The recorded ionogram
Select a pointCyan points are virtual heights from acquired vertical echo times. The dashed line marks peak plasma frequency. A pulse without a return has no height point.
B-X5 · Radio sounding
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.
02 / Measure the delay
Keep the real turning point beside the height inferred from time. The plasma makes those two answers different.
Send 45 narrow-band test pulses and keep every return or missing echo. Click a recorded ionogram point to launch that frequency again.
Cyan points are virtual heights from acquired vertical echo times. The dashed line marks peak plasma frequency. A pulse without a return has no height point.
The profile is the same one shown in the 3D cutaway. Gold marks the selected ray’s true turning height.
The same records, before height conversion
The delay plot uses exactly the same stored pulse records as the ionogram. This ideal instrument records time and return state; it has no amplitude, absorption or receiver noise.
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.
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.
Read the short institutional introduction about virtual height and critical-frequency traces. No archived image is used as this simulation’s data.
Read the introductory density, frequency and group-delay discussion. Magnetic mode splitting is outside this model.
Read equations 9.27–9.35 for the cold-plasma dispersion and group speed. The parabolic-layer solution is derived for the stated profile.
Physics tutorial
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
This cold unmagnetized plasma law gives the group speed of a narrow-band pulse. The phase speed is different.
Angles are measured from vertical. Horizontal wave number stays fixed; the vertical component reaches zero at the turn.
The height definition applies to vertical soundings. For oblique paths half the light-speed delay is a virtual slant range.
This secant-law threshold assumes a flat, single layer. Its equality is an infinite-delay limit in the ideal parabolic ray model.
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.
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.
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.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.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.