Formski 138 Report post Posted July 7, 2007 Hi all, I'm trying to implement Nielsen's Atmospheric Scattering to a skydome in my Direct3D9 program and am getting a black sky. I initialize the parameters to the effects file as follows: float n = 0.9f; // Refractive index of air float N = 0.1f; // Molecular Density float K = 1.0f; float T = 1.0f; float c = (0.6544f*T - 0.6510f) * pow(10.0f,-16.0f); D3DXVECTOR4 sunDir = D3DXVECTOR4(0.5f, 0.5f, 0.5f, 0.0f); D3DXVec4Normalize(&sunDir, &sunDir); D3DXVECTOR4 sunColourIntensity = D3DXVECTOR4(1.0f, 1.0f, 1.0f, 100.0f); D3DXVECTOR4 BetaRayleigh; BetaRayleigh.x = 8 * pow(PI,3.0f) * pow((pow(n,2.0f)-1),2.0f); BetaRayleigh.y = BetaRayleigh.x; BetaRayleigh.z = BetaRayleigh.y; BetaRayleigh.x = BetaRayleigh.x / (3 * N * pow(650.0f,4.0f)); // Red (650nm) BetaRayleigh.x = BetaRayleigh.x / (3 * N * pow(610.0f,4.0f)); // Green (610nm) BetaRayleigh.x = BetaRayleigh.x / (3 * N * pow(475.0f,4.0f)); // Blue (475nm) D3DXVECTOR4 BetaMie; BetaMie.x = 0.434f * c* PI * 4*pow(PI,2.0f) * K; BetaMie.y = BetaMie.x; BetaMie.z = BetaMie.x; BetaMie.x = BetaMie.x / pow(0.650f,2.0f); // Red (650nm) BetaMie.y = BetaMie.y / pow(0.610f,2.0f); // Red (610nm) BetaMie.z = BetaMie.z / pow(0.475f,2.0f); // Red (475nm) D3DXVECTOR4 BetaDashRayleigh = D3DXVECTOR4( BetaRayleigh.x * 3 / (16 * PI), BetaRayleigh.y * 3 / (16 * PI), BetaRayleigh.z * 3 / (16 * PI), BetaRayleigh.w * 3 / (16 * PI)); D3DXVECTOR4 BetaDashMie = D3DXVECTOR4( BetaMie.x * 1 / (4 * PI), BetaMie.y * 1 / (4 * PI),BetaMie.z * 1 / (4 * PI), BetaMie.w * 1 / (4 * PI)); D3DXVECTOR4 BetaRM = BetaMie + BetaRayleigh; D3DXVECTOR4 OneOverBetaRM; OneOverBetaRM.x = 1 / BetaRM.x; OneOverBetaRM.y = 1 / BetaRM.y; OneOverBetaRM.z = 1 / BetaRM.z; D3DXVECTOR4 eyePos = D3DXVECTOR4(objRenderer->GetCameraPos()->x, objRenderer->GetCameraPos()->y, objRenderer->GetCameraPos()->z, 1.0f); // vHG = [1-g^2,1+g^2,-2g,insc] float g=2.0f; D3DXVECTOR4 HG = D3DXVECTOR4(); HG.x = 1 - pow(g, 2.0f); HG.y = 1 + pow(g,2.0f); HG.z = -2*g; D3DXVECTOR4 DensityAlt = D3DXVECTOR4(0.0f, 0.0f, 1.0f, 1.0f); D3DXVECTOR4 ToneMap = D3DXVECTOR4(1.0f, 1.0f, 1.0f, 1.0f); These are then uploaded to the effect file, which is the same as the one in Nielsen's paper. Also I have loaded in the vertex normals to the skydome and the function for the optical depth in the texture coordinates of the vertices. To top it off as well PIX (from the June 07 SDK) won't let me debug the shaders on this project anymore, but that's another problem. I'd appreciate it if anyone can offer any guidance on this please? Thanks Marco 0 Share this post Link to post Share on other sites
lilljohan 489 Report post Posted July 8, 2007 I don't know anything about Nielsen's Atmospheric Scattering but shouldn't BetaRayleigh.x = BetaRayleigh.x / (3 * N * pow(650.0f,4.0f)); // Red (650nm)BetaRayleigh.x = BetaRayleigh.x / (3 * N * pow(610.0f,4.0f)); // Green (610nm)BetaRayleigh.x = BetaRayleigh.x / (3 * N * pow(475.0f,4.0f)); // Blue (475nm)be BetaRayleigh.x = BetaRayleigh.x / (3 * N * pow(650.0f,4.0f)); // Red (650nm)BetaRayleigh.y = BetaRayleigh.y / (3 * N * pow(610.0f,4.0f)); // Green (610nm)BetaRayleigh.z = BetaRayleigh.z / (3 * N * pow(475.0f,4.0f)); // Blue (475nm) 0 Share this post Link to post Share on other sites
