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SUN NOISE and Measurements - VK3UM

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LNA<br />

Located<br />

Located<br />

at Feed<br />

at Feed<br />

METHOD # 1<br />

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

(IDF)<br />

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

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

commensurate<br />

commensurate<br />

with frequency of<br />

with frequency of<br />

measurement.<br />

measurement.<br />

Amplifier<br />

Use of a Spectrum Analyser<br />

Sufficient<br />

Sufficient<br />

combined gain to<br />

combined gain to<br />

drive Spectrum<br />

drive Spectrum<br />

Analyser<br />

Analyser<br />

Spectrum analyser<br />

This example demonstrates what would be the ‘ideal’ measuring setup. Not all shacks<br />

are fortunate to include a Spectrum Analyser!<br />

• Point the Antennae at the cold source <strong>and</strong> adjust the amplifier/ input attenuator<br />

on the Spectrum analyser to form a calibrate level. Ensure that there are not<br />

adjacent high level signals (off measuring frequency) that could impact on<br />

measurement.<br />

• Point antennae at the Sun <strong>and</strong> the difference in level is the Y-Factor. The<br />

measurement should be taken at the widest b<strong>and</strong>width commensurate to the<br />

LNA b<strong>and</strong>width <strong>and</strong> filter used.<br />

Doug McArthur <strong>VK3UM</strong> Page 14 GippsTech 2008

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