EW Math Guide

Full Radar and EW Mathematics Course

A complete section-by-section learning path covering the full radar and electronic warfare formula set: EW concepts, antennas, propagation, noise, jamming, pulse/CW radar, detection, Doppler, horizon, radar equations, RCS, retroreflectors and dB units.

How To Use This Page

This is the complete course map. Each card corresponds to a topic family from the full radar/EW formula collection. The thematic subpages explain the most important subjects in more depth; this page makes sure no major topic is left out.

1. Read

Start with the technical idea in each card. It tells you why the formula matters operationally.

2. Calculate

Use the displayed formula with consistent SI units unless a dB shortcut explicitly states km/GHz.

3. Connect

Move from isolated formulas to system budgets: antenna gain, propagation loss, receiver noise, processing and jammer geometry.

Index-Following Course Map

This map follows the complete technical index as a course outline. The wording and diagrams are original, but the order is intentionally aligned with the source document so no major subject family is skipped.

1. Electronic Warfare Fundamentals

EW, ES, EA and EP. Start by separating the mission from the math. Electronic support measures the spectrum: who is transmitting, where, with which waveform and with what tactical meaning. Electronic attack tries to reduce hostile measurement quality through noise, deception, decoys or expendables. Electronic protection restores friendly margin through antenna design, processing, emission control, agility and LPI design.

Training scenario. An intercept receiver detects a pulsed X-band emitter with stable PRI and narrow antenna scan. ES classifies it as a tracking radar; EA planning then asks whether a noise jammer, range deception or angular deception is the right response; EP asks how the radar might reject the attack.

2. Frequency Bands, Radar Frequencies and ISM Bands

Frequency is the first engineering decision because it sets wavelength. Wavelength determines practical antenna aperture, Doppler scale, scattering region, atmospheric loss and achievable resolution. ISM bands matter because many commercial emitters, drones and datalinks operate there, creating both interference and exploitation opportunities.

λ = c0/f
λm ≈ 0.3/fGHz

Example. At 2.4 GHz, λ is about 12.5 cm; at 10 GHz it is 3 cm. A target feature that is electrically small at 2.4 GHz may be a much stronger scatterer at X band.

3. Antenna Models and Patterns

This lesson covers isotropic reference antennas, dipoles, apertures, phased arrays, parabolic reflectors, horns and electronically scanned arrays. The key concept is that an antenna pattern is a spatial weighting function. The main beam gives gain; sidelobes create unwanted receiving directions.

G = η4πA/λ2
Θ ≈ kλ/D
ΩA ≈ θAzθEl

Graphic assignment. The antenna module uses an original main-lobe/sidelobe diagram and should be expanded with a phased-array steering diagram showing element spacing, phase shift and grating-lobe risk.

4. Field Regions, Gain, Efficiency, Beamwidth and Solid Angle

Near-field/far-field boundaries tell you when normal radar and antenna equations are valid. Gain and beamwidth are coupled through aperture size; efficiency prevents ideal formulas from overstating real performance.

RFF ≥ 2D2
G ≈ 4π/ΩA

Example. A 2 m aperture at 10 GHz has a far-field distance around 267 m. If you test it at 30 m without compact-range correction, the measured pattern can be misleading.

5. Link Budget and Propagation

Link budget starts with transmitted power and antenna gains, then subtracts free-space path loss and real-world losses. Fresnel clearance, earth bulge, atmospheric absorption, rain, polarization mismatch, two-ray reflection and knife-edge diffraction explain why field performance differs from a clean equation.

LFSPL,dB = 92.45 + 20log10Rkm + 20log10fGHz
r1 = √(λd1d2/(d1+d2))

Example. A microwave link over water may meet FSPL budget but still fade deeply because the reflected ray arrives out of phase with the direct ray.

6. Command-Guided Missile Antenna Beams

Command-guided systems use antenna beam geometry to keep the missile, target and guidance link coherent. The mathematics is essentially beamwidth, angular error and update-rate management. A narrow beam improves angular precision but demands tighter pointing and tracking.

Sa ≥ 2Rsin(Θ/2)
Angular error grows into linear miss distance as range increases.

Example. A 1° angular error at 10 km corresponds to roughly 175 m lateral displacement, which is unacceptable for terminal guidance unless corrected by tracking updates.

7. Receiver Noise and Digital Signal Quality

Noise factor, noise figure, equivalent temperature, SQNR, SINAD, SNIR and ENOB describe how much useful information survives the receiver chain. These quantities decide whether a mathematically detectable echo is actually measurable.

N = kTB
NFdB = 10log10F
SQNRdB ≈ 6.02Nbits + 1.76
ENOB = (SINAD - 1.76)/6.02

Example. A 1 MHz receiver with 5 dB NF has a noise floor near -109 dBm. A -96 dBm echo has about 13 dB SNR before processing losses.

