// tmp.cxx -- stuff I don't know what to do with at the moment // // Written by Curtis Olson, started July 2000. // // Copyright (C) 2000 Curtis L. Olson - http://www.flightgear.org/~curt // // This program is free software; you can redistribute it and/or // modify it under the terms of the GNU General Public License as // published by the Free Software Foundation; either version 2 of the // License, or (at your option) any later version. // // This program is distributed in the hope that it will be useful, but // WITHOUT ANY WARRANTY; without even the implied warranty of // MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU // General Public License for more details. // // You should have received a copy of the GNU General Public License // along with this program; if not, write to the Free Software // Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA. // // $Id$ #ifdef HAVE_CONFIG_H # include #endif #include #include #include #include #include #include #include #include
#include
#include
#include #include "light.hxx" #include "sunsolver.hxx" #include "tmp.hxx" // periodic time updater wrapper void fgUpdateLocalTime() { static const SGPropertyNode *longitude = fgGetNode("/position/longitude-deg"); static const SGPropertyNode *latitude = fgGetNode("/position/latitude-deg"); SGPath zone( globals->get_fg_root() ); zone.append( "Timezone" ); SG_LOG(SG_GENERAL, SG_INFO, "updateLocal(" << longitude->getDoubleValue() * SGD_DEGREES_TO_RADIANS << ", " << latitude->getDoubleValue() * SGD_DEGREES_TO_RADIANS << ", " << zone.str() << ")"); globals->get_time_params()->updateLocal( longitude->getDoubleValue() * SGD_DEGREES_TO_RADIANS, latitude->getDoubleValue() * SGD_DEGREES_TO_RADIANS, zone.str() ); } // update the cur_time_params structure with the current sun position void fgUpdateSunPos( void ) { sgVec3 nup, nsun; Point3D rel_sunpos; double dot, east_dot; double sun_gd_lat, sl_radius; // vector in cartesian coordinates from current position to the // postion on the earth's surface the sun is directly over sgVec3 to_sun; // surface direction to go to head towards sun sgVec3 surface_to_sun; FGLight *l = (FGLight *)(globals->get_subsystem("lighting")); SGTime *t = globals->get_time_params(); FGViewer *v = globals->get_current_view(); SG_LOG( SG_EVENT, SG_DEBUG, " Updating Sun position" ); SG_LOG( SG_EVENT, SG_DEBUG, " Gst = " << t->getGst() ); double sun_l; fgSunPositionGST(t->getGst(), &sun_l, &sun_gd_lat); l->set_sun_lon(sun_l); sgGeodToGeoc(sun_gd_lat, 0.0, &sl_radius, &sun_l); l->set_sun_gc_lat(sun_l); Point3D p = Point3D( l->get_sun_lon(), l->get_sun_gc_lat(), sl_radius ); l->set_sunpos( sgPolarToCart3d(p) ); SG_LOG( SG_EVENT, SG_DEBUG, " t->cur_time = " << t->get_cur_time() ); SG_LOG( SG_EVENT, SG_DEBUG, " Sun Geodetic lat = " << sun_gd_lat << " Geocentric lat = " << l->get_sun_gc_lat() ); // update the sun light vector sgSetVec4( l->sun_vec(), l->get_sunpos().x(), l->get_sunpos().y(), l->get_sunpos().z(), 0.0 ); sgNormalizeVec4( l->sun_vec() ); sgCopyVec4( l->sun_vec_inv(), l->sun_vec() ); sgNegateVec4( l->sun_vec_inv() ); // make sure these are directional light sources only l->sun_vec()[3] = l->sun_vec_inv()[3] = 0.0; // cout << " l->sun_vec = " << l->sun_vec[0] << "," << l->sun_vec[1] // << ","<< l->sun_vec[2] << endl; // calculate the sun's relative angle to local up sgCopyVec3( nup, v->get_world_up() ); sgSetVec3( nsun, l->get_sunpos().x(), l->get_sunpos().y(), l->get_sunpos().z() ); sgNormalizeVec3(nup); sgNormalizeVec3(nsun); // cout << "nup = " << nup[0] << "," << nup[1] << "," // << nup[2] << endl; // cout << "nsun = " << nsun[0] << "," << nsun[1] << "," // << nsun[2] << endl; l->set_sun_angle( acos( sgScalarProductVec3 ( nup, nsun ) ) ); SG_LOG( SG_EVENT, SG_DEBUG, "sun angle relative to current location = " << l->get_sun_angle() ); // calculate vector to sun's position on the earth's surface Point3D vp( v->get_view_pos()[0], v->get_view_pos()[1], v->get_view_pos()[2] ); rel_sunpos = l->get_sunpos() - (vp + globals->get_scenery()->get_center()); sgSetVec3( to_sun, rel_sunpos.x(), rel_sunpos.y(), rel_sunpos.z() ); // printf( "Vector to sun = %.2f %.2f %.2f\n", // v->to_sun[0], v->to_sun[1], v->to_sun[2]); // Given a vector from the view position to the point on the // earth's surface the sun is directly over, map into onto the // local plane representing "horizontal". sgmap_vec_onto_cur_surface_plane( v->get_world_up(), v->get_view_pos(), to_sun, surface_to_sun ); sgNormalizeVec3(surface_to_sun); // cout << "(sg) Surface direction to sun is " // << surface_to_sun[0] << "," // << surface_to_sun[1] << "," // << surface_to_sun[2] << endl; // cout << "Should be close to zero = " // << sgScalarProductVec3(nup, surface_to_sun) << endl; // calculate the angle between surface_to_sun and // v->get_surface_east(). We do this so we can sort out the // acos() ambiguity. I wish I could think of a more efficient // way. :-( east_dot = sgScalarProductVec3( surface_to_sun, v->get_surface_east() ); // cout << " East dot product = " << east_dot << endl; // calculate the angle between v->surface_to_sun and // v->surface_south. this is how much we have to rotate the sky // for it to align with the sun dot = sgScalarProductVec3( surface_to_sun, v->get_surface_south() ); // cout << " Dot product = " << dot << endl; if (dot > 1.0) { SG_LOG( SG_ASTRO, SG_INFO, "Dot product = " << dot << " is greater than 1.0" ); dot = 1.0; } else if (dot < -1.0) { SG_LOG( SG_ASTRO, SG_INFO, "Dot product = " << dot << " is less than -1.0" ); dot = -1.0; } if ( east_dot >= 0 ) { l->set_sun_rotation( acos(dot) ); } else { l->set_sun_rotation( -acos(dot) ); } // cout << " Sky needs to rotate = " << angle << " rads = " // << angle * SGD_RADIANS_TO_DEGREES << " degrees." << endl; }