// First calculates the moon's parrallax, that is, the apparent size of the
// (equatorial) radius of the earth, as seen from the moon
mpar = asin ( 1 / r);
- gclat = FG_Latitude - 0.003358 * sin (2 * DEG_TO_RAD * FG_Latitude);
- rho = 0.99883 + 0.00167 * cos(2 * DEG_TO_RAD * FG_Latitude);
+ gclat = f->get_Latitude() - 0.003358 *
+ sin (2 * DEG_TO_RAD * f->get_Latitude() );
+ rho = 0.99883 + 0.00167 * cos(2 * DEG_TO_RAD * f->get_Latitude());
if (geoRa < 0)
geoRa += (2*FG_PI);
// Rotate to proper orientation
// printf(" lon = %.2f lat = %.2f\n", FG_Longitude * RAD_TO_DEG,
// FG_Latitude * RAD_TO_DEG);
- xglRotatef( FG_Longitude * RAD_TO_DEG, 0.0, 0.0, 1.0 );
- xglRotatef( 90.0 - FG_Latitude * RAD_TO_DEG, 0.0, 1.0, 0.0 );
+ xglRotatef( f->get_Longitude() * RAD_TO_DEG, 0.0, 0.0, 1.0 );
+ xglRotatef( 90.0 - f->get_Latitude() * RAD_TO_DEG, 0.0, 1.0, 0.0 );
xglRotatef( l->sun_rotation * RAD_TO_DEG, 0.0, 0.0, 1.0 );
// Draw inner/center section of sky*/
// $Log$
+// Revision 1.15 1998/12/03 01:15:36 curt
+// Converted fgFLIGHT to a class.
+// Tweaks for Sun portability.
+//
// Revision 1.14 1998/11/06 21:17:39 curt
// Converted to new logstream debugging facility. This allows release
// builds with no messages at all (and no performance impact) by using