8. Chaff, Radar Decoys and Expendables

Chaff creates a volume of resonant dipoles, while decoys create false targets using passive RCS or active retransmission. The key learning point is that the radar sees a resolution cell full of scatterers, not a single object.

ldipole ≈ λ/2
V = πθAzθElR2c0τ/8

Example. X-band chaff uses much shorter dipoles than L-band chaff. As the cloud spreads, density falls and the apparent target changes with time and wind.

9. Electronic Jamming and Deception

Noise jamming attacks SNR; deception jamming attacks measurement validity. The course covers burn-through, J/S, self-protection jamming, escort/support/stand-in/stand-off jamming and communications jamming.

J/S = 4πR2ERPJ/(σERPR)
RBT = √[σERPR(J/S)req/(4πERPJ)]
ΔR = c0Δt/2

Example. A 1 µs delayed coherent retransmission appears 150 m away from the true return. If the delay is slowly increased, a range tracker can be pulled away from the real target.

10. Pulse Radar

Pulse radar topics include blind range, unambiguous range, chirp radar, Barker codes, near-perfect codes, peak sidelobe level and duty cycle. The central trade is energy versus resolution: long pulses carry energy, while bandwidth or short pulse duration provides resolution.

R = c0td/2
Runamb ≈ c0/(2PRF)
D = τPRF
Sr,chirp ≥ c0/(2B)

Example. A 20 MHz chirp gives about 7.5 m range resolution even if the transmitted pulse is long enough to carry much more energy than a 7.5 m unmodulated pulse.

11. CW, FMCW, FMiCW and Doppler

Unmodulated CW measures velocity but not range. FMCW adds a frequency ramp so beat frequency maps to range. Doppler is the measurement of radial motion; tangential motion alone does not shift frequency.

fD = 2vr
RFMCW = c0fb/(2S)
vunamb ≈ PRFλ/4

Example. At 10 GHz, a 250 m/s radial target produces about 16.7 kHz Doppler shift.

12. Detection Probability, False Alarms, Dwell and Hits

Detection is statistical because noise, clutter and target RCS fluctuate. Dwell time and hits per scan determine how many pulses are available for integration. False alarm thresholds trade sensitivity against operator or tracker overload.

TD ≈ ΘAz/scan-rate
Hits ≈ TDPRF
FAR = Nfalse/Tobs

Example. A 2° beam scanning at 60°/s dwells for about 33 ms. At 1 kHz PRF, that is about 33 pulses for possible integration.

13. Height Estimation, Ducting, Refraction and Horizon

Radar beams bend in the atmosphere. Normal refraction extends the radio horizon; ducting can trap energy and create long ranges or coverage holes. Height estimation must therefore treat the atmosphere as part of the geometry.

Rhorizon,km = 4.12√hm
RLOS,km = 4.12(√hradar + √htarget)

Example. A 20 m radar can see a 1000 m target to about 149 km under the standard effective-earth approximation.

14. Radar Resolution Cell

The radar resolution cell is the 3D measurement volume defined by range resolution and angular beamwidth. Point targets inside one cell merge; volume targets such as rain or chaff fill the cell.

Sr ≥ c0τ/2
Sa ≥ 2Rsin(θ/2)
V = πθAzθElR2c0τ/8

Example. At 50 km with a 2° beam, classical angular separation is on the order of kilometers, even if range resolution is only meters.

15. One-Way and Two-Way Radar Equations

One-way equations apply to links and intercept receivers. Two-way equations apply to monostatic point-target radar. Loss budgets and Swerling fluctuation models bridge ideal power math to real detection probability.

Pr,one-way = EIRPtGrλ2/(4πR)2
Rmax = [(PtτG2λ2σ)/((4π)3kTSNRLtot)]1/4

Example. Adding 6 dB loss reduces monostatic radar range by about 29%, because range is a fourth-root result.

16. Weather Radar and Volume Targets

Weather radar does not observe one point scatterer. It observes a volume containing many droplets, so the illuminated volume grows with range and changes the range law compared with a point target.

V = πθAzθElR2c0τ/8
Weather return depends on volume reflectivity rather than single-target σ.

Example. A rain cell at longer range fills a larger resolution volume, partly offsetting geometric spreading compared with a single point target.

17. Radar Cross Section and Scattering Regions

RCS depends on target size relative to wavelength, aspect angle, material and polarization. Rayleigh, Mie and optical regions describe how scattering changes as the target becomes electrically larger.

σ = limR→∞4πR2|Es|2/|E0|2
Rayleigh trend: σ ∝ r64
Optical sphere: σ ≈ πr2

Example. A small drone may be weak at lower frequency but stronger at shorter wavelength when its structural features become comparable to λ.

