| | Noise Contribution Analysis for the Arecibo Gregorian Radio Telescope (Site not responding. Last check: 2007-10-20) |
 | | In a radio telescope, minimizing any contribution to the system noise temperature is of great importance when detecting faint signals in the sky, since the integration time to obtain a given signal to noise ratio varies as the square of the system noise temperature. |
 | | For the purposes of noise temperature calculations, the antenna may be viewed as composed of perfect reflectors and perfect fl bodies, (i.e., the dome), at a given temperature. |
 | | For the purpose of noise calculation, the stop-sphere is a two-temperature surface; its lower hemisphere defines the ground temperature, while the upper hemisphere is at the same temperature as the aperture plane. |
| www.ecs.umass.edu /ece/allerton/papers1999/22 (2550 words) |