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Solar cycle signal in air temperature in North America - Amplitude, gradient, phase and distributionThe considered investigation was motivated by three factors. One is related to an extension of single-channel MESA to multi-channel by Strand (1977), Morf et al. (1978), and Jones (1978). MESA is a high-resolution signal processing and spectrum analysis technique due to Burg (1975). The considered developments resulted in the discovery of the 11-year solar cycle signal in the change of the length of day by Currie (1980, 1981). They also led Currie (1981) to study the phase spectrum of the 11-year term in height H of sea level. The investigation tries to clarify the phase relations among the involved parameters. The second factor is connected with an application of the linear time domain technique used by Currie (1981) to temperature records to obtain more accurate information regarding the signal amplitude. The third factor of motivation is related to increases in the number of stations available for an analysis, the greater average length of the records, and the more accurate data set.
Document ID
19810054462
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Currie, R. G.
(NASA Goddard Space Flight Center Laboratory for Planetary Atmospheres, Greenbelt, MD; ARCO Oil and Gas Co., Dallas, TX, United States)
Date Acquired
August 11, 2013
Publication Date
April 1, 1981
Publication Information
Publication: Journal of the Atmospheric Sciences
Volume: 38
Subject Category
Meteorology And Climatology
Accession Number
81A38866
Distribution Limits
Public
Copyright
Other

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