Formski 138 Report post Posted July 8, 2007 Err..um..yeah. Thanks for that!Unfortunately it doesn't change the end result.Marco 0 Share this post Link to post Share on other sites
DonnieDarko 251 Report post Posted July 8, 2007 Just a guess: shouldn't the sunDir vector have the w component set to 1.0f if it is to work correctly in a homogeneous coordinate system?Have you seen the source code snippets in Nielsens thesis? 0 Share this post Link to post Share on other sites
Formski 138 Report post Posted July 8, 2007 Hi Donnie,I had, but went through alot more closely and rewrote most of my code.I have got the vertex shader debugging through Pix again and am finding that the vBetaRayleigh constant is 0,0,0 in the shader. I set it as below:float fRayMult = 1.0f;float n = 0.9f; // Refractive index of airfloat N = 0.00001f; // Molecular DensityvBetaR.x = 8 * pow(PI,3.0f) * pow((pow(n,2.0f)-1),2.0f);vBetaR.y = vBetaR.x;vBetaR.z = vBetaR.y;vBetaR.x = vBetaR.x / (3 * N * pow(0.0000650f,4.0f)); // Red (650nm)vBetaR.y = vBetaR.y / (3 * N * pow(0.0000610f,4.0f)); // Green (610nm)vBetaR.z = vBetaR.z / (3 * N * pow(0.0000475f,4.0f)); // Blue (475nm)vBetaR *= fRayMult;My calcs are from Page 24 of the thesis, equation (2.2)Does this look correct? My thinking is that the light wavelengths are not correct unit wise. Plus I'm not sure what the fRayMult value should be?Thanks againMarco 0 Share this post Link to post Share on other sites
Formski 138 Report post Posted July 16, 2007 I still can't seem to get this to work.I've attached the effect file I'm using, which is basically the one in Nielsen's paper:// this is the effect file for the skydomematrix WorldViewProj : WORLDVIEWPROJECTION;float3 LightDir : LIGHTDIRECTION;vector vSunColorIntensity : SUNCOLORINTENSITY;float3 vBetaRayleigh : BETARAYLEIGH;float3 vBetaDashRayleigh : BETADASHRAYLEIGH;float3 vBetaMie : BETAMIE;float3 vBetaDashMie : BETADASHMIE;float3 vOneOverBetaRM : ONEOVERBETARAYLEIGHMIE;float4 vHG : HENYEYGG;float3 vEyePos : EYEPOSITION;float4 vDensityAlt : DENSDIST;float3 vToneMap : TONEMAP;float4 vConstants = {1.0f, -1.4426950f, 0.01f, 1000.0f}; // Constantsstruct VS_OUTPUT{ float4 Pos : POSITION; float4 Diff : COLOR0; float oFog : FOG;};VS_OUTPUT ScatteringSkyVS( float3 vPos : POSITION, float3 Norm: NORMAL, float2 Tex : TEXCOORD){ VS_OUTPUT Out = (VS_OUTPUT) 0 ; // transform Out.Pos = mul(float4(vPos, 1), WorldViewProj); // determine angle between sun and view direction float4 viewAngle ; viewAngle.x = dot(LightDir, Norm) ; viewAngle.y = (viewAngle.x * viewAngle.x)/2+2; viewAngle.z = lerp(Tex.y, vDensityAlt.z, Tex.x) ; viewAngle.w = Tex.y ; viewAngle.w = lerp(viewAngle.w, vDensityAlt.w, Tex.x) ; // Calculate Extinction terms for inscattered