1) Added support for a var called "__node__" in pynode scripts, that can be used to point to the desired pynode object, to make sure it is chosen.
2) Fixed a semi-obscure crash that could happen when reparsing a pynode script that was used by multiple nodes in different scenes. Memory corruption would happen if the reparsing failed during the recreation of the pynode object, not when executing it.
Submitted By:
Stephane SOPPERA (soppera)
It just increases the max value for gamma correction to 10f. Which
as noted in the patch is the same as the Gimp's color level tool.
Kent
if there was no zbuffer input. However this means a user settings can
be permanently changed without a user knowing. Now it just runs as if
this option is set if there is no zbuffer, but doesn't change the
setting.
Ongoing updates to the Blender.Node Python API:
- Changed Blender.Node.node to Blender.Node.Scripted to be more specific and conform to bpython API.
- Added a Blender.Node.Socket type to be used to define node sockets in a PyNode script. Also, socket type is inferred from the value(s) passed in, instead of also being defined by the script author.
- Added attr access to input and output sockets in the __call__ method. Ex: an input socket called 'color' can be accessed as self.input.color now.
These changes break existing pynode scripts, which shouldn't be a problem yet, of course, since we're still finishing this feature for 2.46. The wiki page and sample .blends have already been updated:
http://wiki.blender.org/index.php/BlenderDev/PyNodeshttp://wiki.blender.org/index.php/BlenderDev/PyNodes/API
Compositor:
Muting option to temporary disable/enable nodes.
Hotkey: press M on selection. It toggles.
Note: no menu entry yet, and drawing style could be tweakered...
The limit in the UI tooltips to set the amount of
images used in animation allow the zero value,
that cause a segfault.
This commit fix the UI, add a init value of 1 to
the node and also check in case that
node_composit_get_image return NULL.
* Make PyNodes work with threaded renderer. This patch is by Willian. He has worked hard on getting this sorted out - now you should be able to render with PyNodes AND multiple threads.
Reversion of premul bugfix, as it was apparently not
working all that well.
Note that this brings back the bug where the erase alpha
paint tool won't display correctly, since the UV image
editor just draws images in key alpha now.
(which basically tells the renderer and compositor to expect a
key image) is now done at the image user level.
This does have some caveats, as image users don't always work
the way I thought they would/should (for example, the same image user
structure is apparently used in the uv image editor for all images,
which is kindof odd).
The UV image editor also now smartly detects if the premul option is
set and draws the image using key alpha, instead of premul
The subversion level was upped to convert the old premul flag, which was at
the image level, to the new one, which is at the image user level.
a premul image but that doesn't work correct. Now it depremuls and
premuls again around the gamma correction. Better solution might be
possible, but this gives compatible results.
compositor node, another in render_realtime_texture. Note that multilayer images
in the image compositor node do not respect the premul flag (though I did write
commented out code for it).
As far as I can tell, the premul option never worked for multilayer images in the
image node, so I'm a little nervous about making it work properly there.
ton, any comments?
I had this assigned to Alfredo for a while, but he hasn't replied to the tracker at all, so I suspect he's not around. I'll commit this now to prevent crashes.
Some of the code in the glare node assumed that all buffers will be 4 channel RGBA, when in fact it was possible to give it a VEC3, such as a spec pass with no alpha, which would crash it. This fix just duplicates the input to a new temporary RGBA buffer to work on, if it's not already RGBA.
1) Trying to bring back compatibility with Python2.3.
2) Adding some stubs to compile blender player again on linux.
Please tell me if Blender still doesn't compile with py 2.3 or if the player isn't compiling. There was a binreloc related stub I needed to add, so probably the player wasn't compiling before the pynodes commit.
Thanks PanzerMKZ for reporting and testing part of the fix to py 2.3.
1) Including the Add->Dynamic submenu in the Nodes window header. Previously pynodes could only be added via toolbox.
2) Disabling pynodes execution when using more than one thread for rendering. This prevents the crashes while a proper fix isn't implemented.
using alpha as premul or nonpremul. Quite useful for brightness
tweaks.
Todo: version-patch this so ConvertPremul button goes away
Todo: make entire compositer accept non-premul by default... or both
This completes the pipeline make-over, as started in 2006. With this
option, during rendering, each sample for every layer and pass is being
saved on disk (looks like non-antialiased images). Then the composite
and color correction happens, then a clip to 0-1 range, and only in end
all samples get combined - using sampling filters such as gauss/mitch/catmul.
This results in artefact-free antialiased images. Even Z-combine or
ID masks now work perfect for it!
This is an unfinished commit btw; Brecht will finish this for strands.
Also Halo doesnt work yet.
To activate FSA: press "Save Buffers" and the new button next to it. :)
The 'Determinator' input didn't work at all - there was some quite weird code in there. I think the patch review process could have been quite a bit better on this one.
This is actually just the alpha value as currently being calculated
by the mist code. It is in many cases not very useful to have this as
alpha in shading result, also for postprocess and composite.
Note: this pass also works with "Mist" not set in World, of course.
- removed editors/area and put this all in screen
- added first python calls (note, a new c file for scriptlinks)
- added view3d editor callbacks (no drawing yet)
- added files in editors/interface
(Cmake and Scons has to be fixed, help welcome!)
