Update of my 2013 FMX Slides on Physically Based Shading in PDF format

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The slides of my 2013 talk at FMX in Stuttgart were avail­able for down­load for a long time now in both Keynote and Pow­er­point for­mats. How­ev­er, peo­ple keep ask­ing for a PDF ver­sion. As I wrote in the com­ments once, I always had bad luck with the PDF export from Keynote, so I left it at that.

Yes­ter­day I made a major dis­cov­ery: The option “export to PDF” is not the only pos­si­bil­i­ty, in fact, it is quite an infe­ri­or one. The thing that I over­looked is that one can also just pre­tend to “print”, and then, in the sub­se­quent print­er dia­log, chose “save to PDF” instead. Not only does this give addi­tion­al options but also pro­duces nicer for­mat­ting and a small­er file!

I won­der how­ev­er the UI design­ers at Apple real­ly intend­ed this to be the pri­ma­ry means of PDF export? 

Any­way, I updat­ed the slides to PDF for­mat and also made some minor cor­rec­tions. I exchanged the font Human­ist 521 with Gill Sans. Appar­ent­ly the for­mer is an offi­cial clone of the lat­ter, and since Gill Sans is pre­in­stalled on a Mac any­way, I may as well just use the orig­i­nal. The met­rics also seem to look nicer in the PDF. I also copy-edit­ed some of the notes to be more edu­ca­tion­al than just a tran­script of my talk.

Here is again, the direct down­load link.

Down­load “FMX 2013 Slides PDF with Notes” fmx-11-revised.pdf – Down­loaded 914 times – 15 MB

Followup to Atmospheric Scattering—Part 1: Overview

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This post is the first in a series to fol­low-​up on my 2012 GPU Pro 3 arti­cle about atmos­pher­ic scat­ter­ing [11]. What I showed there was a full sin­gle-​scat­ter­ing solu­tion for a plan­e­tary atmos­phere run­ning in a pix­el shad­er, dynam­ic and in real time, with­out pre-​com­pu­ta­tion or sim­pli­fy­ing assump­tions. The key to this achieve­ment was a nov­el and effi­cient way to eval­u­ate the Chap­man func­tion [2], hence the title. In the time since then I have improved on the algo­rithm and extend­ed it to include aspects of mul­ti­ple scat­ter­ing. The lat­ter caus­es hor­i­zon­tal dif­fu­sion (twi­light sit­u­a­tions) and ver­ti­cal dif­fu­sion (deep atmos­pheres), and nei­ther can be ignored for a gen­er­al atmos­phere ren­der­er in a space game, for exam­ple.

I have writ­ten a Shader­toy that reflects the cur­rent state of affairs. It’s a mini flight sim­u­la­tor that also fea­tures clouds, and oth­er ren­der­ing good­ies. A WebGL2 capa­ble brows­er is need­ed to run it. Under Win­dows, the ANGLE/Direct3D trans­la­tor may take a long time to com­pile it (up to a minute is noth­ing unusu­al, but it runs fast after­wards). When suc­cess­ful­ly com­piled it should look like this:
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Most Popular Posts and Tags

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I have added a per­ma­nent page with a sum­ma­ry of the most pop­u­lar posts on this blog. I also tried to add mean­ing­ful tags to all posts. Here are the most impor­tant tags:

Content type tags

  • down­load — a down­load is avail­able is this post
  • gem — a code snip­pet or oth­er copy-paste thing is avail­able
  • math — posts that are heavy on math for­mu­lae

Topic tags

So, where are the stars?

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In my pre­vi­ous rant about dynam­ic expo­sure in Elite Dan­ger­ous (which hon­est­ly applies to any oth­er space game made to date), I made a rough cal­cu­la­tion to pre­dict the bright­ness of stars as they should real­is­ti­cal­ly appear in pho­tos tak­en in out­er space. My pre­dic­tion was, that,

  • for an illu­mi­na­tion of sim­i­lar strength to that on earth,
  • if the sun­lit parts are prop­er­ly exposed,
  • and with an angu­lar res­o­lu­tion of about 2 arc min­utes per pix­el,

then the pix­el-val­ue of a promi­nent star should be in the order of 1 to 3 (out of 255, in 8‑bit sRGB encod­ing). Since then I was curi­ous to find some real world val­i­da­tion for that fact, and it seems I have now found it.