equation float3 extinction; extinction = vBetaRayleigh * viewAngle.z + vBetaMie * viewAngle.w; extinction = exp(-extinction); // Calculate mie scattering term (3.13) // Phase2 (theta) = (10g^2)/(1+g^2-2g*cos(theta))^(3/2) // vHG = [1-g^2,1+g^2,-2g,insc] float4 phaseThetaMie; phaseThetaMie.x = vHG.z * viewAngle.x + vHG.y; phaseThetaMie.y = rsqrt(phaseThetaMie.x); phaseThetaMie.z = pow(phaseThetaMie.y,3); phaseThetaMie.w = phaseThetaMie.z * vHG.x; // Inscattering (i) = (Beta R * Phase R(theta) + BetaM * PhaseM(Theta)) * // [1-exp(-Beta R*s), exp(-Beta M*s) ] / (Beta R + Beta M) float3 rayleigh; rayleigh = vBetaDashRayleigh * viewAngle.y; float3 mie; mie = vBetaDashMie * phaseThetaMie.w; float3 temp; temp = vConstants.x - extinction; float3 inscatter; // I(inscattering) inscatter = (mie + rayleigh) * vOneOverBetaRM; inscatter *= temp; inscatter *= vSunColorIntensity.xyz; inscatter *= vSunColorIntensity.w; // color Out.Diff.rgb = inscatter; Out.Diff.b += 0.15f; Out.Diff.a = 1.0f; return (Out);}float4 ScatteringSkyPS(VS_OUTPUT In) : COLOR{ return In.Diff;}technique ScatteringSky{ pass P0 { vertexShader = compile vs_2_0 ScatteringSkyVS(); pixelShader = compile ps_2_0 ScatteringSkyPS(); Lighting = FALSE; ZWriteEnable = FALSE; CullMode = NONE; //FillMode = WireFrame; }}The code for filling the constants to the effect is as follows:float vEyey = -objRenderer->GetCameraPos()->y; D3DXMATRIX matWVP; D3DXMatrixMultiply(&matWVP, objRenderer->GetViewMatrix(), objRenderer->GetProjectionMatrix()); pSkydomeScatterFX->SetMatrix(m_pWorldViewProj, &matWVP); float fRayMult = m_pAtmosphere->GetBetaRayleighMultiplier(); float fMieMult = m_pAtmosphere->GetBetaMieMultiplier(); D3DXVECTOR4 vSunDir = *m_pAtmosphere->GetSunDir(); vSunDir.y = vSunDir.y; pSkydomeScatterFX->SetVector(m_pLightDir, &vSunDir); D3DXVECTOR4 vSunColourIntensity = D3DXVECTOR4(1.0f, 1.0f, 1.0f, 100.0f); vSunColourIntensity.w = 9.2f - 550.0f * fMieMult; pSkydomeScatterFX->SetVector(m_pvSunColorIntensity, &vSunColourIntensity); float fDensityAltBase[4]; fDensityAltBase[0] = vEyey /1000.0f; fDensityAltBase[1] = powf(0.95f, fDensityAltBase[0]); fDensityAltBase[2] = 20000.0f * expf(-vEyey / 10000.0f); fDensityAltBase[3] = 8000.0f * expf(-vEyey / 20000.0f); pSkydomeScatterFX->SetValue(m_pvDensityAlt, &fDensityAltBase, 16); D3DXVECTOR4 vBetaR, vBetaDashR, vBetaM, vBetaDashM, vBetaRM, vOneOverBetaRM; // MF vBetaR = *m_pAtmosphere->GetBetaRayleigh(); vBetaR *= fRayMult; pSkydomeScatterFX->SetVector(m_pvBetaRayleigh, &vBetaR); vBetaDashR = *m_pAtmosphere->GetBetaDashRayleigh(); vBetaDashR *= fRayMult; pSkydomeScatterFX->SetVector(m_pvBetaDashRayleigh, &vBetaDashR); vBetaM = *m_pAtmosphere->GetBetaMie(); vBetaM *= fMieMult; pSkydomeScatterFX->SetVector(m_pvBetaMie, &vBetaM); vBetaDashM = *m_pAtmosphere->GetBetaDashMie(); vBetaDashM *= fMieMult; pSkydomeScatterFX->SetVector(m_pvBetaDashMie, &vBetaDashM); vBetaRM = vBetaR + vBetaM; //pSkydomeScatterFX->SetVector(m_pvBetaRM, &vBetaRM); vOneOverBetaRM.x = 