- now areas/headers are being converted on file read
- note: previously saved 2.50 files will crash!!! (.B.blend)
- area regions are being drawn, first handler for cursor added (on edge)
- window duplicate and scale works correct for screen subdiv
Todos for me:
- need to fix things in syntax (function names) a bit still
- more operators for screen
- define how Context will work... still unresolved when it gets set
- docs!
Reviews of code structure is welcome!
There are also more todos now for others, but it can wait a couple of days
This commit makes it possible to use relative values when using a Blur node. There
is a new toggle in the node that can be used to enable the feature.
Thanks to David Millan Escriva for contribution!
This commit adds possibility to define black and white level of the
mapping curve of the RGB Curves node. This functionality is exactly
the same found in the Curves tool of the UV/Image Editor. It can be
used to extract wanted color ranges out of the input easily.
Thanks to Björn C. Schaefer for contribution!
Directional Blur node allows the users to do various blur operations on the input
image. It essentially offers three different kind of ways of blurring in one node.
It is possible to blur using a certain direction, spin and zoom. These three ways
can be used in conjunction.
The node contains following controls:
*Iterations, Wrap
*Center: X, Y
*Distance, Angle
*Spin
*Zoom
Iterations is used to determine the smoothness of the result. The more iterations,
the smoother result. Low values are good for preview.
Wrap means that the image is wrapped as if it was tiled on both x and y directions.
To see better what this means, try it with spin for instance.
Center values (X and Y) determine the location which is used as a pivot point for
the operations. It is center (0.5) of the image by default.
Distance and angle are used to adjust directional blur. The result can be described
as a sweep that varies based on given distance (bigger distance, longer sweep) and
angle. Angle is given in degrees.
Spin produces rotating blur based on given angle. Yet again it is in degrees. Also
negative values work.
Zoom causes the image to be zoomed towards set center point (Center values).
Thanks to Alfredo de Greef (eeshlo) for contribution.
Possible development ideas:
*Make an algorithm to extend image in case spin is used. Extend would temporarily
change the size of the canvas of the input image. Canvas would be filled based on
colors on the edges of the input image. After the blur operation has been done,
the image would be cropped back to normal size. The advantage of this would be nicer
result of spin (no problems with image size) on a computational cost.
*Make values animatable. This is something that is better solved on more general
level. ("everything is animatable" paradigm)
*Provide an option to calculate automatic value for iterations. A good value that
produces a smooth result could be calculated based on direction deltas. This would be
useful in conjuction of animatable values.
=================
Big commit, but little user visible changes.
- Dupliverts and duplifaces are now rendered as instances, instead
of storing all of the geometry for each dupli, now an instance is
created with a matrix transform refering to the source object.
This should allow us to render tree leaves more memory efficient.
- Radiosity and to some degree raytracing of such objects is not
really efficient still. For radiosity this is fundamentally hard
to solve, but raytracing an octree could be created for each object,
but the current octree code with it's fixed size doesn't allow this
efficiently.
- The regression tests survived, but with I expect that some bugs will
pop up .. hopefully not too many :).
Implementation Notes
====================
- Dupligroups and linked meshes are not rendered as instances yet,
since they can in fact be different due to various reasons,
instancing of these types of duplis that are the same can be added
for them at a later point.
- Each ObjectRen now stores it's own database, instead of there being
one big databases of faces, verts, .. . Which objects that are actually
rendered are defined by the list of ObjectRenInstances, which all refer
to an ObjectRen.
- Homogeneous coordinatess and clipping is now not stored in vertices
anymore, but instead computed on the fly. This couldn't work for
instances. That does mean some extra computation has to be done, but
memory lookups can be slow too, and this saves some memory. Overall
I didn't find a significant speed impact.
- OSA rendering for solid and ztransp now is different. Instead of e.g.
going 8 times over the databases times and rendering the z-buffer, it
now goes over the database once and renders each polygon 8 times. That
was necessary to keep instances efficient, and can also give some
performance improvement without instances.
- There was already instancing support in the yafray export code, now it
uses Blender's render instances for export.
- UV and color layer storage in the render was a bit messy before, now
should be easier to understand.
- convertblender.c was reorganized somewhat. Regular render, speedvector
and baking now use a single function to create the database, previously
there was code duplicated for it.
- Some of these changes were done with future multithreading of scene
and shadow buffer creation in mind, though especially for scene creation
much work remains to be done to make it threadsafe, since it also involves
a lot of code from blenkernel, and there is an ugly conflict with the way
dupli groups work here .. though in the render code itself it's almost there.
[#7660] Solaris 10 x86 support (Makefiles)
Hopefully it will not mess up anything for anyone else. I removed
some hardcoded static libs and made NAN_*_LIB definitions so they could be
overridden, to allow greater flexability.
Let me know if there are any problems/questions.
Kent
- update for new particle system
- made blenderplayer.exe compile again (DDS library missing)
- exchanged a few float math functions (logf, sinf, cosf, expf, powf) with their double counterparts in CMP_nodes
(MSVC chokes on them, because the compiler is not C99 compliant)
