Lecture
This lecture covers the physics behind solar race design, focusing on the sensible and latent heat properties of buildings, geometric projections, and the movement of the sun relative to Earth. It explains the construction of solar races at different latitudes, the use of stereographic projections, and the impact of solar height on building orientation. The presentation delves into the effects of solar movement on facade illumination, shadow casting by vertical and horizontal elements, and the efficiency of sun protection strategies. It also discusses the importance of horizontal and vertical elements in providing effective solar protection in different hemispheres.