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What does the science say? - Brigham Young University

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Notes on Right-­‐Hand Figure<br />

Antenna sky temperature. Noise temperature of an idealized<br />

antenna (lossless, no Earth-­‐directed sidelobes) located at <strong>the</strong><br />

Earth’s surface, as a func0on of frequency, for a number of beam<br />

eleva0on angles. Solid curves are for geometric-­‐mean galac0c<br />

temperature, sun noise 10 0mes quiet level, sun in unity-­‐gain<br />

sidelobe, cool temperate-­‐zone troposphere, 2.7K cosmic blackbody<br />

radia0on, zero ground noise. The upper dashed curve is for<br />

maximum galac0c noise (center of galaxy, narrow-­‐beam antenna).<br />

Sun noise 100 0mes quiet level, zero eleva0on, o<strong>the</strong>r factors <strong>the</strong><br />

same as solid curves. The lower dashed curve is for minimum<br />

galac0c noise, zero sun noise, 90â—¦ eleva0on angle. (The bump in<br />

<strong>the</strong> curves at about 500MHz is due to <strong>the</strong> sun-­‐noise characteris0c.<br />

The curves for low eleva0on angles lie below those for high angles<br />

at frequencies below 400MHz because of reduc0on of galac0c<br />

noise by atmospheric absorp0on. The maxima at 22.2 and 60 GHz<br />

are due to <strong>the</strong> water-­‐vapor and oxygen absorp0on resonance.)<br />

11

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