ISS_and_Endeavour_EV+0

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\usepackage{cmbright}

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The ‘mod­ern’ look­ing sans-serif font I use recent­ly in \LaTeX equa­tions on this blog is called ‘Com­put­er Mod­ern Bright’, and actu­al­ly is not so mod­ern at all: Designed by Wal­ter Schmidt in 1996, it is still to date the only free sans-serif font avail­able for \LaTeX with full math sup­port. Type‑1 ver­sions of this font are avail­able in the cm-super pack­age, but I did­n’t need to install any­thing, because appar­ent­ly, Quick­La­TeX has them already. The only thing to do was adding just one line to the pre­am­ble:

\usepackage{amsmath}
\usepackage{amsfonts}
\usepackage{amssymb}
\usepackage{cmbright}   % computer modern bright

I also turned on the SVG images fea­ture that was added with ver­sion 3.8 of Quick­La­tex, so the equa­tions are no longer pixel­lat­ed on reti­na dis­plays or when zoom­ing in! Neat, huh?

Elite Dangerous: Impressions of Deep Space Rendering

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I am a backer of the upcom­ing Elite Dan­ger­ous game and have par­tic­i­pat­ed in their pre­mi­um beta pro­gramme from the begin­ning, pos­i­tive­ly enjoy­ing what was there at the ear­ly time. ‘Pre­mi­um beta’ sounds like an oxy­moron, pay­ing a pre­mi­um for an unfin­ished game, but it is noth­ing more than pur­chas­ing the same backer sta­tus as that from the Kick­starter cam­paign.

I came into con­tact with the orig­i­nal Elite dur­ing christ­mas in 1985. Com­pared with the progress I made back then in just two days, my recent per­for­mance in ED is lousy; I think my com­bat rat­ing now would be ‘com­pe­tent’.

But this will not be a game­play review, instead I’m going to share thoughts that were inspired while play­ing ED, most­ly about graph­ics and shad­ing, things like dynam­ic range, sur­face mate­ri­als, phase curves, ‘real’ pho­tom­e­try, and so on; so … after I loaded the game and jumped through hyper­space for the first time (actu­al­ly the sec­ond time), I was greet­ed by this screen fill­ing disk of hot plas­ma:

ED001

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X‑Plane announces Physically Based Rendering

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I always won­dered when X‑Plane would jump on the PBR band­wag­on. I like X‑Plane, I think its the best active­ly-devel­oped (*) flight sim­u­la­tor out there, but I always felt that shad­ing could be bet­ter. For instance, there is this unre­al­is­tic ‘Lam­bert-shad­ed’ world ter­rain tex­ture, which becomes too dark at sun­set; anoth­er is the dread­ed ‘con­stant ambi­ent col­or’ that plagues the shad­ing of objects.

Now in this post on the X‑Plane devel­op­er blog, Ben announces that Phys­i­cal­ly Based Ren­der­ing is a future devel­op­ment goal, yay! Then he goes on to say that, while sur­face shad­ing will be a solved prob­lem™ because of PBR, oth­ers like par­tic­i­pat­ing media (clouds, atmos­phere) would still need mag­ic tricks for the fore­see­able future. Con­tin­ue read­ing →

Journey into the Zone (Plates)

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I have exper­i­ment­ed recent­ly with zone plates, which are the 2‑D equiv­a­lent of a chirp. Zone plates make for excel­lent test images to detect defi­cien­cies in image pro­cess­ing algo­rithms or dis­play and cam­era cal­i­bra­tion. They have inter­est­ing prop­er­ties: Each point on a zone plate cor­re­sponds to a unique instan­ta­neous wave vec­tor, and also like a gauss­ian a zone plate is its own Fouri­er trans­form. A quick image search (google, bing) turns up many results, but I found all of them more or less unus­able, so I made my own.

Zone Plates Done Right

I made the fol­low­ing two 256×256 zone plates, which I am releas­ing into the pub­lic so they can be used by any­one freely.

Cosine zone plate with constrast weighting

Cosine zone plateCC0

Zone plates with contrast weighting

Sine zone plateCC0

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