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Top Forums Shell Programming and Scripting AWK script - extracting min and max values from selected lines Post 302595389 by grincz on Friday 3rd of February 2012 03:07:23 AM
Old 02-03-2012
Hi ahamed,
results are more possible bus still not there..
Code:
max = 99,000
min = -1,000

I know that max should be over 160 and min around 40-50.
@Birei script is working on a smaller files but with the bigger files it doesn't work.

Maybe the problem is that some lines have 4digit values in the 5th column - like this?
Code:
ATOM  25935  O9   TB  1334      -0.810  62.300  67.500  1.00  0.00            
ATOM  25936  C10  TB  1334       0.460  61.650  67.370  1.00  0.00            
ATOM  25937  O11  TB  1334       1.350  61.990  66.560  1.00  0.00            
ATOM  25938  C12  TB  1334       0.690  60.320  68.140  1.00  0.00            
ATOM  25939  C13  TB  1334       1.260  60.630  69.520  1.00  0.00            
ATOM  25940  C14  TB  1334       1.220  59.500  70.510  1.00  0.00            
ATOM  25941  C15  TB  1334      98.740  64.820  67.620  1.00  0.00            
ATOM  25942  O16  TB  1334      98.500  66.090  67.050  1.00  0.00            
ATOM  25943  C17  TB  1334      98.350  67.110  68.070  1.00  0.00            
ATOM  25944  O18  TB  1334      98.930  67.020  69.120  1.00  0.00            
ATOM  25945  C19  TB  1334      97.930  68.370  67.370  1.00  0.00            
ATOM  25946  C20  TB  1334      96.460  68.870  67.670  1.00  0.00            
ATOM  25947  C21  TB  1334      96.170  70.140  66.910  1.00  0.00

 

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BALLS(1)						      General Commands Manual							  BALLS(1)

NAME
balls - preprocessor for space-filling models in Raster3D molecular graphics package SYNOPSIS
balls [-h] Balls reads a file describing atom colours and/or a PDB coordinate file and produces a file containing Raster3D descriptor records for each atom in the input file. The file produced by balls may be fed directly to render or it may be combined with descriptor files produced by other Raster3D utilities. EXAMPLES
To describe a simple space-filling model coloured by residue type: cat mycolours.pdb protein.pdb | balls | render > mypicture.png To include a pre-selected view matrix with the same model: cp view1.matrix setup.matrix cat mycolours.pdb protein.pdb | balls | render > mypicture.png To prepend header records describing a pre-selected scale and view: cat mycolours.pdb protein.pdb | balls -h > balls.r3d cat header.r3d balls.r3d | render > mypicture.png OPTIONS
-h Suppress header records in output. By default balls will produce an output file which starts with header records containing a default set of scaling and processing options. The -h flag will suppress these header records so that the output file contains only sphere descrip- tors. This option is useful for producing files which describe only part of a scene, and which are to be later combined with descriptor files produced by other programs. DESCRIPTION
The input to balls consists of a single text file containing colour information and atomic coordinates in PDB data bank format. Coordi- nates are output as Raster3D descriptor records with colours and sphere radii assigned according to the COLO records described below. By default atoms are assigned CPK colours. By default the output file contains a set of header records as required by the render program. The header is constructed to include a TMAT matrix corresponding to the transformation matrix contained in file setup.matrix (if it exists), or to the Eulerian angles contained in file setup.angles (if it exists). Colours are assigned to atoms using a matching process, using COLOUR records prepended to the input PDB file. Raster3D uses a pseudo-PDB record type with with COLO in the first 4 columns: Columns 1 - 4 COLO 7 - 30 Mask (described below) 31 - 38 Red component 39 - 46 Green component 47 - 54 Blue component 55 - 60 van der Waals radius in Angstroms 61 - 80 Comments Note that the Red, Green, and Blue components are in the same positions as the X, Y, and Z components of an ATOM or HETA record, and the van der Waals radius goes in place of the Occupancy. The Red, Green, and Blue components must all be in the range 0 to 1. The Mask field is used in the matching process as follows. First the program reads in and stores all the ATOM, HETA, and COLOUR records in input order. Then it goes through each stored ATOM/HETA record in turn, and searches for a COLOUR record that matches the ATOM/HETA record in all of columns 7 through 30. The first such COLOUR record to be found determines the colour and radius of the atom. In order that one COLOUR record can provide colour and radius specifications for more than one atom (e.g., based on residue or atom type, or any other criterion for which labels can be given somewhere in columns 7 through 30), the "#" symbol is used as a wildcard. I.e. a # in a COLOUR record matches any character in the corresponding column in an ATOM or HETA record. All other characters must match literally to count as a match. Note that the very last COLO record in the input should have # symbols in all of columns 7 through 30 in order to pro- vide a colour for any atom whose ATOM/HETA record fails to match any previous COLOUR record. This idea of matching masks for colour speci- fications is due to Colin Broughton. Several files of COLOUR records, including one based on Bob Fletterick's "Shapely Models" and another mimicking CPK model parts, are pro- vided as samples. ENVIRONMENT
The files setup.matrix and setup.angles, if they exist, affect the header records produced by balls. SOURCE
anonymous ftp site: ftp.bmsc.washington.edu web URL: http://www.bmsc.washington.edu/raster3d/raster3d.html contact: Ethan A Merritt University of Washington, Seattle WA 98195 merritt@u.washington.edu SEE ALSO
render(l), rods(l), ribbon(l) AUTHORS
Originally written by David J Bacon and Wayne F Anderson. Extensions and revisions by Ethan A Merritt. Raster3D 8 May 1999 BALLS(1)
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