A procedure has been developed which determines the excitation parameters of a linear array of isotropic sources such that the signal-to-noise ratio is maximized. The signal is considered to be a point source and the noise has a known distribution in space.
β¦ LIBER β¦
Signal-to-noise ratios for possible stellar occultations by pluto
β Scribed by A.S. Bosh; J.L. Elliot; S.E. Kruse; R.L. Baron; E.W. Dunham; L.M. French
- Book ID
- 103102198
- Publisher
- Elsevier Science
- Year
- 1986
- Tongue
- English
- Weight
- 314 KB
- Volume
- 66
- Category
- Article
- ISSN
- 0019-1035
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