Trans-Equatorial
Propagation (TEP) is a phenomenon in radio wave propagation that occurs between
two regions located on opposite sides of the Earth's equator. It involves the
propagation of radio waves from one hemisphere to the other by utilizing the
Earth's ionosphere, particularly the F2 layer.
Here's how TEP works:
1. Ionospheric
Reflection: Radio waves transmitted from one region
travel upward into the ionosphere, where they encounter the F2 layer. The F2
layer is the highest layer of the ionosphere, located at an altitude of
approximately 200 to 600 kilometers (124 to 373 miles) above the Earth's
surface.
2. Refraction
and Reflection: When radio waves encounter the F2 layer, they
can undergo refraction and reflection. Refraction occurs when radio waves bend
as they pass through the ionosphere, while reflection occurs when radio waves
are reflected back toward the Earth's surface by the ionosphere.
3. Equatorial
Crossing: In TEP, radio waves that are reflected or
refracted by the F2 layer can cross the equator and propagate into the opposite
hemisphere. This crossing typically occurs near the magnetic equator, where the
Earth's magnetic field lines are nearly horizontal and facilitate the
propagation of radio waves between hemispheres.
4. Reception: Once the radio waves have crossed the equator, they continue to
propagate in the opposite hemisphere and can be received by radio operators
located in that region. This allows for long-distance communication between
stations located in different hemispheres, often spanning thousands of
kilometers.
Trans-Equatorial Propagation
(TEP) is most commonly observed on the 10-meter
amateur radio band (28 MHz) and is favored by high solar activity and
geomagnetic disturbances, which enhance ionospheric conditions. While TEP can
provide exciting opportunities for long-distance communication, it is also
subject to variations in ionospheric conditions and is not always predictable.
Amateur radio operators often monitor the 10-meter band for TEP openings,
particularly during periods of enhanced solar activity, to take advantage of
this unique propagation mode.
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