1.0f / vBetaRM.x; vOneOverBetaRM.y = 1.0f / vBetaRM.y; vOneOverBetaRM.z = 1.0f / vBetaRM.z; pSkydomeScatterFX->SetVector(m_pvOneOverBetaRM, &vOneOverBetaRM); float fIns = 0.3f; // Inscattering Multiplier float SunTheta = m_pAtmosphere->GetSunTheta(); // Sun Theta // vHG = [1-g^2,1+g^2,-2g,insc] float g = 0.444f + vEyey * (float)1.053e-5 - (float)5.984e-2 * SunTheta - (float)3.521e-6 * SunTheta * vEyey; float g2 = 0.100f + vEyey * (float)1.11e-5 - (float)3.18e-2 * SunTheta - (float)6.01e-6 * SunTheta * vEyey; float c = -0.076923f + 153.846f * fMieMult; g = g + c*(g2-g); D3DXVECTOR4 vG = D3DXVECTOR4(1-g*g, 1+g*g, 2*g, fIns); pSkydomeScatterFX->SetVector(m_pvHG, &vG); D3DXVECTOR4 DensityAlt = D3DXVECTOR4(0.0f, 0.0f, 1.0f, 1.0f); DensityAlt.x = vEyey / 1000.0f; DensityAlt.y = powf(0.95f, DensityAlt.x); DensityAlt.z = 20000.0f * expf(-vEyey / 10000.0f); DensityAlt.w = 8000.0f * expf(-vEyey / 20000.0f); D3DXVECTOR4 vEye = D3DXVECTOR4(objRenderer->GetCameraPos()->x, vEyey, objRenderer->GetCameraPos()->z, 1.0f); pSkydomeScatterFX->SetVector(m_pvEyePos, &vEye);and the Atmosphere object has the following:// Calculate Rayleigh and Mie scattering terms fBetaRayleighMultiplier = RayleighMultiplierDefault; fBetaMieMultiplier = MieMultiplierDefault; SetTime(0.0f); vSunColour = D3DXVECTOR4(1.0f, 1.0f, 1.0f, 1.0f); // Set to white float fLambda[3],fLambda2[3], fLambda4[3]; // Lambda Factors fLambda[0] = RedWavelength; // red // note 650e-9 m = 650nm. fLambda[1] = GreenWavelength; // green fLambda[2] = BlueWavelength; // blue for (int i=0; i < 3; i++) { fLambda2[i] = fLambda[i]*fLambda[i]; fLambda4[i] = fLambda2[i]*fLambda2[i]; } vLambda2 = D3DXVECTOR4(fLambda2[0], fLambda2[1], fLambda2[2], 0.0f); vLambda4 = D3DXVECTOR4(fLambda4[0], fLambda4[1], fLambda4[2], 0.0f); vBetaRayleigh.w = 0.0f; vBetaRayleigh.x = 8 * PI * PI * PI * (n*n-1)*(n*n-1); vBetaRayleigh.y = vBetaRayleigh.x; vBetaRayleigh.z = vBetaRayleigh.y; vBetaRayleigh.x = vBetaRayleigh.x / (3 * N * vLambda4.x); // Red (650nm) vBetaRayleigh.y = vBetaRayleigh.y / (3 * N * vLambda4.y); // Green (610nm) vBetaRayleigh.z = vBetaRayleigh.z / (3 * N * vLambda4.z); // Blue (475nm) /*vBetaRayleigh.x = 2.44e-5f; vBetaRayleigh.y = 1.18e-5f; vBetaRayleigh.z = 6.95e-6f;*/ float K = 0.67f; float c = (0.6544f*T - 0.6510f) * (float)10e-16; //float c = (0.6544f*2.0f - 0.6510f) * (float)10e-16; vBetaMie.w = 0.0f; vBetaMie.x = 0.434f * c * PI * 4 * PI * PI * K; vBetaMie.y = vBetaMie.x; vBetaMie.z = vBetaMie.x; vBetaMie.x = vBetaMie.x / vLambda2.x; // Red (650nm) vBetaMie.y = vBetaMie.y / vLambda2.y; // Red (610nm) vBetaMie.z = vBetaMie.z / vLambda2.z; // Red (475nm) /*vBetaMie.x = 2.4e-6f; vBetaMie.y = 6e-7f; vBetaMie.z = 4e-7f;*/ vBetaDashRayleigh = D3DXVECTOR4(vBetaRayleigh.x * 3 / (16 * PI), vBetaRayleigh.y * 3 / (16 * PI), vBetaRayleigh.z * 3 / (16 * PI), 0.0f); vBetaDashMie = D3DXVECTOR4( vBetaMie.x / (4 * PI), vBetaMie.y / (4 * PI), vBetaMie.z / (4 * PI), 0.0f);Finally the header for the atmosphere object has the