by William R. Hepburn, DX Info Centre
Tropospheric propagation is radio propagation that occurs in the lowest
layer of the Earth's atmosphere - the troposphere. It is 100% weather-related. A
Tropo DX mode is
any abnormal condition
that scatters, reflects or refracts VHF, UHF and/or microwave signals in
the troposphere causing changes to their normal coverage. Another name
for this is anomalous propagation, or AP for short. Tall mountain
ranges form a physical barrier to tropospheric propagation, thus tropo
is more rare in or across mountainous regions. Deserts are usually too
dry to support the long distance tropospheric modes. There are six main
tropospheric DX modes. The refraction and ducting effects are similar to
those that cause visual mirages. Therefore, the distant signals
received via tropo can be considered "radio mirages". Signals that are
normally below the radio horizon and out-of-range instead appear above
the radio horizon and receivable. (Note that due to the difference in
wavelengths, the radio horizon is farther away than the visual horizon).
A description of the tropo modes follows:
1) LINE-OF-SIGHT (GW)
- Also known as Groundwave. Normal continuous reception where the
receiving and transmitting antennas can see each other, taking into
account the 4/3 Earth curvature of radio waves. Figure 1 illustrates
normal conditions where the receiver is out-of-range. The illustration
2) TROPOSPHERIC SCATTER (TrS)
- An almost ever-present condition that brings in distant fluttery
signals beyond normal line-of-sight. Scattering of the signals occurs in
contact with discontinuities in the troposphere. These discontinuities
can be small temperature or humidity variations, such as can be found
around cloud layers, individual clouds, updrafts, downdrafts, the
tropopause (the boundary between the troposphere and the stratosphere), small particles and droplets
such as drizzle, mist, haze, dust, smoke, volcanic ash, etc., or even flocks of birds and large swarms of insects.
3) TROPOSPHERIC SUPER-REFRACTION (TrE)
- Also known as Tropospheric Enhancement or Tropospheric Bending.
Super-refraction occurs when the lower troposphere becomes stratified
into two stable layers. A warm dry layer over a cool moist layer (with
warm and cool
being relative terms). The boundary between these two layers is called
an inversion. Normally in the lower troposphere, temperatures decrease
with height and humidity increases with height
- thus why they are called inversions. Signals bend as they cross the
inversion. When they start bending downwards, the signals can travel
farther, reaching places that are normally beyond the radio horizon and
out-of-range. The effective bending is now less than 4/3 Earth
radius, but still more than 1 Earth radius. The base of the inversion
is considered to be the ground. The top of the inversion is the airmass
boundary. The thickness of the inversion can roughly determine the
lowest usable (affected) frequency (LUF). Figure 2 illustrates
4) TROPOSPHERIC DUCTING (TrD)
- Ducting occurs when the super-refractive bending becomes so much that
the signal hits the ground at a distance far away from the
transmitter - and is then reflected back up to the inversion, to then be
refracted back down again. In essence, the signals become trapped in a
"trapping layer" or duct. The effective bending is now less than 1 Earth radius. The
base of the duct is the ground. The top of
the duct is the inversion. Signals do weaken when reflecting off the
ground. Signals that reflect off of a water surface instead (ocean/lake)
retain much more strength. One side-effect of ducting is reduced range
for aircraft flying above the inversion. Most ducting occurs below 3000 m
(10,000'). Above that level, the air starts to get too sparse in
density for inversions to be strong enough. Figure 3 illustrates
5) ELEVATED TROPOSPHERIC DUCTING - In
cases where the top of the inversion is very high above the ground, it
may become possible for the low level moisture to rise and pool beneath
the inversion top. In these cases, 3 different airmass layers can form -
with the surface layer being somewhat warmer and drier than the cool
moist air higher up. This results in a duct that is elevated above the
ground. Although the signals are being carried far from the transmitter,
receivers at low elevation will not be able to receive them. Only tall
masts or locations on high hills that "poke" into the duct will be able
to receive the signals. Often this is the case with the transmitter as
well, as tall masts or locations on high hills poking into the duct get
direct access to it. Although the bulk of the trapped signals stay
within the duct, they may occasionally escape allowing for random and
spotty reception beneath the duct. Often, long ducts may consist of
portions that are surface-based and portions that are elevated. Figure 4
|Main Types of Tropo, according to Meteorology
1) RADIATION TROPO
- Also known as Radiative Cooling Tropo or Nocturnal Tropo. A common
nocturnal event that often occurs during clear, calm nights
on land. Radiative cooling results in cooler
more humid conditions near the surface which forms a shallow inversion.
