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SUN NOISE and Measurements - VK3UM

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LNA<br />

Located<br />

right at feed<br />

METHOD # 4<br />

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

(IDF)<br />

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

commensurate<br />

with frequency of<br />

measurement.<br />

S Meter<br />

Shack LNA<br />

Amplifier<br />

HF Receiver<br />

SSB or AM<br />

Down<br />

Converter<br />

Use of a Down Converter <strong>and</strong> HF Receiver with S Meter<br />

This example is considered to be ‘not ideal’ It will however, with care, it can provide<br />

satisfactory results.<br />

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

• Adjust the RF Gain to a known S meter point (e.g. S1).<br />

• Point antennae at the Sun.<br />

• Read the increase in the S meter<br />

• the increase of the S Meter in dB is the Y-Factor<br />

This accuracy of this method is determined by the receivers’ linearity <strong>and</strong> the<br />

exact value of S meter units. It is advisable to check the linearity of the S Meter<br />

with a calibrated signal generator.<br />

Doug McArthur <strong>VK3UM</strong> Page 17 GippsTech 2008

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