This fixes the upostop-- test by auto-casting implicit constants to
unsigned (and it gives a warning for signed-unsigned comparisons
otherwise). The generated code isn't quite the best, but the fix for
that is next.
Also clean up the resulting mess, though not properly. There are a few
bogus warnings, and the legit ones could do with a review.
It now checks the next block to see if it is free with enough space and
carves off a chunk if so, or chops off the end of the current block if
smaller, otherwise it allocates *before* freeing.
The model gets unset during intermission and deleting the entity breaks
the intermission camera. This doesn't really feel right, but it does fix
the intermission camera. Really, the whole entity linking thing and
camera control needs a cleanup (and merging between nq and qw).
This makes a possible improvement to e1m3, only barely affects ad_tears,
but makes about 30% difference to gmsp3v2 (21fps to 27, and from 3300
leafs to 2700).
The cascade_shadow and cube_shadow names are no longer relevant thanks
to the staging images, and the output field for render passes is
optional in general and irrelevant for shadow maps.
The rendering of the shadow maps now takes the culling information into
account resulting in a drastic reduction of work. There's still more
work to be done, but demo1 peaks at over 1000fps at 640x480, gmsp3v2 now
gets 14fps (1920x1080) near the front gate (used to be 3, then 6),
ad_tears is up to 3fps, but marcher is still unhappy, but it has
infinite radius lights, so needs more culling work (clipped light
volumes will help, I think). Also, culling lights for which nothing has
moved within their volumes will help somewhat (though not as much for
most id maps, I suspect).
Using the translucency pass made it easy to have depth-tested
translucent "solid" light volumes instead of always visible lines (which
are still an option as that's useful too). Most importantly, being able
to see the surfaces helped no end in figuring out that my hulls were
created with counter-clockwise windings instead of quake's usual
clockwise windings and thus my hulls were being rendered inside-out in
the occlusion pass.
The results of the occlusion queries give the lights that don't have a
visible hull, but unfortunately that includes any lights which the
camera is inside, but simple distance checks sort that out (with a
fudge-factor for the icosahedron vertices (1.583 (3(2+p)/(2+3p), p is
golden ratio)).
My efforts (especially the collect zone (what was I thinking)) got
tracy's knickers in a twist resulting in vanishing zones in the server.
It looks like there are some synchronisation issues between cpu and gpu,
but I'm not *too* worried about it at this stage.
The info isn't used yet, but this shows that vulkan's occlusion queries
are at least somewhat useful. However, the technique isn't perfect:
infinite radius lights (1/r and 1/r^2) are difficult to cull, and all
lights can poke through thin enough walls, and then lights containing
the camera get culled incorrectly (will need a separate test). Still, it
looks like it will help once everything is tied together.
And make it callable directly (needed to be able to submit the command
buffer separately from the main commands (though this does mess with
tracy a little).
They weren't rendering properly at all due to the matrix updates getting
overwritten by the light data (I'd forgotten to advance the packet data
pointer).
This doesn't make much of a difference on the GPU, but it drastically
cuts down CPU usage, especially for ad_tears: shadow map drawing is down
from 16.3ms to 3.7ms thanks to no having to run the alias model queues
as often.
Batching shadow map rendering needs be able to reference matrices for
multiple lights in a single batch, but the only input is the view index,
so use that to look up the matrix index rather than using it to index
the matrices directly (modulo the base index that's still there).
Actually, only 29 are used because nvidia's drivers segfault when there
are more than 29 views (regardless of the exact bit pattern in the view
mask). This will allow rendering shadow maps in large batches, which
should make for better GPU utilization.
Even that's getting pretty big, but with the quanta at 128, that's a
maximum of 8 different image sizes (which is nice for my planned
"staging image" idea).
Interestingly, this caused a reduction in memory use for some maps (but
did increase marcher's again, but not as much as the bogus rounding
did). The idea was to use sparse bindings to remap shadow map layers,
but it turns out sparse bindings are insanely slow (beyond unusable).
However, the reduction in the number of shadow map images seems to be
worth it.
Since switching to the 1.2 api as a requirement, might as well use the
relevant structs instead of extension struct (for multiview). Came up
when double-checking the max views property due to running into what
appears to be an nvidia bug where > 29 views (any bit pattern) cause a
segfault when creating the pipeline.
I had missed that upping max lights to 2048 meant that up to 12288
matrices are needed for all the possible lights. This made it so the
light type could not be encoded in id_data, but the shaders never used
it anyway. This leaves one bit free.
I'd added some developer output to see how the layers were distributed
between images and found the image widths to be... odd. It turns out I
was double-adding the shadow_quanta. Oops. Results in ~164MB less memory
used by marcher (for 32 pixel quanta).
This allows "large" updates to be done in a single staging buffer packet
instead of one packet per quad (or slice). Currently, they're batched
into groups of 64 (not really enough for conchars, but that's only at
init-time, so not all that bad). Nicely, this seems to simplify the
staging code.
Fixes#65.
