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Sandbox Physics

B-X5 · Radio sounding

Radio Echoes from the Ionosphere

Why does a radio echo suggest a higher layer than the height where the wave actually turns? A pulse slows as it enters the plasma. Converting its round-trip delay into a height with the vacuum speed of light therefore places the apparent reflection above the actual turning point.

Send a radio pulse into an electron layer and follow its return or escape. Sweep the frequency, record the echo delays and compare the virtual height with the true turning height.

Interactive modelRadio Echoes from the Ionosphere

02 / Measure the delay

The echo is a clock. Is it also a ruler?

Keep the real turning point beside the height inferred from time. The plasma makes those two answers different.

Peak plasma frequency—\text{—}
True turning height—\text{—}
Round-trip delay—\text{—}
Virtual height or slant range—\text{—}
Ground landing distance—\text{—}

Record a vertical frequency sweep

Send 45 narrow-band test pulses and keep every return or missing echo. Click a recorded ionogram point to launch that frequency again.

The electron layer behind the echoes

The profile is the same one shown in the 3D cutaway. Gold marks the selected ray’s true turning height.

What the delay measures

For a vertical sounding, the vacuum light speed turns half the travel time into a virtual height. At an oblique angle that same quantity is a virtual slant range. The true turning height follows the plasma density and the conserved horizontal wave number.

h′=cτ2(θ0=0),n2(zt)=sin⁡2θ0h'=\frac{c\tau}{2}\quad(\theta_0=0),\qquad n^2(z_t)=\sin^2\theta_0

At the exact critical limit this ideal parabolic ray takes indefinitely long to turn. Near a cutoff, real finite-bandwidth pulses need a full wave calculation. This forward simulation does not infer an unknown density profile from field measurements.

Sources and reading scope

Physics tutorial

Radio Echoes from the Ionosphere

BackgroundSend a radio pulse into an electron layer and follow its return or escape. Sweep the frequency, record the echo delays and compare the virtual height with the true turning height.

Why it mattersAn echo gives a travel time. Learning the height of an atmospheric layer takes a model of how the pulse moves.

Start with the essentials

Focus question
Why does a radio echo suggest a higher layer than the height where the wave actually turns?
One-sentence intuition
The group delay measures a virtual height; the turning point belongs to the density profile and the selected frequency.

Core mathematical model

The plasma changes the wave speed

ω2=c2∣k∣2+Nee2ϵ0me,vg=cn<c\omega^2=c^2|\mathbf{k}|^2+\frac{N_e e^2}{\epsilon_0m_e},\qquad v_g=cn<c

This cold unmagnetized plasma law gives the group speed of a narrow-band pulse. The phase speed is different.

Horizontal symmetry fixes the ray

p=nsin⁡θ=sin⁡θ0,n2(zt)=p2p=n\sin\theta=\sin\theta_0,\qquad n^2(z_t)=p^2

Angles are measured from vertical. Horizontal wave number stays fixed; the vertical component reaches zero at the turn.

Delay gives a virtual height

h′=cτ2,τ=2c∫0ztdzn2(z)−p2h'=\frac{c\tau}{2},\qquad \tau=\frac{2}{c}\int_0^{z_t}\frac{dz}{\sqrt{n^2(z)-p^2}}

The height definition applies to vertical soundings. For oblique paths half the light-speed delay is a virtual slant range.

An oblique wave can return at a higher frequency

fm=12πNme2ϵ0me,fthreshold=fmcos⁡θ0f_m=\frac{1}{2\pi}\sqrt{\frac{N_m e^2}{\epsilon_0m_e}},\qquad f_{\mathrm{threshold}}=\frac{f_m}{\cos\theta_0}

This secant-law threshold assumes a flat, single layer. Its equality is an infinite-delay limit in the ideal parabolic ray model.

Common difficulties

Virtual height and a mirror

Typical misconceptionThe ionogram shows where a physical reflecting surface sits.

Better mental modelThe electron density changes continuously. A pulse bends and slows along its path; its travel time alone does not give the true turning height.

A cutoff and a working radio link

Typical misconceptionA returning path guarantees a usable signal at its landing point.

Better mental modelThis model calculates paths and delays. Absorption, antenna patterns, noise and a real receiver determine signal strength and practical availability.

Run the experiment

  1. 01

    Start with a vertical echo

    Select “A vertical echo” and press “Launch pulse”. Compare the true turning height with the virtual height.

    What to observe: The pulse returns to the same sounder. The virtual height is larger because propagation slows inside the layer.
  2. 02

    Record an ionogram

    Press “Acquire vertical sweep”. Increase peak density and repeat. Export the CSV to inspect each simulated delay.

    What to observe: The return limit moves upward with the square root of peak density. The trace bends to long delays near the limit.
  3. 03

    Change only the direction

    Compare the two 9 MHz presets. Open the turning-point view after the oblique launch.

    What to observe: The vertical ray penetrates; the oblique ray turns and reaches a distant ground point. Its delay is labeled as slant range.
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