Monday, 24 February 2014
UK satellite reception in Europe: why do I lose my signal in the evening?
Over
the past few weeks, since the migration of BBC TV and radio services to
new satellite Astra 2E, there have been reports from viewers in Europe
around the edge of the UK spotbeam saying that they lose access to BBC
(and other) channels in the evenings.
This has prompted a number of conspiracy theories, such as that the
power of the satellite beam is being deliberately reduced during
primetime TV or that the satellite isn't working properly.
So what's the cause of the daily "wobble", which results in viewers
around the edge of the spotbeam - notably across Germany, the Alps,
northern Italy, southern France and parts of Spain, to lose channels in
the evening?
To understand the problem, we need to look at the sharp drop-off around the edge of the UK spotbeam.
The main UK free-to-air broadcasters required a better satellite set-up
to combat issues regarding broadcast rights, royalties and copyright
matters.
So a sharper spotbeam for the UK was created. Reception from the new
spotbeam rapidly drops off around the edge, meaning that within 100
miles (160km), dish sizes can go from 80cm to 130cm or more. It's in
these zones that the daily variations are most noticeable. The slightest
change in circumstances or transmitting parameters, which would
otherwise not matter, has the power to knock out reception.
Some internet users have concluded that the Astra 2E satellite must move
around every day as an explanation of the daily cycles. Although
satellites can move around a bit at their orbital position, modern
satellites will keep to their orbital position with minimum variation.
The slightest movement could affect reception on the ground around the
edges of the spotbeam, but for the some of the main reasons behind the
daily cycle, we have to look elsewhere:
Thermal distortion on the part of the satellite's antennas itself can
impact on reception. This is a natural effect, but could be exaggerated
by the very sharp drop off around the edge spotbeam.
Second, there is the theory that the position of the sun with regards
the satellite is a factor. Viewers have reported losing channels at the
time of the evening. That's when the sun is directly opposite the Astra
2E satellite in the sky
*, shining straight at the satellite. The
bright sunlight is not the main factor here, though. Instead, the sun's
radiation and the effects of the ionosphere are an issue.
Both issues aren't normally a factor for domestic satellite TV
reception. But for viewers living around the edge of the spotbeam, they
can be part of the reason why reception disappears in the evening.
Reception of services broadcast via the pan-Europe beam goes unaffected,
simply because the signal is much stronger.
A bigger dish, quality LNB and cables can help overcome daily cycle
variations. Also, because Astra 2E is slightly to the east of the other
Astra 2 satellites, a slight tweak to the dish may also help sustain a
reliable signal for longer. For some viewers, the signal is only lost in
the evenings when the weather is bad and thick cloud reduces the
already weaker evening signal.
Viewers who don't live in the UK, Ireland, northern France, Belgium or
the Netherlands must note that the signals on the Astra 2E/F spotbeams
are not intended for their reception, and any out-of-area reception is a
bonus.
*Astra 2E orbits above the equator at around 28.35 degrees East
longitude. When the sun is over 151.65 degrees West it is opposite Astra
2E in the sky. Astra 2E, as all geostationary satellites, is located
nearly 36,000 km above the earth - far enough away so as not to be in
the earth's shadow at that particular time. From Astra 2E's perspective,
in the late evening (GMT), the sun is shining straight over the earth
and straight "in its face", or straight at its transmitting and
receiving equipment. Note that it's not the bright light, but rather the
sun's energy that causes issues for satellites, and that any resulting
detrimental effect on reception is outside of its intended coverage
area.
On earth, we have similar issues when the sun gets in the way. From late
February into March and again around early October, there are numerous
issues with "
sun outages",
when the sun is directly behind the satellite we are receiving a signal
from. TV satellites transmit with enough power in order for viewers in
the main footprint (or spotbeam) area to continue viewing, but around
the edges of the footprint (or spotbeam), reception can be affected.
In the analogue era, viewers saw an increase in "sparklies"; comet
shaped marks on the picture, as a result of sun interference. In the
digital era, blocking or loss of signal can occur.
The time such interference is likely to occur and its duration depends
on your location, which satellite you are receiving from, and the size
of your dish. The bigger the dish, the shorter the interference time,
and the fewer days of interference you have. In the UK, interference
from the sun could be a issue for some Sky and Freesat viewers during
the next 14 days, for a few minutes after 10am each morning. Internet
sun outage calculators can be found via Google.
BRITISH TV
BLACKOUT IN EUROPE
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