Bird Technologies 5012 User Manual

INSTRUCTION SHEET
WIDEBAND POWER SENSOR
MODEL 5012
©Copyright 2008 by Bird Electronic Corporation
Instruction Book P/N 920-5012 Rev. C
Description
The Bird 5012 Wideband Power Sensor (WPS) is a Thruline sensor that can measure average, peak, or burst power, VSWR, crest factor, and Complementary Cumulative Distribution Function (CCDF). It can be used with the Bird 5000-EX Digital Power Meter (DPM) and the Bird Virtual Power Meter Software (VPM).
NOTE: Firmware upgrades extending the WPS’s capabilities may
be periodically released. For the latest firmware upgrade, contact Bird Customer Service at (440) 248-1200 or visit our website at
http://www.bird-electronic.com
Connections
WARNING
Never attempt to connect or disconnect RF equipment from the
transmission line while RF power is being applied.
Leaking RF energy is a potential health hazard.
To connect the WPS to the Digital Power Meter, use the serial cable provided. Connect the male end of the cable to the DPM and the female end to the WPS. A separate power supply for the WPS is not required when using a DPM.
There are two ways to connect the WPS to a PC running the Virtual Power Meter Software:
y To connect using the serial port, first connect a 12V DC power
supply to the WPS. Once the STATUS LED turns on and begins blinking, use the serial cable provided and connect the female end of the cable to the computer and the male end to the WPS. The WPS must be powered up before connecting to the PC.
y To connect using the USB port, connect the USB cable to the
computer and to the WPS. A separate power supply is not required when using the USB port.
NOTE: When using the optional serial to USB adapter, connect
the WPS serial port to the adapter’s serial port, and the adapter’s USB connector to the PC.
Zeroing Sensor
Average Power
Peak Envelope Power
0 W
50 W
100 W
Over time, the sensor’s “zero value” (reading with no applied RF power) can drift, making all readings inaccurate by this value. For example, if the zero value is –0.02 W, measuring a 50 W signal will give a reading of 49.98 W, a 0.04% error. Measuring a 1 W signal will give a reading of 0.98 W, a 2% error. If the drift would be a significant error, rezero the sensor:
y Make sure the sensor has reached a stable operating temperature.
y Make sure no RF power is applied to the sensor.
y Press “Zero”. Calibration will begin.
y Calibration will take about 30 seconds. Do not interrupt the
calibration! A bar on the screen will display calibration progress.
y After successful calibration, “Cal Pass” or “Calibration Complete”
will be displayed. Press any key to return to normal operation.
y If calibration fails, “Cal Fail” will be displayed. Press a key to
return to normal operation, then check that the WPS is properly connected, and that the RF is off. Rezero.
Function Descriptions
Figure 1
Average and Peak
Envelope Power
Square Wave Signal
Average Power
Average power is a measure of the equivalent “heating” power of a signal, as measured with a calorimeter. It measures the total RF power in the system, and does not depend on number of carriers or modulation scheme. The WPS is a broadband sensor that measures power across its entire frequency range. Its diodes operate in their ‘square law’ region so that the detector output is directly proportional to the average power, without any additional error correction.
Average power is the most important measurement of any transmission system since the average power is normally specified on the operating license. It is also valuable as a maintenance tool, showing overall system health, and for calibration.
VSWR
Rho (µ) = PRP
F
Filter
Too Small
Filter
Too Wide
Correct
Filter
Noise
Signal
VSWR measures the relation between forward and reflected average power. The Bird Wideband Power Sensor calculates the VSWR from the Forward and Reflected Average Power measurements. Rho and Return Loss are also the same measurement, but in different units:
, , and
The health of the feedline and antenna systems can be monitored using VSWR measurement under full power operating conditions. High VSWR is an indicator of feed line damage, overtightened cable or feed line clamps, or antenna changes/damage due to weather conditions, icing, or structural damage to the tower.
Video Filter
Figure 2
Video Filter Settings,
300 kHz Signal
Except for average power and VSWR measurements, all WPS measurements rely on a variable video filter to improve accuracy. This filter can be set to either 4.5 kHz, 400 kHz, or full bandwidth. It should be as narrow as possible while still being larger than the demodulated signal bandwidth (video bandwidth). Narrowing the filter limits the noise contribution caused by interfering signals. Listed below are some common modulation schemes and the appropriate video filter.
Video Filter Modulation Type
4.5 kHz CW Burst (Burst width > 150 µs), Voice Band AM,
400 kHz CW Burst (b.w. > 3 µs), GSM, 50 kHz AM, DQPSK
Full Bandwidth
FM, Phase Modulation, Tetra
CW Burst (b.w. > 200 ns), CDMA, WCDMA, DQPSK, DAB/DVB-T
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