Introduction

VIPS comes with a convenient C++ API. It is a very thin wrapper over the C API and adds automatic reference counting, exceptions, operator overloads, and automatic constant expansion. You can drop down to the C API at any point, so all the C API docs also work for C++.

/* compile with:
 *      g++ -g -Wall example.cc `pkg-config vips-cpp --cflags --libs`
 */

#include <vips/vips8>

using namespace vips;

int
main (int argc, char **argv)
{ 
  if (VIPS_INIT (argv[0])) 
    vips_error_exit (NULL);
  
  if (argc != 3)
    vips_error_exit ("usage: %s input-file output-file", argv[0]);

  VImage in = VImage::new_from_file (argv[1],
    VImage::option ()->set ("access", VIPS_ACCESS_SEQUENTIAL));
  
  double avg = in.avg ();
  
  printf ("avg = %g\n", avg);
  printf ("width = %d\n", in.width ());
  
  in = VImage::new_from_file (argv[1],
    VImage::option ()->set ("access", VIPS_ACCESS_SEQUENTIAL));
  
  VImage out = in.embed (10, 10, 1000, 1000,
    VImage::option ()->
      set ("extend", "background")->
      set ("background", 128));
  
  out.write_to_file (argv[2]);
  
  vips_shutdown ();
  
  return (0);
}

Everything before VImage in = VImage::.. is exactly as the C API. vips_error_exit() just prints the arguments plus the libvips error log and exits with an error code.

VImage in = VImage::.. is the C++ equivalent of vips_image_new_from_file(). It works in the same way, the differences being:

There are a series of similar constructors which parallel the other constructors in the C API, see VImage::new_from_memory(), VImage::new_from_buffer(), and VImage::new_matrix().

The convenience function `VImage::new_from_image()` makes a constant image from an existing image. The image it returns will have the same size, interpretation, resolution and format as the image you call it on, but with every pixel having the constant value you specify. For example:

      new_image = image.new_from_image(12);

Now `new_image` has the same size as `image`, but has one band, and every pixel has the value 12. You can pass a `std::vector<double>` as the argument to make a constant image with a different number of bands.

There's also VImage::new_memory() and VImage::new_temp_file(), which when written to with VImage::write() will create whole images on memory or on disc.

The next line finds the average pixel value, it's the equivalent of the vips_avg() function. The differences from the C API are:

All other operations follow the same pattern, for example the C API call vips_add():

int vips_add( VipsImage *left, VipsImage *right, VipsImage **out, ... );

appears in C++ as:

VImage VImage::add( VImage right, VOption *options ) const

The next line uses VImage::width() to get the image width in pixels. There are similar functions paralleling vips_image_get_format() and friends. Use VImage::set() to set metadata fields, VImage::get_int() and c. to fetch metadata.

Next we reload the image. The VImage::avg() will have scanned the image and reached the end of the file, we need to scan again for the next operation. If we'd selected random access mode (the default) in the original VImage::new_from_file(), we would not need to reload.

The next line runs vips_embed() with two optional parameters. The first sets the value to an enum (here we use a string to set the value, it'll be looked up in the list of possible enum values, or you can use the symbols from the C API), the second sets the value to an int. The "background" parameter is actually a VipsArrayDouble: if you pass an int instead, it will be automatically converted to a one-element array for you. You can pass a std::vector<double> too: the utility function VImage::to_vectorv() is a convenient way to make one.

Finally, VImage::write_to_file() will write the new image to the filesystem. You can add a VOption as a final parameter and set options for the writer if you wish. Again, the operation will throw a VError exception on error. The other writers from the C API are also present: you can write to a memory array, to a formatted image in memory, or to another image.

The API docs have a handy table of all vips operations, if you want to find out how to do something, try searching that.

Automatic constant expansion

The C++ API will automatically turn constants into images in some cases. For example, you can join two images together bandwise (the bandwise join of two RGB images would be a six-band image) with:

VImage rgb = ...; 
VImage six_band = rgb.bandjoin( rgb );

You can also bandjoin a constant, for example:

VImage rgb_with_alpha = rgb.bandjoin( 255 );

Will add an extra band to an image, with every element in the new band having the value 255. This is quite a general feature. You can use a constant in most places where you can use an image and it will be converted. For example:

VImage a = (a < 128).ifthenelse( 128, a ); 

Will set every band element of a less than 128 to 128.

The C++ API includes the usual range of arithmetic operator overloads. You can mix constants, vectors and images freely.

The API overloads [] to be vips_extract_band(). You can write:

VImage xyz = VImage::xyz( 256, 256 ) - VImage::to_vectorv( 2, 128.0, 128.0 ); 
VImage mask = (xyz[0].pow( 2 ) + xyz[1].pow( 2 )).pow( 0.5 ) < 100;

to make a circular mask, for example.

The API overloads () to be vips_getpoint(). You can write:

VImage xyz = VImage::xyz( 256, 256 ) - VImage::to_vectorv( 2, 128.0, 128.0 ); 
// this will have the value [0, 0]
std::vector<double> point = xyz(128, 128);

Enum expansion

VIPS operations which implement several functions with a controlling enum, such as vips_math(), are expanded to a set of member functions named after the enum. For example, the C function:

int vips_math( VipsImage *in, VipsImage **out, VipsOperationMath math, ... );

where VipsOperationMath has the member VIPS_OPERATION_MATH_SIN, has a C convenience function vips_sin():

int vips_sin( VipsImage *in, VipsImage **out, ... );

and a C++ member function VImage::sin():

VImage VImage::sin( VOption *options = 0 ) const

Image metadata

VIPS images can have a lot of metadata attached to them, giving things like ICC profiles, EXIF data, and so on. You can use the command-line program vipsheader with the -a flag to list all the fields.

You can read metadata items with the member functions get_int(), get_double(), get_string() and get_blob(). Use get_typeof() to call vips_image_get_typeof() and read the type of an item. This will return 0 for undefined fields.

const char *VImage::get_string( const char *field ) throw( VError );

You can use the set() family of overloaded members to set metadata, for example:

void VImage::set( const char *field, const char *value );

You can use these functions to manipulate exif metadata, for example:

VImage im = VImage::new_from_file( "x.jpg" )
int orientation = im.get_int( VIPS_META_ORIENTATION );
im.set( VIPS_META_ORIENTATION, 2 );
im.write_to_file( "y.jpg" );

Extending the C++ interface

The C++ interface comes in two parts. First, VImage8.h defines a simple layer over GObject for automatic reference counting, then a generic way to call any vips8 operation with VImage::call(), then a few convenience functions, then a set of overloads.

The member definition and declaration for each operation, for example VImage::add(), is generated by a small Python program called gen-operators.py. If you write a new VIPS operator, you'll need to rerun this program to make it visible in the C++ interface.

You can write the wrapper yourself, of course, they are very simple. The one for VImage::add() looks like this:

VImage VImage::add( VImage right, VOption *options ) const
{
    VImage out;

    call("add",
        (options ? options : VImage::option())->
            set("out", &out)->
            set("left", *this)->
            set("right", right));

    return out;
}

Where VImage::call() is the generic call-a-vips8-operation function.