inversion usually "burns off" shortly after sunrise. Due to its shallow
nature, Radiation Tropo often follows the topography of the land.
2) HIGH-PRESSURE TROPO
- Also known as Subsidence Tropo. Sinking air (subsidence) in a
high-pressure system warms and dries as it descends. Often cool moist
air can become trapped underneath forming an inversion. High-Pressure
tropo can last all day. Often, Radiation Tropo occurs simultaneously at
night, blocking more distant signals from High-Pressure Tropo. As a
result, conditions can often be better during the day.
3) FRONTAL TROPO
- Frontal inversions can be found in the area ahead of an approaching
warm front, behind a departing cold front, or north of a
quasi-stationary front. Inclement weather often accompanies fronts and
may hinder duct formation. Due to the fast motion of cold fronts,
ducting events are often short-lived.
4) DOWNSLOPE TROPO
- Also known as Chinook Tropo, Santa Ana Tropo, Fœhn Tropo, Bora Tropo,
Zonda Tropo, etc. Downslope Tropo is caused by air descending down a
mountainside that warms and dries as it descends. If the pre-existing
airmass is cool enough, it may become trapped under an inversion.
6) VALLEY TROPO
- Warm dry air can override cooler moist air trapped in a valley under
the resulting inversion. This is different from topography-conforming
Radiation Tropo in that the inversion can persist all day long, long
after any radiative effects have dissipated.
7) MARINE TROPO
- Also known as Maritime Tropo, Oceanic Tropo or Lake-Effect Tropo.
Marine Tropo occurs when warm dry air overrides a cooler body of water.
Marine inversions often extend the entire breadth of lakes and can
extend for thousands of miles over the ocean. It also spreads into coastal areas by way of sea or lake breezes. Marine tropo can become
enhanced or combined with other types such as High-Pressure Tropo. It
normally peaks during the afternoon when the inversion is the strongest.
Outside of the equatorial zone, spring and early summer is the best season.
|Exotic Tropospheric DX Modes
Here are some other tropospheric modes that are more rare and exotic :
1) RAIN SCATTER (RS)
- Rain scatter mainly occurs in the higher UHF and microwave bands. A
band of very heavy rain at a distance can scatter or even reflect
signals. The effect is the one used for Meteorological Radars. (Note
that snow is not an useful reflector). Signals may appear to
arrive from the wrong direction - that of the rain band rather than the
2) HAIL SCATTER (HS) - Similar to Rain Scatter but caused by Hail.
3) ICE PELLET SCATTER (SS)
- Known as Sleet Scatter in the USA. Similar to Rain Scatter but caused by Ice Pellets.
5) AIRCRAFT SCATTER (AS)
- Caused by reflections off of aircraft. Aircraft scatter is more common within 10 miles of an active airport.
Reflections off of hills, mountains, buildings and Knife-Edge Diffraction by itself are not considered true DX modes since they are omni-present. However, when present in combination with tropo they can help to extend signal range even further.
There are also conditions in the ionosphere that produce distant
reception via a whole different set of modes (mainly affecting frequencies below ~ 120 MHz). Ionospheric "Skip" and
Scatter are not caused by the weather, but instead by the interaction
between the Sun and the Earth's outer atmosphere, or by objects such as
meteors (and possibly thunderstorm sprites). For more information on
these modes, consult Wikipedia's article on VHF-UHF Propagation.
©2019 William R. Hepburn