, large antennas.
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Effects: Ducting → strong signals, fading; scattering → weak, fluctuating signals.
Tropospheric Propagation
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Troposphere Structure: Up to ~10 km; refractive index decreases with height (standard atmosphere: $n-1 \propto 1/h$).
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Ducts:
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Surface-based duct: Strong inversion near surface.
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Elevated duct: Inversion layer aloft.
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Use in Microwave: Ducting can cause anomalous propagation (beyond LOS) for 1–10 GHz; also causes interference.
7. ENVIRONMENTAL & PRACTICAL EFFECTS ON PROPAGATION
Effects of Atmosphere, Terrain, and Obstacles
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Atmosphere:
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Refraction: Bends rays downward (effective Earth radius $k \approx 4/3$).
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Absorption: By oxygen (60 GHz), water vapor (22 GHz, 183 GHz).
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Scattering: By rain, fog (above 10 GHz).
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Terrain:
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Roughness: Causes diffuse scattering; reduces specular reflection.
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Slopes: Changes effective antenna height.
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Obstacles (buildings, vegetation):
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Diffraction: Around edges; knife-edge model.
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Penetration loss: Through walls, trees (frequency-dependent).
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Earth’s Effect on Antenna Patterns
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Vertical Pattern Distortion: Ground reflection combines with direct wave → interference pattern.
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Image Theory (perfect ground):
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Replace ground by image antenna (current opposite phase for vertical dipole, same phase for horizontal dipole).
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Total field = direct + reflected (with phase change: $$\displaystyle 180^\circ $$ for vertical pol, $$\displaystyle 0^\circ $$ for horizontal pol over perfect conductor).
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Real Ground: Finite conductivity → reflection coefficient $$\displaystyle \Gamma < 1 $$, phase not exactly $$\displaystyle 0^\circ $$ or $$\displaystyle 180^\circ $$. Reduces gain, tilts pattern.
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Monopole Example: Over perfect ground, pattern $$\displaystyle \propto \cos(\frac{\beta h}{2} \cos\theta) $$; over real ground, lower gain, higher elevation angle for max.
Broadcast Antenna Arrays
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Horizontal Patterns: Controlled by array of towers (AM: vertical polarization; FM: horizontal).
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AM Broadcast Arrays:
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Directional Arrays: Use towers with different excitations to shape horizontal pattern → protect other stations at night (skywave interference).
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Pattern: Cardioid, multi-lobed.
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FM Broadcast Arrays:
- Often circularly polarized; arrays for specific coverage.
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Coverage Area Optimization: Maximize signal in target area, minimize in others. Use superposition of array factors.
8. ADVANCED TOPICS & DESIGN TOOLS
Numerical Tools for Antenna Analysis
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Method of Moments (MoM): Integral equation solution; good for wires, surfaces. Basis functions, impedance matrix.
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Finite Element Method (FEM): Differential equation; good for complex dielectrics, cavities. Mesh generation.
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Finite Difference Time Domain (FDTD): Time-domain; broadband, transient analysis. Yee lattice.
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Software:
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HFSS (High-Frequency Structure Simulator): FEM/MoM, 3D.
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CST Microwave Studio: FDTD, integral equation.
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NEC (Numerical Electromagnetics Code): MoM for wires.
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Application: Predict patterns, impedance, SAR, etc.
Antenna Gain Measurement
- Standard Gain Horn Method: Compare unknown antenna to calibrated gain horn.
$$G_{unknown} = G_{horn} + 10\log_{10}\left(\frac{P_{un}}{P_{horn}}\right) - 10\log_{10}\left(\frac{A_{un}}{A_{horn}}\right) - \text{losses}$$
or using Friis: $$\displaystyle G_{un} = G_{horn} + 10\log_{10}(P_{un}/P_{horn}) - 10\log_{10}((4\pi R/\lambda)^2) - L $$.
- Example: Given oscillator power, attenuator reading, distance → compute gain.
Virtual Height
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Definition: Apparent reflection height assuming straight-line propagation. $$\displaystyle h' > h_{true} $$ due to refraction.
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Measurement: Using ionosonde; send pulse, measure round-trip time $t$ → $$\displaystyle h' = c t / 2 $$.
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Use: In MUF and skip distance calculations.
V-Antenna
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Definition: Two long wire antennas joined at an angle $\alpha$ (typically $$\displaystyle 90^\circ $$–$$\displaystyle 120^\circ $$).
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Pattern: Main lobe tilted from broadside by $\alpha/2$.
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Application: HF communication, where broadside pattern not desired.
Flat Sheet and Corner Reflectors
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Flat Sheet Reflector: Flat conducting plate placed $\lambda/4$ behind dipole → increases gain by ~6 dB, narrows beam.
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Corner Reflector: Two flat sheets at $$\displaystyle 90^\circ $$ (or $$\displaystyle 60^\circ $$); dipole at apex. Gain $\approx 8–10$ dBi, unidirectional, wide bandwidth.
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Principle: Image in reflector(s) creates array effect; spacing $\lambda/4$ gives in-phase addition.
END OF UNIT 4 NOTES
Focus on High-Frequency topics: Retarded Potential, Oscillating Dipole, Dipoles, Long Wire, Yagi, Microstrip, Parabolic Reflector, Sky Wave (MUF/Skip), Ground Wave, Space Wave.