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SUN NOISE and Measurements - VK3UM

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LNA<br />

Located<br />

at feed<br />

METHOD # 3<br />

Pass b<strong>and</strong> Filter<br />

(IDF)<br />

B<strong>and</strong>width<br />

commensurate<br />

with frequency of<br />

measurement.<br />

AF Power Meter<br />

VK1OD<br />

Measurement<br />

Software<br />

(sound card)<br />

Shack LNA<br />

Amplifier<br />

HF Receiver<br />

SSB or AM<br />

Down<br />

Converter<br />

Precision<br />

Stepped<br />

Attenuator<br />

Use of a Down Converter HF Receiver <strong>and</strong> AF Power Meter<br />

This example approaches what would be to expected in most ‘advanced VHF/UHF<br />

Amateur installations <strong>and</strong> will provide excellent <strong>and</strong> reproducible results.<br />

• Turn the Receiver AGC off <strong>and</strong> reduce the RF Gain to a satisfactorily level<br />

where overload will not occur with the system gain.<br />

• Point the Antennae at the cold noise source.<br />

• Set the precision attenuator to a value such that you may add additional<br />

attenuation as expected by the increase of Sun noise.<br />

• Calibrate the AF power meter or record the value with the VK1OD Software 7 .<br />

• Point antennae at the Sun.<br />

• Increase the attenuation to obtain the calibrate level as set earlier.<br />

• the amount of added attenuation is the Y-Factor<br />

Doug McArthur <strong>VK3UM</strong> Page 16 GippsTech 2008

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