---
title: "MUF, critical frequency and skip (curved earth)"
subject: "Propagation and Antenna"
chapter: 4
key: "semester_6/propagation_and_antenna:muf-fcr-skip-curved-earth"
source: https://www.bctengineer.com/q/semester_6/propagation_and_antenna/muf-fcr-skip-curved-earth
site: BCT Engineering
---

# MUF, critical frequency and skip (curved earth)

Propagation and Antenna · Chapter 4: Propagation and Radio Frequency Spectrum

- Asked in: 2075 Bhadra, 2+8 marks
- Video: [Maximum Usable Frequency (MUF) (Definition, Basics, Derivation, Formula & Calculation) Explained](https://www.youtube.com/watch?v=0Houq2d-Jtk) — Engineering Funda
- Answer checked by Claude Opus 5.5 (high effort) on 2026-10-14
- Page: https://www.bctengineer.com/q/semester_6/propagation_and_antenna/muf-fcr-skip-curved-earth
- Whole chapter: https://www.bctengineer.com/md/semester_6/propagation_and_antenna/chapter-4

## Question

What is Maximum Usable Frequency (MUF)? Derive the expression of MUF, critical frequency (fcr) and skip distance assuming curved earth.

## Short answer

MUF is the highest frequency reflected between two points for a given angle of incidence. f_MUF = fcr sec φ with fcr = 9√Nmax (critical frequency). For curved earth, tan φ = R sin(D/2R)/(R+h−R cos(D/2R)), and skip distance D = (2R/k)[1−√(1−2k²h/R)] with k = √((f/fcr)²−1).

## Answer

#### Maximum Usable Frequency (MUF)
The **MUF** is the highest frequency that is returned to earth by the ionosphere between two given points (for a given angle of incidence). Higher frequencies pass through the layer. It is related to the critical frequency fcr (highest frequency reflected at vertical incidence) by the secant law: **f_MUF = fcr sec φ**. In practice the optimum working frequency OWF ≈ 0.85 MUF is used.

#### Derivation for curved earth
**Assumptions:** spherical earth of radius R; layer acting as a thin reflector at virtual height h; both antennas on the ground; reflection point P above the mid-point of the path.

First, the secant law. The refractive index of the layer is n = √(1 − 81N/f²). By Snell's law, a ray entering at angle φ returns where n = sin φ:
```text
1 − 81Nmax/f² = sin² φ
81Nmax/f²     = cos² φ
f = 9√Nmax / cos φ = fcr sec φ,   fcr = 9√Nmax
```

Then the curved-earth geometry:

```text
               P  (reflection point, height h)
              /|\
             / | \      φ = angle of incidence at P
            /φ |  \
   ~~~~~~~~/~~~|~~~\~~~~~~~ ionosphere
       T  /    |    \  R    (on earth surface)
        \.     |     ./
          `.   |θ  .'       θ = D / (2R)
            `. | .'
               O  (earth centre)
   OT = R,  OP = R + h,  arc TR = D
```

Step 1: Drop a perpendicular from T onto OP. Its foot Q lies at distance R cos θ from O, and TQ = R sin θ. In triangle TQP:
```text
QP    = (R + h) − R cos θ
tan φ = TQ / QP = R sin θ / (R + h − R cos θ)
```
Step 2: Secant law for the ionosphere (from n = √(1 − 81N/f²) and Snell's law): f_MUF = fc sec φ, with fc = 9√Nmax. So:
```text
f_MUF = fc √(1 + tan² φ)

f_MUF = fc √{ 1 + [ R sin(D/2R) /
              (R + h − R cos(D/2R)) ]² }
```
Step 3: For D small compared with R, sin θ ≈ θ = D/2R and cos θ ≈ 1 − θ²/2:
```text
tan φ ≈ (D/2) / (h + D²/8R)
f_MUF ≈ fc √{ 1 + [ (D/2) / (h + D²/8R) ]² }
```
Step 4: Skip distance for a given frequency f. Let k = √[(f/fc)² − 1] = tan φ:
```text
D/2 = k (h + D²/8R)
(k/8R) D² − D/2 + k h = 0
D = (2R/k) [ 1 − √(1 − 2k²h/R) ]   (smaller root)
```
Check: as R → ∞, √(1 − x) ≈ 1 − x/2, so D → 2kh = 2h√[(f/fc)² − 1], the flat-earth result.

Step 5: Limit due to curvature. The largest angle φ occurs when the ray leaves the transmitter along the horizon (tangent at T):
```text
sin φmax = R / (R + h)
f_MUF(max) = fc sec φmax
D_max (one hop) = 2R cos⁻¹[R / (R + h)]
```
For h = 300 km, R = 6370 km: sin φmax = 0.955, φmax = 72.8°, sec φmax = 3.37, D_max ≈ 3836 km. So single-hop MUF cannot exceed about 3.4 fc.

#### Summary
```text
fcr   = 9 √Nmax
f_MUF = fcr sec φ,
tan φ = R sin(D/2R) / (R + h − R cos(D/2R))
D     = (2R/k)[1 − √(1 − 2k²h/R)],  k = √[(f/fcr)² − 1]
```

**Example:** fcr = 8 MHz, h = 300 km, f = 16 MHz: k = √3 = 1.732; D = (2 × 6370/1.732)[1 − √(1 − 2 × 3 × 300/6370)] ≈ 1125 km (the flat-earth formula gives 1039 km).

## Check yourself

The answer's key points as multiple-choice questions, with the correct option and why.

1. Using Snell's law n = sin(phi), the secant law is obtained as:
   A. f = 9 sqrt(Nmax)/cos(phi) = fcr sec(phi)
   B. f = 9 sqrt(Nmax) cos(phi)
   C. f = fcr tan(phi)
   D. f = 81 Nmax sec(phi)
   Answer: A. 1 - 81Nmax/f^2 = sin^2(phi) gives 81Nmax/f^2 = cos^2(phi). (Key point: Secant law derivation)

2. The optimum working frequency used in practice is about:
   A. 1.5 MUF
   B. 0.85 MUF
   C. 0.85 fcr
   D. MUF exactly
   Answer: B. It allows a margin for ionospheric variations. (Key point: OWF)

3. For curved earth, with k = sqrt[(f/fcr)^2 - 1], the skip distance is:
   A. D = 2kh
   B. D = (2R/k)[1 + sqrt(1 - 2k^2 h/R)]
   C. D = (2R/k)[1 - sqrt(1 - 2k^2 h/R)]
   D. D = kR/2h
   Answer: C. It is the smaller root of (k/8R)D^2 - D/2 + kh = 0. (Key point: Skip distance equation)

4. In the example (fcr = 8 MHz, h = 300 km, f = 16 MHz) the curved-earth skip distance compared with flat earth is:
   A. Smaller
   B. Equal
   C. Zero
   D. Larger (about 1125 km vs 1039 km)
   Answer: D. Curvature reduces the incidence angle for a given D, so the skip distance is longer. (Key point: Curvature effect on value)

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