The normal troposphere

Last Updated on July 11, 2026 by John Berry

It’s difficult for radio amateurs to understand all the various propagation mechanisms without understanding the core benchmark. That benchmark is the normal lower atmosphere or normal troposphere.

The normal, non-ionised troposphere comprises mainly atoms of nitrogen and oxygen, water vapour, and lesser concentrations of other gases like argon. The density of atoms and molecules typically reduces with height.

Photo by Miguel A Amutio on Unsplash

Refraction in the normal troposphere

The fact that the density of the troposphere reduces with height is hugely important in propagation. I’ve shown this in the diagram below.

Image shows propagation in a vacuum for reference as a straight line. But in the normal troposphere, the ray is shown bent as the wave is refracted towards the surface of the Earth.
I’ve shown the ray bent in the normal troposphere. The wave is refracted towards the surface of the Earth.

A radio wave propagates in a straight line in a vacuum. I’ve shown this in black above, with the wave front advancing from Station A. This signal would be lost to space with low signal level arriving at Station B. Communications with that station would likely be impossible.

A radio wave propagating in a normal troposphere shown in white would encounter a decreasing particle density with height. The lower parts of the wave front would be slowed down more than the upper parts. As a result, the ray representing propagation would be refracted towards the higher density at the bottom of the troposphere. The ray would be bent towards the surface of the Earth.

As a result of this refraction, communications with Station B may be possible. If we ignore excess losses, such as that from obstructions, path loss is given by the Free Space Loss equation .

4/3 Earth radius

Without a useful distortion, we’d have to draw curved lines when analysing paths between stations in a normal troposphere. Conveniently, we can distort the Earth’s radius instead, and draw a straight line between the stations.

To enable this, we use an effective Earth radius of 4/3 representing the radius exceeded for 50% of time. This effective Earth radius is 8,495km.

This distortion of the Earth’s radius yields an effective Earth radius is shown below.

Image shows the effect of refraction in the normal troposphere. The straight line between stations is drawn with an effective Earth radius of 4/3.
A standard approach to path analysis is to draw the path between the stations as a straight line while increasing the Earth radius by 4/3

In fact, the effective Earth radius varies with time and locations for any path. The degree to which this beam bending occurs depends on the air pressure, the temperature, and the density of water in the troposphere. Those parameters vary day by day, hour by hour, and even minute by minute.

An anomalous troposphere

This phenomenon of beam bending is hugely important to radio amateurs.

Firstly, as noted above, radio waves don’t travel in straight lines in the troposphere. They are bent towards the surface of the Earth. Hence propagation distances (over those determined by straight line ray tracing) are typically enhanced.

And secondly, the effective Earth radius goes well above 4/3 for small percentages of time. This means that any path which ordinarily contains obstructions blocking the signal might be flattened. A path that ordinarily suffers huge diffraction loss (and hence does not support communications) may become a free space path for a short time. Radio amateurs call this a ‘tropo opening’ and say that ‘lift conditions’ exist.

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