VHF UHF Propagation

From HFUnderground

Revision as of 12:02, 16 June 2022 by ChrisSmolinski (Talk | contribs)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to: navigation, search

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



This site is a participant in the Amazon Services LLC Associates Program, an affiliate advertising program designed to provide a means for sites to earn advertising fees by advertising and linking to Amazon.com. Some links may be affiliate links. We may get paid if you buy something or take an action after clicking one of these.