HF Signal Propagation Bill Leonard N0CU 1 June 2019

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Presentation transcript:

HF Signal Propagation Bill Leonard N0CU 1 June 2019

Primary Modes of HF Wave Propagation Direct (line of sight) wave Ground (surface) wave Beyond line of sight Maximum range ~40 mi Vertical polarization only Sky wave (via ionosphere) D2 D1

Primary Modes of HF Wave Propagation Direct (line of sight) wave Maximum range 10-20 mi Ground (surface) wave Beyond line of sight Maximum range ~40 mi Vertical polarization only Sky wave (via ionosphere)

Secondary Modes of Wave Propagation Ionospheric modes Meteor scattering Auroral backscatter Sporadic-E propagation Tropospheric modes Tropospheric ducting Up to 1000 mi Frequencies >40 MHz Tropospheric scattering Rain scattering Airplane scattering Lightning scattering

Why Are Ground Waves Vertically Polarized? Polarization of a linear EM wave is defined by the E field Horizontally polarized wave has the E field in contact with the Earth A conductive surface will act like a short to an E field Ex: Dipole antenna laying on highly conductive ground plane Magnetic fields are unaffected by conductive materials Magnetic fields are affected by ferromagnetic materials Ex: Magnetic loop antenna near ground V + - Earth Ground Vertically polarized wave Short has no effect on magnetic field Earth Ground

Groundwave Propagation Beyond Horizon Vertically polarized linear EM wave Conductive Surface (Earth) Image antenna wave Image antenna Earth is a lossy dielectric Resistance: loss causes signal attenuation Capacitance: slows down wave travel near the Earth Causes wave to bend and follow the curvature of the Earth

Polarization Of A Reflected Wave You are receiving a European DX station on 14 MHz via the North Pole. He is using a horizontally polarized antenna. Question: What is the polarization of the signal at your antenna Horizontal Vertical Can’t tell because of Faraday rotation None of the above

Polarization Of A Reflected Wave You are receiving a European DX station on 14 MHz via the North Pole. He is using a horizontally polarized antenna. Question: What is the polarization of the signal at your antenna Horizontal Vertical Can’t tell because of Faraday rotation None of the above Answer: None of the above Why: All ionospherically refracted (reflected) signals are elliptically polarized

Wave Polarization Linear Circular        300 × 201        300 × 201 Wave Polarization Linear Horizontal vs Vertical polarization Cross pol => no signal Circular E & H fields both rotate 360 deg per wavelength of travel Left vs right polarization Linear Rx with circular Tx (and vice versa) Loss = -3 dB regardless of orientation of antennas How to generate a circularly polarized signal? Helix antenna Crossed dipoles RHCP

Ions and Plasmas An ion is an atom that has had one or more electrons stripped away A plasma is an ionized gas consisting of approximately equal numbers of positively charged ions and negatively charged electrons The free electrons in the plasma in the ionosphere are what causes refraction of radio waves - +

Why Are All Ionospherically Refracted Signals Elliptically Polarized? The ionosphere is a magnetized plasma (ionized gas) Magnetized plasmas are birefringent A “Birefringent” medium is a medium with two refractive indices A linearly polarized EM wave passing thru a magnetized plasma splits into two separate, counter rotating circularly polarized waves: Ordinary (O-mode) wave Extraordinary (X-mode) wave The O-mode wave follows the magnetic field lines Propagation path is close to what would occur in a non-magnetized plasma The X-mode wave goes perpendicular to the magnetic field lines Higher path loss More susceptible to ducting (can go farther than the O-mode)

Divergence of O and X Mode Waves Ionosphere O-wave X-wave

Forward O Mode Waves Ionosphere O-wave X-wave

Reverse O Mode Waves Ionosphere O-wave X-wave X-wave O-wave

Forward X Mode Waves Ionosphere O-wave X-wave

Reverse X Mode Waves Ionosphere O-wave X-wave X-wave O-wave

Why Is Birefringence Important? Ionosphere is no longer reciprocal One way propagation is the norm The two paths for a QSO are different X and O waves: May, or may not have equal powers Can take radically different paths exiting the ionosphere Beam headings may not follow Great Circle routes Up to 90 deg different at the poles Have different MUFs, skip distances, propagation velocities, & attenuation Degree of divergence of X and O waves: Varies with location, frequency, take off angle, state of the ionosphere,… Worst at low frequencies and at the Poles Least along the Magnetic Equator Most propagation programs only deal with O-mode Proplab Pro Ver 3 shows both

Reflection vs Refraction The ionosphere is a refractive surface (not a reflective surface) Why this is important => ?