LlGetSunDirection/de
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Beschreibung
Funktion: vector llGetSunDirection( );177 | Funktions ID |
0.0 | Verzögerung |
10.0 | Energie |
gibt die Sonnenrichtung in der Region.
Die Sonnenposition kann - abhängig von den Wünschen des Simbesitzers - dynamisch oder statisch sein.
Beispiele
Dies kann genutzt werden um schnell zu bestimmen ob Tag oder Nacht ist (in gekürzten SL Tagen). Wenn der zurückgegebene Z Parameter des Vektors positiv ist, steht die Sonne über dem Horizont (Tag) ansonsten unter dem Horizont (Nacht).
<lsl>integer lightsOn = -1;//nicht TRUE oder FALSE
CheckSun() {
vector sun = llGetSunDirection(); integer turnLightsOn = (sun.z < 0); if(turnLightsOn != lightsOn) { lightsOn = turnLightsOn; llSetPrimitiveParams([ PRIM_FULLBRIGHT, ALL_SIDES, lightsOn ]); }}</lsl>
Notizen
AVERAGE_SUN_TILT = -.25 * pi SEASONAL_SUN_TILT = .03 * pi SUN_NORMALIZED_OFFSET = .45
So wird mSunOffset berechnet: <cpp>F64 daily_phase = DAILY_OMEGA * U64_to_F64(local_time / USEC_PER_SEC); F32 sun_phase = (F32)fmod(daily_phase, 2.0*F_PI); sun_hour -= 6.0f; mSunOffset = HOURS_TO_RADIANS * sun_hour - (0.25f * F_PI) * cosf(HOURS_TO_RADIANS * sun_hour) - sun_phase;
//Und hier steht wie die Sonnenrichtung berechnet wird:
void LLRegion::calculateSunInfo(
U64 current_time, LLVector3& directionp, LLVector3& ang_velocityp, F32& sun_phase)
{
U64 local_time = current_time; if(getSunFixed()) { local_time = 0; } // Sun moves (once a day) about a circle that lies on a tilted plane. // The angle of the plane cycles (once a year) a few radians about // some average. // These are F64's, otherwise we get rounding errors over time F64 daily_phase = DAILY_OMEGA * U64_to_F64(local_time / USEC_PER_SEC) + mSunOffset; F64 yearly_phase = YEARLY_OMEGA * U64_to_F64(local_time / USEC_PER_SEC); F32 tilt = AVERAGE_SUN_TILT + SEASONAL_SUN_TILT_AMPLITUDE * (F32)sin(yearly_phase);
sun_phase = (F32)fmod(daily_phase, 2.0*F_PI); // move sun around a circle directionp.setVec((F32)cos(-daily_phase), (F32)sin(-daily_phase), 0.0f); //tilt the circle about X-axis (due east) directionp.rotVec(tilt, 1.0f, 0.0f, 0.0f);
// calculate angular velocity (radians per second) ang_velocityp.setVec(0.0f, 0.0f, (F32)DAILY_OMEGA); ang_velocityp.rotVec((F32)tilt, 1.0f, 0.0f, 0.0f);
// James wanted the night to be shorter than the day. // We can do this by offsetting the center of the sun's orbit in the positive // z-direction and normalizing the new vector. directionp.mV[VZ] += SUN_NORMALIZED_OFFSET; F32 R = directionp.normVec();
// We also need to correct the angular velocity // // V = W % R // V has constant magnitude // As R goes up, W must go down // W and R are always perpendicular // ===> // W *= 1 /
Siehe auch
Funktionen
• | llGetTimeOfDay |