Program 1: ray casting 2019

Due: 11:59pm, Friday September 20

Goal: In this assignment you will practice the ray casting methods that we are discussing.

Submission: Submit your assignment using this Google Form.

Introductory refs: On javascript.


BASIC GRADING:
  • 10% Part 0: properly turned in assignment
  • 50% Part 1: ray cast the colored boxes in the input file without lighting
  • 40% Part 2: color the boxes with Blinn-Phong illumination
  • Participation: Receive participation credit (outside of this assignment) for posting images of your progress, good or bad, on the class forum!
Note that prior parts need not remain functional if later parts are completed well.


General:
You will only render axis-aligned boxes in this assignment, which are described in an input file. We will test your program using several different input files, so it would be wise to test your program with several such files. The input files describe an array of boxes using JSON. An example input file resides at https://ncsucgclass.github.io/prog1/boxes.json. When you turn in your program, you should use this URL in hardcode as the location of the input boxes file — it will always be there. While testing, you should use a different URL referencing a file that you can manipulate, so that you can test multiple triangle files. Note that browser security makes loading local files difficult, so we encourage you to access any input files with HTTP GET requests.

We provide a small shell in which you can build your code. You can run the shell here, and see its code here. The shell shows how to draw pixels without using WebGL, and how to parse the input boxes.json file. It contains three drawing functions: one that merely draws random pixels, one that loads the boxes file and draws orthographic projections of them using canvas draw functions, and one that loads the boxes file and renders some random pixels in them. The last is probably closest to what you must produce for this program. Some of our programming exercises also contain relevant code.

All vertex locations should be described in world coordinates, meaning they do not require any transformation. Locate the eye at (0.5,0.5,-0.5), with a view up vector of [0 1 0] and a look at vector of [0 0 1]. Locate the window a distance of 0.5 from the eye, and make it a 1x1 square normal to the look at vector and centered at (0.5,0.5,0), and parallel to the view up vector. With this scheme, you can assume that everything in the world is in view if it is located in a 1x1x1 box with one corner at the origin, and another at (1,1,1). Put a white (1,1,1) (for ambient, diffuse and specular) light at location (-0.5,1.5,-0.5).

Advice: be careful to implement the algorithm we described in class, which loops first over pixels, then over primitives. The code you find in our exercises to date implements rasterization, which loops first over primitives, then pixels.

You should code the core of this assignment yourself. You may not use others' code to determine the location of pixels in the world, to do ray-box intersection, or to color a pixel. You may use math libraries you find, but you must credit them in comments. You may recommend libraries to one another, speak freely with one another about your code or theirs, but you may never directly provide any code to another student. If you are ever uncertain if what you are contemplating is permissible, simply ask me or the TA.


Part 0: Properly turned in assignment
Remember that 10% of your assignment grade is for correctly submitting your work! For more information about how to correctly submit, see this page on the class website.

Part 1: Using ray casting, render unlit, colored boxes
Use ray casting to render unlit boxes, with every pixel in each box having the unmodified diffuse color of that box (e.g, if the diffuse color of a box is (1,0,0), every pixel in it should be red). You will have to test for depth, to ensure that each box is correctly colored. You should see flatly colored boxes.

Part 2: Using ray casting, render lit boxes
Now you will have to perform a local Blinn-Phong lighting calculation at each intersection. As you perform that lighting calculation, don't forget to normalize your vectors. You should now see boxes with depth revealed by illumination, in the same locations and with the same silhouettes as in part 1.


EXTRA CREDIT GRADING: 
  • 461: 1% — arbitrarily sized images (and interface windows)
  • 461: 1% — arbitrary viewing setups
  • 461: 1% — off-axis and rectangular projections
  • 461: 1% — multiple lights at arbitrary locations
  • 461: 3% — 561: 1% — shadows during ray casting
  • 461: 5%561: 3% — render spheres
Other extra credit is possible with instructor approval. You must note any extra credit in your readme.md file, otherwise you will likely not receive credit for it.

Extra credit: Arbitrarily sized images and viewports 
Accept a new canvas (viewport) width and height through your UI. Size your canvas to match, and change your ray casting interpolation to match. This should affect every part of your assignment.

Extra credit: Support arbitrary viewing setups
Accept new eye location, view up and look at vectors through your UI. Reorient the window to be normal to the new look at vector and centered around the new eye. Render the scene with these viewing parameters. Note that with bad viewing parameters, you will not see the model. This should affect every part of your assignment.

Extra credit: Support off-axis and rectangular projections 
Accept new window parameters through your UI (relative to the viewing coordinates described by the look at and up vectors, these will be two X values (left, right) and two Y values (top, bottom)). Adjust your ray casting interpolation to this new windows. Render the scene with these new projection parameters. Note that if you also perform the arbitrary viewing extra credit, these coordinates may not be in world space! Also with bad projection parameters, you will not see the model. This should affect every part of your assignment.

Extra credit: Multiple and arbitrarily located lights
Read in an additional lights.json file that contains an array of objects describing light location and color. Note that these lights will have distinct ambient, diffuse and specular colors. Render the scene with these lights. During illumination, you will have to sum the colors all the lights. You can find an example lights.json file here. Assume that the input lights file will always reside at this URL when you turn in your code.

Extra credit: Detect shadows during ray casting
When performing lighting during ray casting, shoot an additional ray toward the light to decide if only ambient light reaches the intersection. If you also support multiple lights, make sure to shoot a ray at each light! This should only affect the last part of your assignment.

Extra credit: Render spheres 
Read in an additional spheres.json file that describes the sphere center, its radius, and one material (set of reflectivity coefficients) to use with them all. Read in and render these spheres in addition to the input primitives. You will have to perform ray-sphere intersection, and must code this yourself. You can find an example spheres.json file here. Assume that the input spheres file will always reside at this URL when you turn in your code.