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Stability and noise spectra of relative Loran-C frequency comparisonsRelative comparisons of Loran-C frequency transmissions between the master station of Catanzaro (Simeri Crichi) and the X, Z slave stations of Estartit (Spain) and Lampedusa (Italy) are carrying out by the GG LORSTA monitor station of the Mediterranean Sea Loran-C chain. These comparisons are able to emphasize the relative and, under certain conditions, the absolute rate of the emitting standard frequencies of the slave stations and some relevant statistical properties of the Loran-C Method for frequency transmission and time synchronization. The stability of each Loran-C frequency standard transmission is subject to perturbations, more or less known, due to the propagation medium and other causes. Following the Allan (1966) method for data processing, the performance of the relative rate of frequency of the transmissions of the X, Z slave stations are described calculating the standard deviation of a set of N frequency measurements from its mean averaged during sampling times. This standard deviation is designated as the measure of the stability of the Loran-C frequency transmission.
Document ID
19750003222
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Proverbio, E.
(International Astronomical Latitude Station Cagliari, Italy)
Quesada, V.
(International Astronomical Latitude Station Cagliari, Italy)
Simoncini, A.
(International Astronomical Latitude Station Cagliari, Italy)
Date Acquired
August 8, 2013
Publication Date
January 1, 1973
Publication Information
Publication: NASA. Goddard Space Flight Center Proc. of the 5th Ann. NASA and DOD Precise Time and Time Interval Planning Meeting
Subject Category
Aircraft Communications And Navigation
Accession Number
75N11294
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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