VHF UHF Propagation
From HFUnderground
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Revision as of 12:30, 16 June 2022
Contents |
Aurora
Ionospheric F2
The same mode of propagation as often occurs on HF. As intense ionization of the ionosphere's F2 layer is necessary, this mode only occurs during peak solar conditions around the maximum of the solar cycle, if at all, and only affects VHF Lo band up to perhaps the 6m band.
Ionospheric scattering
Meteor Scatter
Sporadic E
Trans-equatorial (TEP)
Tropospheric Ducting
Tropospheric scatter
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