Lecture 13: Global Illumination & Path Tracing (20)
dangeng184
I know that there's a typo and x and p refer to the same thing. But what I don't understand is what exactly x represents. It must be the point on the surface of the object at which our ray hits right? The weird thing is that a few slides from here the pseudocode has a line that says intersect(x, wi). But it makes no sense to intersect a line with a point. So does x just refer to the entire object?
dangeng184
Ok nevermind, I see that x just refers to a point position. The psuedocode in a few slides from here that says intersect(x, wi) is just odd notation for "find me the point on the light source that intersects with the ray ωi that extends from x. This was we get the radiance from the light source along ωi.
mylesdomingo
I didn't really understand this graph until I figured out what this polar coordinates system meant.
Fundamentally, what we are doing is for a point calculating the irradiance values from light sources from all different angles within a hemispherical zone.
To iterate over the integral, we use polar coordinates omega phi, to find each incidental ray within the hemisphere, which is equivalent to the colloquial description above.
I know that there's a typo and x and p refer to the same thing. But what I don't understand is what exactly x represents. It must be the point on the surface of the object at which our ray hits right? The weird thing is that a few slides from here the pseudocode has a line that says
intersect(x, wi)
. But it makes no sense to intersect a line with a point. So does x just refer to the entire object?Ok nevermind, I see that x just refers to a point position. The psuedocode in a few slides from here that says
intersect(x, wi)
is just odd notation for "find me the point on the light source that intersects with the ray ωi that extends from x. This was we get the radiance from the light source along ωi.I didn't really understand this graph until I figured out what this polar coordinates system meant.
Fundamentally, what we are doing is for a point calculating the irradiance values from light sources from all different angles within a hemispherical zone.
To iterate over the integral, we use polar coordinates omega phi, to find each incidental ray within the hemisphere, which is equivalent to the colloquial description above.