Source code for rios.readerinfo


"""
This module contains the ReaderInfo class
which holds information about the area being
read and info on the current block

"""
# This file is part of RIOS - Raster I/O Simplification
# Copyright (C) 2012  Sam Gillingham, Neil Flood
#
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
#
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License
# along with this program.  If not, see <http://www.gnu.org/licenses/>.

import math

import numpy
from osgeo import gdal_array

from . import imageio


[docs]class ReaderInfo(object): """ ReaderInfo class. Holds information about the area being read and info on the current block """ def __init__(self, workingGrid, windowxsize, windowysize, overlap, loggingstream): self.loggingstream = loggingstream # grab the working grid self.workingGrid = workingGrid # save the window size and overlap self.windowxsize = windowxsize self.windowysize = windowysize self.overlap = overlap # work out the area being read self.xsize = int(round((self.workingGrid.xMax - self.workingGrid.xMin) / self.workingGrid.xRes)) self.ysize = int(round((self.workingGrid.yMax - self.workingGrid.yMin) / self.workingGrid.yRes)) # total number of blocks self.xtotalblocks = int(math.ceil(float(self.xsize) / self.windowxsize)) self.ytotalblocks = int(math.ceil(float(self.ysize) / self.windowysize)) # The feilds below apply to a particular block # and are filled in after this object is copied # to make it specific fir each block self.blockwidth = None self.blockheight = None self.blocktl = None self.blockbr = None self.xblock = None self.yblock = None # dictionary keyed by id() of the number array # value is a tuple with the GDAL dataset object # that corresponds to it, and the original filename self.blocklookup = {}
[docs] def setBlockDataset(self, block, dataset, filename): """ Saves a match between the numpy block read and it's GDAL dataset. So we can look up the dataset later given a block. This routine is for internal use by RIOS. Its use in any other context is not sensible. """ self.blocklookup[id(block)] = (dataset, filename)
[docs] def getWindowSize(self): """ Returns the size of the current window. Returns a tuple (numCols, numRows) """ return (self.windowxsize, self.windowysize)
[docs] def getOverlapSize(self): """ Returns the size of the pixel overlap between each window. This is the number of pixels added as margin around each block """ return self.overlap
[docs] def getTotalSize(self): """ Returns the total size (in pixels) of the dataset being processed """ return (self.xsize, self.ysize)
[docs] def getTransform(self): """ Return the current transform between world and pixel coords. This is as defined by GDAL. """ return self.workingGrid.makeGeoTransform()
[docs] def getProjection(self): """ Return the WKT describing the current projection system """ return self.workingGrid.projection
[docs] def getTotalBlocks(self): """ Returns the total number of blocks the dataset has been split up into for processing """ return (self.xtotalblocks, self.ytotalblocks)
[docs] def setBlockSize(self, blockwidth, blockheight): """ Sets the size of the current block This routine is for internal use by RIOS. Its use in any other context is not sensible. """ self.blockwidth = blockwidth self.blockheight = blockheight
[docs] def getBlockSize(self): """ Get the size of the current block. Returns a tuple:: (numCols, numRows) for the current block. Mostly the same as the window size, except on the edge of the raster. """ return (self.blockwidth, self.blockheight)
[docs] def setBlockBounds(self, blocktl, blockbr): """ Sets the coordinate bounds of the current block This routine is for internal use by RIOS. Its use in any other context is not sensible. """ self.blocktl = blocktl self.blockbr = blockbr
[docs] def getBlockCoordArrays(self): """ Return a tuple of the world coordinates for every pixel in the current block. Each array has the same shape as the current block. Return value is a tuple:: (xBlock, yBlock) where the values in xBlock are the X coordinates of the centre of each pixel, and similarly for yBlock. The coordinates returned are for the pixel centres. This is slightly inconsistent with usual GDAL usage, but more likely to be what one wants. """ (tl, _) = (self.blocktl, self.blockbr) (nCols, nRows) = self.getBlockSize() nCols += 2 * self.overlap nRows += 2 * self.overlap (xRes, yRes) = self.getPixelSize() (rowNdx, colNdx) = numpy.mgrid[0:nRows, 0:nCols] xBlock = tl.x - self.overlap * xRes + xRes / 2.0 + colNdx * xRes yBlock = tl.y + self.overlap * yRes - yRes / 2.0 - rowNdx * yRes return (xBlock, yBlock)
