Ian Roberts ZS6BTE
By using the ionisation following lightning
flash, it is possible for communications through VHF into the microwave
frequencies to take place over similar distances available from Sporadic E
propagation or meteor scatter (700-800 km or more). This is possible due to the
height attained by lightning discharges and their associated ionisation effects, red sprites and blue jets.
"Lightning scattering has sometimes been
observed on VHF and UHF over distances of about 500 km. The hot lightning
channel scatters radio-waves for a fraction of a second. The RF noise burst
from the lightning makes the initial part of the open channel unusable and the
ionization disappears quickly because of recombination at low altitude and high
atmospheric pressure. Although the hot lightning channel is briefly observable
with microwave radar, no practical use for this mode has been found in
communications." https://en.wikipedia.org/wiki/Radio_propagation#Lightning_scattering
This statement is in direct conflict with my
observations made over several years using UHF TV transmitters as beacons
received at distances exceeding 550 km.
From another source providing some technical
information:
"A typical cloud to ground lightning
flash culminates in the formation of an electrically conducting plasma channel
through the air in excess of 5 kilometres
(3.1 mi) tall, from within the cloud to the ground's surface. The actual
discharge is the final stage of a very complex process. At its peak, a typical thunderstorm
produces three or more strikes to
the Earth per minute. Lightning primarily occurs when warm air is mixed with
colder air masses, resulting in atmospheric disturbances necessary for
polarizing the atmosphere."
"In general, cloud-to-ground
(CG) lightning flashes account for only 25% of all total lightning flashes
worldwide."
Fig 1: Global map of lightning activity
Fig 2: Zoomed view - parts of
https://en.wikipedia.org/wiki/Lightning
It follows that 75% of
lightning discharges are of the cloud-to-cloud (CC) or in-cloud (IC) variety.
The lightning flash forms a
highly electrically conductive plasma channel. The core temperature of the
plasma during the flash may exceed 50,000 K, causing it to brilliantly radiate
with a blue-white color. Once the electric current stops flowing, the channel
cools and dissipates over tens or hundreds of milliseconds, often disappearing
as fragmented patches of glowing gas. The nearly instantaneous heating during
the flash causes the air to explosively expand, producing a powerful shock wave
heard as thunder. This travels at about 1.6km per 5 seconds. The average
duration of a stroke of lightning is about 30 microseconds. An average
thunderstorm is up to 16 km wide and travels at 40 km/h.
Lightning produces both X-ray
and gamma ray radiation - the mechanism is not fully understood. This
undoubtedly contributes to the development of the highly ionised plasma cone
around and in the atmosphere above the discharge path, which is so effective in
reflecting radio waves.
Sprites are massive but weak
luminous flashes that appear directly above an active thunderstorm. They occur
at the same time as CG or IC lightning discharges. Sprites can extend to
altitudes of about 95 km and are most often red. The sprites are rarely seen
singly. They usually occur in clusters of two or more. The colour
indicates ionisation at the location of the sprite.
Fig 3: Red sprites
http://sprite.gi.alaska.edu/html/sprites.htm
Blue Jets
Blue jets appear above
thunderstorms. They are narrow cones which are ejected from the electrically active
core regions of a thunderstorm and also indicate ionisation
at the location. Blue jets are typically emitted at speeds of approximately 100
km/s (Mach 300). They then fan out and disappear at altitudes
of 40-50 km.
Fig 4: A Blue Jet
http://umbra.nascom.nasa.gov/spd/images/Blue_Jet_FULL.GIF
Lightning Flash as a Propagation Mechanism
Since lightning flash ionisation around a thunderhead may commonly reach
altitudes of 20000m (20km or over 60000
ft), it is obvious that distance enhancement will be available in a
point-to-point VHF or UHF communications link. This distance is enhanced
further due to the altitude of up to 90-odd km reached by the sprite and jet
zones mentioned above.
But what is the nature of the
available ionisation and why is it usable?
Using a rotatable
high gain UHF antenna system with preamp pointing to Aliwal
North TV (distance about 550 km) and a UHF receiver in USB mode, the trace in
Fig 5 was obtained. The trace shows much spread and amplitude enhancement over
the tropospheric scatter path due to the very favourable weather conditions
prevailing, amounting to some 30 dB. Additionally lightning bursts ride on this
signal level producing pulse waveforms lasting typically 0.1 to 0.6 seconds and
providing another 20 to 30 dB of signal recovery on top of the already
available 30 dB on the enhanced tropospheric scatter path. These pulses display
as the horizontal streaks across the TV carrier frequency and from the timer an
average of 15 major discharges per minute can be counted. Many lesser
discharges, possibly two to three times as many, could be heard during the one
minute interval.
Each lightning burst lasts
about 30 microseconds and during that period the electromagnetic pulse effect (EMP)
completely disables any chance of communication due to the overpowering RF noise
accumulation.
But the ionised zone still exists
after this and readily reflects high radio frequencies over the remainder of
the 0.1 to 0.6 seconds of the ionised effect.
The audio impression when
listening is a sharp click from the discharge's EMP, followed by a
Doppler-shifted zinging audio tone or tones, very reminiscent of a meteor
scatter echo and possessing the same rise and fall wave shape, Fig 6b.
From this it follows that
lighting flash is not suitable for slow communication such as voice, but the
ionised zones last more than long enough to communicate using fast data modes
such as FSK441 and JTMS offered in the WSJT suite of PC soundcard-based
programs.
Path Prediction
Predicting a path is simply a
matter of examining weather maps (Fig7) for the most likely thunder cloud
formations and directions and the near real time lightning discharge map in Fig
8, and aiming the antenna in that direction. Note the correlation between the
thunder clouds in Fig 7 and the actual discharges in Fig 8.
The longest distance will be
obtained when the partner station is on the other side of the thundercloud
formation, total distance 700 to 800 km looks very feasible, while more nearby
stations may be worked on lightning flash backscatter when both stations point
to the same thundercloud.
Fig 5: Waterfall recording of an active 791
MHz UHF propagation path over 550 km. The horizontal pulses superimposed on the
carrier are lightning discharges
Fig 6a: Amplitude versus 1 minute Time
response of the UHF path
Fig 6b: Zoomed view of a major pulse
Fig 7: Eumetsat
real light image of the path discussed (approximately along the red line)
http://oiswww.eumetsat.org/IPPS/html/MSG/RGB/NATURALCOLOR/SOUTHERNAFRICA/index.htm
Fig 8: Map indicating the active
lightning strike zones
http://webflash.ess.washington.edu/EurAfricaL_plot_weather_map.jpg