% @(#)visualpers.hlq 17.1.1.1 (ESO-IPG) 01/25/02 17:21:10 %++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ %.COPYRIGHT (c) 1993 European Southern Observatory %.IDENT visualpers.hlq %.AUTHOR 06-APR-93, IPG/ESO %.KEYWORDS MIDAS, help files, %.PURPOSE On-line help file for the command: VISUAL/PERS %.VERSION 1.0 JS : Creation, 06-APR-93 %---------------------------------------------------------------- \se SECTION./PERS \es\co VISUAL/PERS JS 06-APR-93 \oc\su VISUAL/PERS Wavelet_File_Name [output_visu_file] [Display_Number] [Visu_Mode] [Increment] [Threshold] [Display] \us\pu Purpose: visualizes the wavelet transform of an image in perspective \up\sy Syntax: VISUAL/PERS Wavelet_File_Name [output_visu_file] [Display_Number] [Visu_Mode] [Increment] [Threshold] [Display] \ys\pa Wavelet_File_Name = Wavelet File Name \ap\pa output_visu_file = file created for the visualisation. The default value is file_visu. \ap\pa Display_Number = the midas number of the created display window. The default value is 1. \ap\pa Visu_Mode = CO (Color) or BW (Black and White) The default value is CO. \ap\pa Increment = parameter which defines the number of lines of the image used. If Increment = 3, only on line on 3 are used. The default value is 1. \ap\pa Threshold = parameter which defines the maximum value which is taken into account. All the values superior to this maximum are set to the maximum. The maximum value is:\\ M = Standard_Deviation (scale) * Threshold\\ The default value is 5. \ap\pa Display = Y or N. If Display = Y then the created image is displayed in the window; if Display = N then no display is done, only the output_visu_file is created. Ddefault is Y. \ap\see See also: WAVE/TRANSF, VISUAL/SYNT, VISUAL/WAVE, VISUAL/PLAN, VISUAL/CUBE, VISUAL/CONT \ees\no Note: If the wavelet transform was computed by mallat's algorithm, this command has no effect. \on\exs Examples: \ex VISUAL/PERS Wavelet_File_Name Visualizes the wavelet transform in perspective \xe \sxe