[12115] | 1 | #version 120 |
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| 2 | |
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| 3 | /* Bump mapping vertex program |
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| 4 | In this program, we want to calculate the tangent space light vector |
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| 5 | on a per-vertex level which will get passed to the fragment program, |
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| 6 | or to the fixed function dot3 operation, to produce the per-pixel |
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| 7 | lighting effect. |
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| 8 | */ |
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| 9 | // parameters |
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| 10 | uniform vec4 lightPosition; // object space |
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| 11 | uniform mat4 worldViewProj; |
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| 12 | |
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| 13 | attribute vec4 vertex; |
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| 14 | attribute vec3 normal; |
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| 15 | attribute vec4 tangent; |
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| 16 | attribute vec2 uv0; |
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| 17 | |
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| 18 | varying vec2 oUv0; |
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| 19 | varying vec3 oTSLightDir; |
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| 20 | |
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| 21 | void main() |
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| 22 | { |
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| 23 | // Calculate output position |
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| 24 | gl_Position = worldViewProj * vertex; |
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| 25 | |
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| 26 | // Pass the main uvs straight through unchanged |
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| 27 | oUv0 = uv0; |
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| 28 | |
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| 29 | // Calculate tangent space light vector |
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| 30 | // Get object space light direction |
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| 31 | // Non-normalised since we'll do that in the fragment program anyway |
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| 32 | vec3 lightDir = lightPosition.xyz - (vertex * lightPosition.w).xyz; |
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| 33 | |
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| 34 | // Calculate the binormal (NB we assume both normal and tangent are |
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| 35 | // already normalised) |
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| 36 | |
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| 37 | // Fixed handedness |
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| 38 | vec3 binormal = cross(normal, tangent.xyz) * tangent.www; |
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| 39 | |
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| 40 | // Form a rotation matrix out of the vectors, column major for glsl es |
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| 41 | mat3 rotation = mat3(vec3(tangent[0], binormal[0], normal[0]), |
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| 42 | vec3(tangent[1], binormal[1], normal[1]), |
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| 43 | vec3(tangent[2], binormal[2], normal[2])); |
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| 44 | |
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| 45 | // Transform the light vector according to this matrix |
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| 46 | oTSLightDir = rotation * lightDir; |
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| 47 | } |
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