following constants:#define PlanetRadius 6.378e6#define AtmosphereRadius 6.378e6#define SunBrightness 40.0f#define RedWavelength 650e-9f // -9#define GreenWavelength 610e-9f#define BlueWavelength 475e-9f#define MieMultiplierDefault 0.01f#define RayleighMultiplierDefault 0.2f#define n 1.003f // Refractive index of air#define N 2.545e25f // Molecular Density#define T 555e-9f // Turbidity - see page 35At this stage if I override the Rayleigh and Mie constants I get a pretty much dark blue background with no sun appearing and almost no change in shading intensity.I'd appreciate it if anybody can see where it has gone wrong as I've spent several days trying to debug this. As far as I can see I've covered all bases so I'm suspecting a stupid error somewhere.Thanks in advance,Marco 0 Share this post Link to post Share on other sites
Ysaneya 1383 Report post Posted July 16, 2007 Atmosphere radius is the same than planet radius !?Y. 0 Share this post Link to post Share on other sites
bluntman 255 Report post Posted July 16, 2007 Quote:Original post by FormskivBetaR.x = vBetaR.x / (3 * N * pow(0.0000650f,4.0f)); // Red (650nm)vBetaR.y = vBetaR.y / (3 * N * pow(0.0000610f,4.0f)); // Green (610nm)vBetaR.z = vBetaR.z / (3 * N * pow(0.0000475f,4.0f)); // Blue (475nm)MarcoAlot of the constants you are using are very small numbers, e.g. (3 * N * pow(0.0000650f,4.0f)) with N = 0.00001f produces a value of around 1.0e-67, which is WAY smaller than a float can represent. If you calculate that you get 0's in your floats. You need to change your units I think! 0 Share this post Link to post Share on other sites
Formski 138 Report post Posted July 16, 2007 Quote:Original post by YsaneyaAtmosphere radius is the same than planet radius !?Y.Sorry, this was a constant copied from another piece of code somewhere else that is not used anywhere. 0 Share this post Link to post Share on other sites
mrhyperpenguin 468 Report post Posted July 16, 2007 when you're setting your effect parameters, you set your sun color to white. this isn't correct. the sun color is white in space but once it reaches our atmosphere it is absorbed by atmospheric particles and out-scattered. try using this method to calculate your sun color. Vector3 ComputeAttenuation(float fTheta, int nTurbidity) { float fBeta = 0.04608365822050f * nTurbidity - 0.04586025928522f; float fTauR, fTauA; float[] fTau = new float[3]; float m = 1.0f / ((float)Math.Cos(fTheta) + 0.15f * (float)Math.Pow(93.885f - fTheta / MathHelper.Pi * 180.0f, -1.253f)); // Relative Optical Mass int i; float[] fLambda = new float[3]; fLambda[0] = 0.65f; // red (in um.) fLambda[1] = 0.57f; // green (in um.) fLambda[2] = 0.475f; // blue (in um.) for (i = 0; i < 3; i++) { // Rayleigh Scattering // Results agree with the graph (pg 115, MI) */ // lambda in um. fTauR = (float)Math.Exp(-m * 0.008735f * (float)Math.Pow(fLambda[i], -4.08f)); // Aerosal (water + dust) attenuation // beta - amount of aerosols present // alpha - ratio of small to