18. Complex Targets, RCS Examples and Retroreflectors

Complex targets combine specular returns, edge diffraction, cavities, creeping waves and multiple interactions. Retroreflectors deliberately send energy back toward the radar and are used for calibration and decoys.

Trihedral corner: σ ≈ 4πa4/(3λ2)
σdBsm = 10log10(σ/1m2)

Example. Doubling a corner reflector edge length increases ideal RCS by 12 dB because the edge length is raised to the fourth power.

19. Decibels and Symbol Glossary

Decibels turn multiplication into addition and make large radar ratios manageable. The symbol glossary is not administrative; it is a unit-control tool. Most wrong radar calculations are unit mistakes.

LP,dB = 10log10(P2/P1)
LE,dB = 20log10(E2/E1)
dBm = 10log10(PmW)

Example. 500 W = 27 dBW. A 3 dB change is approximately a factor of two in power.

Part A: EW Concepts and Spectrum

Electronic Warfare Areas

EW is divided into support, attack and protection. Mathematically, ES estimates emitter parameters, EA reduces hostile SNR or creates false measurements, and EP restores margin through design and tactics.

AreaEngineering Measurement
ESFrequency, bandwidth, bearing, modulation, pulse timing, polarization.
EAJ/S, false range, false Doppler, angular error, denied link margin.
EPProcessing gain, agility, sidelobe suppression, LPI, filtering.

Frequency, Wavelength and Bands

λ = c0 / f
λm ≈ 300 / fMHz = 0.3 / fGHz

Frequency band determines likely antenna size, propagation behavior, Doppler scale, resolution potential and atmospheric loss.

At 3 GHz, λ = 0.1 m. At 10 GHz, λ = 0.03 m, so the same aperture has about 10.5 dB more theoretical gain.

Part B: Antennas

Field Regions

Rreactive < 0.62√(D3/λ)
Rfar ≥ 2D2

Use far-field formulas only after the wavefront has become approximately planar. Antenna test ranges and radar cross-section ranges must respect this boundary.

A 2 m aperture at 10 GHz reaches far field near 267 m.

Pattern, Gain and Efficiency

G = η4πA/λ2
GdBi = 10log10G
η = Aeffective/Aphysical

Gain is not free power; it is directional concentration. Efficiency includes illumination taper, feed loss, spillover and surface errors.

Beamwidth and Solid Angle

Θ ≈ kλ/D
ΩA ≈ θAzθEl
G ≈ 4π/ΩA

Beamwidth controls search volume, angular resolution and support-jamming geometry. Use radians for solid-angle math.

Polarization Loss

Lpol,dB = -10log10pol)

Polarization mismatch reduces target return or link power. It is especially important for chaff, rain, circular polarization and volume targets.

Part C: Link Budget and Propagation

Free-Space Path Loss

LFSPL,dB = 92.45 + 20log10Rkm + 20log10fGHz

FSPL is isotropic spreading loss. It is the clean baseline before terrain, atmosphere, rain and antenna effects.

50 km at 10 GHz gives 146.4 dB FSPL.

Fresnel Zone

r1 = √(λd1d2/(d1+d2))
FZ = 4πhTXhRX

Clearance through the first Fresnel zone is needed for reliable point-to-point links.

Earth Bulge, Refraction and Horizon

Rhorizon,km = 4.12√hm
RLOS,km = 4.12(√hradar + √htarget)

Normal refraction bends radio paths slightly downward, modeled with an effective earth radius. Ducting can extend or distort this assumption.

Two-Ray and Knife-Edge

Pr,two-ray ∝ hTX2hRX2/d4
ν = h√[2(d1+d2)/(λd1d2)]

Two-ray explains sea/ground fading. Knife-edge diffraction estimates loss behind ridges or obstructions.

Atmospheric and Rain Attenuation

Ltotal = LFSPL + Lgas + Lrain + Lfog + Lpol + Lmisc

Atmospheric loss is often ignored below roughly 10 GHz for moderate ranges, but it becomes important at high microwave and millimeter-wave frequencies.

Part D: Receiver, Noise and Digital Quality

Noise Factor, Figure and Temperature

F = SNRin/SNRout
NFdB = 10log10F
Te = 290(F - 1)

Noise figure tells how much the receiver degrades SNR. Equivalent temperature expresses that degradation as input noise temperature.

Thermal Noise

N = kTB
NdBm ≈ -174 + 10log10BHz + NFdB

Bandwidth is a direct noise multiplier. Narrow filters improve sensitivity but can reject signal energy if mismatched.

SQNR, SINAD and ENOB

SQNRdB ≈ 6.02N + 1.76
ENOB = (SINADdB - 1.76)/6.02

These formulas describe digitizer quality. Real ADCs lose performance through clock jitter, nonlinearity and front-end distortion.

