, Puerto Rico's highest peak, and its TV transmission towers To broadcast its programs, a television station requires
operators to operate equipment, a transmitter or
radio antenna, which is often located at the highest point available in the transmission area, such as on a
summit, the top of a high
skyscraper, or on a tall
radio tower. To get a signal from the
master control room to the transmitter, a
studio/transmitter link (STL) is used. The link can be either by radio or
T1/
E1. A
transmitter/studio link (TSL) may also send
telemetry back to the station, but this may be
embedded in
subcarriers of the main broadcast. Stations which retransmit or simulcast another may simply pick-up that station
over-the-air, or via STL or satellite. The license usually specifies which other station it is allowed to carry.
VHF stations often have very tall antennas due to their long
wavelength, but require much less
effective radiated power (ERP), and therefore use much less
transmitter power output, also saving on the
electricity bill and emergency
backup generators. In
North America, full-power stations on
band I (channels 2 to 6) are generally limited to 100 kW analog video (
VSB) and 10 kW analog audio (
FM), or 45 kW digital (
8VSB) ERP. Stations on
band III (channels 7 to 13) can go up by 5
dB to 316 kW video, 31.6 kW audio, or 160 kW digital. Low-VHF stations are often subject to
long-distance reception just as with FM. There are no stations on
Channel 1.
UHF, by comparison, has a much shorter wavelength, and thus requires a shorter antenna, but also higher power. North American stations can go up to 5000 kW ERP for video and 500 kW audio, or 1000 kW digital. Low channels travel further than high ones at the same power, but UHF does not suffer from as much
electromagnetic interference and background "noise" as VHF, making it much more desirable for TV. Despite this, in the U.S., the
Federal Communications Commission (FCC) is taking another large portion of this band (channels 52 to 69) away, in contrast to the rest of the world, which has been taking VHF instead. This means that some stations left on
VHF are harder to receive after the
analog shutdown. Since at least 1974, there are no stations on
channel 37 in North America for
radio astronomy purposes. ==Program production==