Full text: Actes du Symposium International de la Commission VII de la Société Internationale de Photogrammétrie et Télédétection (Volume 1)

As an example of an unresolvable feature, consider diurnal vari- 
ations, for instance in a photochemically active species. The evolution of 
such a constituent will contain a number of tidal harmonics, each moving with 
zonal wavenumber is c, - 2mm rads/day, or m cpd. Wavenumber 1 contribution 
lies precisely on the Nyquist fold. A11 higher wavenumbers lie outside the 
region permitted by aliasing. 
In addition to guarding against contamination by unresolvable 
components, the converse must also be avoided. Resolvable spectra within the 
allowed region must not be allowed to project upon their aliases outside it. 
From the standpoint of computing space-time spectra, this simply means that 
only values within the permitted region of wavenumber-frequency space are 
calculated. The situation in determining synoptic fields, however, is more 
delicate. Consider a spectral approach where the asynoptic data are expanded 
synoptically in a set of wavenumbers and assimilated by integrating forward 
in time to derive synoptic charts. The wavenumbers allowed in computation digi 
must be restricted in accordance with the aliasing limitations. Similarly, been 
albeit implicit, the time integration must be filtered. Otherwise aliases scan 
will manifest themselves in the synoptic products. This holds equally for pixe 
the additional contamination inherent to combined data. Failure to eliminate orth 
this contamination can result in a complete aberration of the true behavior panc 
(Salby, 1982b; 1982c). Clearly the aliases should be excluded from model of t 
initialization. Since they obey none of the physical laws prescribed in the à ne 
model, it is unlikely that their presence would be benign. dise 
Acknowledgment | digi 
This research was performed while the author was employed at the 
National Center for Atmospheric Research, sponsored by the National Science of t 
Foundation. and 
of a 
References fore 
Bdth, M. 1974: Spectral Analysis in Geophysics. Elsevier, Amsterdam. 563 pp. 
Chapman, W., Cross, M., Flower, D., Peckham, G., and S. Smith, 1974: A 
spectral analysis of global atmospheric temperature fields observed 
by the selective chopper radiometer on the Nimbus-4 satellite 
during the year 1970-1. Proc. Roy. Soc. Lond. A338, 57-76. 
  
  
  
gate 
and 
Hartmann, D., 1976: The structure of the stratosphere in the Southern Hemi- 1984 
sphere during late winter 1973 as observed by satellite. J. Atm. reso 
Sci., 33 1141-1154. of f- 
of s 
Hayashi, Y., 1980: A method for estimating space-time spectra from polar 
orbiting satellite data. J. Atm. Sci. 37, 1385-1392, 
ment 
Salby, M., 1982a: Sampling theory for asynoptic satellite observations. Part done 
I: Space-time spectra, resolution, and aliasing. Submitted to J. mate 
Atm. Sci. of it 
; 4 digi 
>» 1982b: Sampling theory for asynoptic satellite observations. Part II: tion 
Fast Fourier Synoptic Mapping. Submitted to Uc Aui. Sci. 10 x 
. 1982c: Synoptic field reirieval from asynoptic satellite observations. 
Proceedings, International Symposium on Data Interpretation, of Swed 
the International Society of Photogrammetry and Remote Sensing. of 1 
Toulouse, France, 1982. S in 1 
the 
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ELEME EE AREE 1 — 7 
 
	        
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