large particle sizes. (0:4,usually 1.3) // Results agree with the graph (pg 121, MI) const float fAlpha = 1.3f; fTauA = (float)Math.Exp(-m * fBeta * (float)Math.Pow(fLambda[i], -fAlpha)); // lambda should be in um fTau[i] = fTauR * fTauA; } return new Vector3(fTau[0], fTau[1], fTau[2]); }see how things work out with this little update. also note that i tried setting the sun color to white in my implementation and it didn't give me your results, so something else somewhere must be also broken.(i got this method from the Hoffman/Preetham scattering demo) 0 Share this post Link to post Share on other sites
Formski 138 Report post Posted July 17, 2007 I've grabbed some of the code from the ATI Scattering Demo project atmosphere.cpp file and worked that in. Now it's a pretty much flat coloured blue skydome.The following is what I am setting parameters to the shaders as:LightDir = (0, 0, 1)vSunColorIntensity = (0.0081549045, 0.0012669618, 1.5124032e-5, 3.6999998)vBetaRayleigh =(0.00013942779, 0.00017975607, 0.00048890937)vBetaDashRayleigh = (8.3214827e-6, 1.0728400e-6, 2.9179630e-5)vBetaMie = (5.7405967e-5, 6.4610540e-5, 0.00010514310) vBetaDashMie = (1.3337873e-5, 1.5144456e-5, 2.4976185e-5)vOneOverBetaRM = (5080.4292, 4092.2119, 1683.3529)vHG = (0.99229097, 1.0077090, -0.17560202, 0.30000001)vEyePos = (0, 5000, 0, 1)vDensityAlt = (5.0, 0.77378088, 12130.613, 6230.4063)Also I am storing pow(NormalY, 0.2f) in the second texture coordinate and 1.05f * 190000.0f in the first texture coordinate for each vertex.Using a Rayleigh multiplier of 0.2 and Mie miemultiplier of 0.01. I'm finding in the shader the calculated 'rayleigh' and 'mie' variables are coming out extremely small.Marco 0 Share this post Link to post Share on other sites
Kenneth Gorking 124 Report post Posted July 18, 2007 Nielsen uses 'phaseThetaMie.x = -vHG.z * viewAngle.x + vHG.y', but yours is 'phaseThetaMie.x = vHG.z * viewAngle.x + vHG.y'. Might be it :) 0 Share this post Link to post Share on other sites
Formski 138 Report post Posted July 19, 2007 Thanks Kenneth - I had copied over Nielsen's shader verbatim and not seen this error in it.After playing around further with this here is the current result with the sun at Phi = PI/2 and Theta = 0 (set using Preetham's code so sun is facing viewpoint) (Note I'm not shading the terrain at all yet, only the skydome)It may not be obvious but the shading goes from lighter at the horizon to dark at the top of the skydome with no 'sun' visible. The sun direction and intensities is calculated using Preetham's code from his ATI demo and the .w elements of the intensity vector is set using Nielsen's code (which I've pretty much copied over into my shader setup pathway)I've been through the BetaRayleigh and BetaMie calculations with both Excel and in code and ensured they matched (doing everything one step at a time so rounding errors are eliminated) which has changed the values from my post above, so please ignore them.The skydome is a half sphere