How it is working: - You load your file of hdf5 format - The program will try to find groups with certain codes like EBSD --> if there is no such data an error is thrown - One can modify the search codes - The data will be extracted using an algorithm fitted to the data - There are helper functions to convert data and build the EBSD object
Syntax
[ebsd] = loadEBSD_h5(fname, varargin)Options
| raw | import the data as recorded by the detector instead of the version cleaned up by the vendor software. Oxford files hold both, everybody else only the raw one |
| dataSet | which data set to import from a file that holds several of them, either as the number shown in the list printed on import, or as (part of) its name, e.g. EBSD.load(fname,'dataSet',2) or EBSD.load(fname,'dataSet','OIM Map 2') |
| headerOnly | return only phase/header metadata, skip reading the (potentially large) per-pixel position/rotation/phase data and any other top-level category (e.g. electron images). Also lists the data sets the file contains. |