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Description Sensitivity vs Range for SETI.
Date
Source http://history.nasa.gov/CP-2156/ch5.5.htm
Author John H. Wolfe, Robert E. Edelson, John Billingham, R. Bruce Crow, Samuel Gulkis, Edward T. Olsen, Bernard M. Oliver, Allen M. Peterson, Charles L. Seeger, Jill C. Tarter.
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public domain


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Here is the original caption. Figure 5. Maximum sensitivities that may be realized during the observing program in both the sky survey (SS) and targeted observations (TS). For comparison, sloping lines representing a range of transmitter EIRP have been included so that the sensitivity required to detect classes of transmitters having the indicated EIRPs can be deduced as a function of distance to the transmitter.

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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June 1979

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Date/TimeThumbnailDimensionsUserComment
current18:09, 10 January 2008Thumbnail for version as of 18:09, 10 January 2008626 × 527 (37 KB)LouScheffer{{Information |Description= Sensitivity vs Range for SETI. |Source= http://history.nasa.gov/CP-2156/ch5.5.htm |Date=June, 1979 |Author=John H. Wolfe, Robert E. Edelson, John Billingham, R. Bruce Crow, Samuel Gulkis, Edward T. Olsen, Bernard M. Oliver, All

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