created in 3DSMax with normals reversed inwards. It's radius is set to 200000 (assuming 200000 metres or 200KM) The altitude of the screenshots above is at 5000.My thoughts were that the density calculations may be incorrect (equation 5.7 & 5.8). At each vertex I have calculated in Tex.x the fifth root of the vertex's Y-Normal value, and in Tex.y I have calculated (1.05-TexX)*190000 which is as per (5.8)The only thing that sticks out still is that I'm unsure what units Nielsen was using for his code - are distances/positions in Metres, KMs etc?Marco 0 Share this post Link to post Share on other sites
mrhyperpenguin 468 Report post Posted July 19, 2007 In my testing, the radius of the skydome does not effect the color of the sky. Also, i cannot recall what units the Nielsen paper uses. Although i have another suggestion for you to try. You have the Mie Scattering multiplier set to 0.01f, try setting it to something smaller.image 1 Mie Scattering Multiplier set to 0.01fimage 2Mie Scattering Multiplier set to 0.003f 0 Share this post Link to post Share on other sites
Formski 138 Report post Posted July 19, 2007 Quote:Original post by mrhyperpenguinIn my testing, the radius of the skydome does not effect the color of the sky. Also, i cannot recall what units the Nielsen paper uses. Although i have another suggestion for you to try. You have the Mie Scattering multiplier set to 0.01f, try setting it to something smaller.image 1 Mie Scattering Multiplier set to 0.01fimage 2Mie Scattering Multiplier set to 0.003fThanks for that, but I found setting the Mie Scattering multipier to 0.003f simply whited out my skydome entirely.After re-grabbing the code from the Preetham ATI scattering demo for the Beta Rayleigh values it seems to have cleaned up part of the problem. Now I have a skydome that correctly handles the changes in altitude and also the horizon correctly, but no sun!The HorizonThe 'Sun'This is with the sun at the zenith (Theta = 0, Phi = PI/2)I take it Nielsen was pretty much using Preetham's code for setting the parameters? 0 Share this post Link to post Share on other sites
glaeken 294 Report post Posted July 20, 2007 Looking at your Vertex Shader, I don't see anywhere where you compute the viewing direction (unless I'm completely blind). Looking up the Nielsen paper, he calls this vEyeVert. This might help a bit ;)Edit: Doh, I was looking at the wrong effect file, nevermind. I wasn't too familier with Nielsen's technique and I was just recalling from the Hoffman-Preethem paper.[Edited by - glaeken on July 23, 2007 7:49:42 AM] 0 Share this post Link to post Share on other sites
Formski 138 Report post Posted July 20, 2007 glaeken,I thought that was covered by calculating the dot product of the vertex normal of the skydome with the light direction of the sun?Is it the Mie or the Rayleigh Scattering that will show the sun on the skydome? I thought it was the Mie scattering personally.Marco 0 Share this post Link to post Share on other sites