[docs] def setBlockCount(self, xblock, yblock): """ Sets the count of the current block This routine is for internal use by RIOS. Its use in any other context is not sensible. """ self.xblock = xblock self.yblock = yblock
[docs] def getBlockCount(self): """ Gets the count of the current block """ return (self.xblock, self.yblock)
[docs] def getPixelSize(self): """ Gets the current pixel size and returns it as a tuple (x and y) """ return (self.workingGrid.xRes, self.workingGrid.yRes)
[docs] def getPixRowColBlock(self, x, y): """ Return the row/column numbers, within the current block, for the pixel which contains the given (x, y) coordinate. The coordinates of (x, y) are in the world coordinate system of the reference grid. The row/col numbers are suitable to use as array indices in the array(s) for the current block. If the nominated pixel is not contained within the current block, the row and column numbers are both None (hence this should be checked). Return value is a tuple of 2 int values (row, col) """ transform = self.workingGrid.makeGeoTransform() imgRowCol = imageio.wld2pix(transform, x, y) imgRow = imgRowCol.y imgCol = imgRowCol.x blockStartRow = self.yblock * self.windowysize - self.overlap blockStartCol = self.xblock * self.windowxsize - self.overlap blockRow = int(imgRow - blockStartRow) blockCol = int(imgCol - blockStartCol) if ((blockRow < 0 or blockRow > (self.windowysize + 2 * self.overlap)) or (blockCol < 0 or blockCol > (self.windowxsize + 2 * self.overlap))): blockRow = None blockCol = None return (blockRow, blockCol)
[docs] def getPixColRow(self, x, y): """ This function is for internal use only. The user should be looking at getBlockCoordArrays() or getPixRowColBlock() for dealing with blocks and coordinates. Get the (col, row) relative to the current image grid, for the nominated pixel within the current block. The given (x, y) are column/row numbers (starting at zero), and the return is a tuple:: (column, row) where these are relative to the whole of the current working grid. If working with a single raster, this is the same as for that raster, but if working with multiple rasters, the working grid is the intersection or union of them. Note that this function will give incorrect/misleading results if used in conjunction with a block overlap. """ col = self.xblock * self.windowxsize + x row = self.yblock * self.windowysize + y return (col, row)
[docs] def isFirstBlock(self): """ Returns True if this is the first block to be processed """ return self.xblock == 0 and self.yblock == 0
[docs] def isLastBlock(self): """ Returns True if this is the last block to be processed """ xtotalblocksminus1 = self.xtotalblocks - 1 ytotalblocksminus1 = self.ytotalblocks - 1 return self.xblock == xtotalblocksminus1 and self.yblock == ytotalblocksminus1
[docs] def getFilenameFor(self, block): """ Get the input filename of a dataset """ # can't use ds.GetDescription() as may have been resampled (ds, fname) = self.blocklookup[id(block)] return fname
[docs] def getGDALDatasetFor(self, block): """ Get the underlying GDAL handle of a dataset """ (ds, fname) = self.blocklookup[id(block)] return ds
[docs] def getGDALBandFor(self, block, band): """ Get the underlying GDAL handle for a band of a dataset """ ds = self.getGDALDatasetFor(block) return ds.GetRasterBand(band)
[docs] def getNoDataValueFor(self, block, band=1): """ Returns the 'no data' value for the dataset underlying the block. This should be the same as what was set for the stats ignore value when that dataset was created. The value is cast to the same data type as the dataset. """ ds = self.getGDALDatasetFor(block) band = ds.GetRasterBand(band) novalue = band.GetNoDataValue() # if there is a valid novalue, cast it to the type # of the dataset. Note this creates a numpy 0-d array if novalue is not None: numpytype = gdal_array.GDALTypeCodeToNumericTypeCode(band.DataType) novalue = numpy.cast[numpytype](novalue) return novalue
[docs] def getPercent(self): """ Returns the percent complete. """ percent = int(float(self.yblock * self.xtotalblocks + self.xblock) / float(self.xtotalblocks * self.ytotalblocks) * 100) return percent