SNIR

SNIR = S/(N + I)
SNIRdB = SdB - 10log10(N + I)

SNIR is often more operationally useful than SNR because interference and jamming add to the noise-like denominator.

Part E: Chaff, Decoys and Jamming

Chaff

ldipole ≈ λ/2
σcloud ≈ Nσdipole for an ideal incoherent cloud

Chaff effectiveness depends on dipole length, cloud density, polarization, wind spreading and the radar resolution cell.

Radar Decoys

False range: ΔR = c0Δt/2
False Doppler: ΔfD = 2Δv/λ

Active decoys and repeaters create controlled timing, frequency or angular errors. Passive decoys rely on large RCS.

Self-Protection J/S and Burn-Through

J/S = 4πR2ERPJ/(σERPR)
RBT = √[σERPR(J/S)req/(4πERPJ)]

Jammer power is one-way; radar echo is two-way. Closing range favors the radar echo.

Support and Communications Jamming

Support: (J/S)dB = ERPJ - ERPR + 11 + GS - GM + 40logRT - 20logRJ - 10logσ
Comms: J/S = ERPJGSRT2/(ERPTGMRJ2)

Support jamming depends strongly on sidelobe gain and platform geometry. Communications jamming is a one-way link competition.

Part F: Pulse Radar, CW Radar and Doppler

Pulse Timing

PRF = 1/PRT
R = c0td/2
Rblind = c0(τ+trecovery)/2

Pulse timing controls range measurement, blind range and ambiguity.

Unambiguous Range and Velocity

Runamb ≈ c0/(2PRF)
vunamb ≈ PRFλ/4

This is the Doppler dilemma: low PRF helps range; high PRF helps velocity.

Pulse Compression, Chirp and Barker Codes

PCR ≈ Bτ
Sr ≥ c0/(2B)
PSLdB = 20log10(xi/x0)

Pulse compression gives energy of a long pulse with resolution of a short pulse. Code sidelobes matter for weak targets near strong ones.

CW, FMCW and FMiCW

fD = 2vr
RFMCW = c0fb/(2S), S = df/dt

Unmodulated CW measures velocity; FMCW adds range through beat frequency.

Part G: Detection, Dwell and Tracking

Probability of Detection and False Alarm Rate

FAR = Nfalse/Tobs
Threshold rises as allowed false alarm probability decreases.

Detection is statistical. Required SNR depends on target fluctuation, integration, false alarm probability and desired detection probability.

Dwell Time and Hits Per Scan

TD ≈ ΘAz/scan-rate
Hits ≈ TDPRF

More hits can improve integration, but slower scan rates reduce update rate.

Radial Speed and JEM

vr = v cos(α)
fD = 2vr

Only radial velocity creates Doppler. Jet engine modulation adds micro-Doppler features from rotating blades.

Resolution Cell

Sa ≥ 2Rsin(θ/2)
V = πθAzθElR2c0τ/8

Point targets merge inside one cell. Volume targets such as rain or chaff fill the cell and scale differently with range.

Part H: Radar Equations, Losses and Weather

One-Way Equation

Pr = EIRPtGrλ2/(4πR)2

Use for communications, intercept receivers and secondary radar.

Two-Way Radar Equation

Rmax = [(PtτG2λ2σ)/((4π)3kTSNRLtot)]1/4

Use for monostatic radar detection of point targets.

Loss Budget

Ltot,dB = La+Lant+LB+Ln+Lf+Li+Lr+Lt+Lx

Atmosphere, beamshape, filtering, fluctuation, integration and line losses all reduce range.

Weather Radar

V = πθAzθElR2c0τ/8
Weather return uses volume reflectivity rather than point RCS.

Because the illuminated volume grows with R2, weather radar range behavior differs from point-target radar.

Part I: RCS, Retroreflectors and dB

RCS Definition and Simple Shapes

σ = limR→∞4πR2|Es|2/|E0|2
Sphere optical: σ = πr2
Plate normal: σ = 4πa2b22

RCS is aspect-, frequency- and polarization-dependent. Real targets fluctuate as scattering centers add and cancel.

Rayleigh, Mie and Optical Regions

Rayleigh trend: σ ∝ r64
Optical trend: σ ≈ projected/scattering area

Small targets become far more visible as wavelength shrinks. Resonance can produce peaks and nulls.

Retroreflectors

Trihedral: σ ≈ 4πa4/(3λ2)
Van Atta trend: σ ≈ πn2λ2/4

Retroreflectors are designed to send energy back toward the source and can create high RCS in compact packages.

Decibels and Absolute Units

LP,dB = 10log10(P2/P1)
LE,dB = 20log10(E2/E1)
σdBsm = 10log10(σ/1m2)

Use dBm for power relative to 1 mW, dBW for 1 W, dBi for isotropic gain and dBsm for RCS.