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24<br />

Special DigitalLife<br />

INFODIGITAL December 2008<br />

A<br />

small satellite key and a suitable<br />

receiver is all you need to<br />

access hundreds of programmes<br />

<strong>in</strong> your home. The location of ASTRA<br />

19.2° East alone offers a colourful<br />

and <strong>in</strong>ternational selection of several<br />

hundred digital free-to-view satellite<br />

programmes from all over <strong>the</strong> world.<br />

Moreover, several fur<strong>the</strong>r hundred pay-<br />

<strong>Sat</strong> <strong>in</strong> <strong>the</strong> City<br />

DigiDish 33: Really large<br />

selection from small<br />

satellite antennas<br />

per-view encoded channels are also<br />

available. The parabolic antenna necessary<br />

for access<strong>in</strong>g <strong>the</strong> same is also considerably<br />

smaller than those required<br />

for analogue transmissions:<br />

This is how small <strong>the</strong> DigiDish 33 is.<br />

The digital satellites, namely <strong>in</strong> comparison<br />

to <strong>the</strong>ir analogue peers, boast a<br />

considerably higher output power.<br />

The best example of this is <strong>the</strong> Techni<strong>Sat</strong><br />

DigiDish 33. The m<strong>in</strong>i antenna,<br />

which has a diameter of barely 33 cm,<br />

appears dim<strong>in</strong>utive to <strong>the</strong> eye. However,<br />

its performance is anyth<strong>in</strong>g but.<br />

Receiv<strong>in</strong>g what previously required a<br />

parabolic antenna 65cm <strong>in</strong> diameter<br />

is no major problem for <strong>the</strong> newer<br />

and smaller version.<br />

Pr<strong>in</strong>ciple beh<strong>in</strong>d receiv<strong>in</strong>g<br />

satellite signals<br />

To receive <strong>in</strong>cidental television signals,<br />

which are transmitted via satellite, on<br />

<strong>the</strong> one hand we have <strong>the</strong> concave<br />

antenna and on <strong>the</strong> o<strong>the</strong>r, <strong>the</strong> aforementioned<br />

(round) LNB, <strong>in</strong> which frequencies,<br />

thanks to <strong>the</strong> way <strong>the</strong> curve<br />

is constructed almost as <strong>in</strong> a burn<strong>in</strong>g<br />

glass. When learn<strong>in</strong>g physics (optics)<br />

<strong>in</strong> school, we all doubtless vaguely remember,<br />

that <strong>the</strong> angle of <strong>in</strong>cidence is<br />

also <strong>the</strong> angle of reflection. The same<br />

ratio applies to <strong>the</strong> <strong>in</strong>cident signals:<br />

each satellite has a specific position<br />

<strong>in</strong> <strong>the</strong> orbit and thus transmits its relevant<br />

“Footpr<strong>in</strong>t” onto <strong>the</strong> correspond<strong>in</strong>gly<br />

positioned antenna. S<strong>in</strong>ce <strong>the</strong><br />

myriad range of satellites around <strong>the</strong><br />

world each have different orbit positions,<br />

<strong>the</strong>ir signal angles also vary and<br />

can consequently not all be picked up

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