SummaryThe spatial and temporal variations of the energy and moisture budgets of a megalopolis (Los Angeles basin) were examined during a frontal passage February 23, 1969) and during an extremely clear day (March 4, 1969) in order to determine the existing continuum of possible extremes during that season. The distributional aspects of solar radiation (direct and diffuse), reflected solar radiation, net radiation, latent heat flux, sensible heat flux, and heat flux in or out of the urban interface were examined. Budgets of input and output of the storm study were contrasted with those of the clear day study. Also measured and compared were actual surface temperatures, terrain radiant temperatures, radiant sky temperatures, and dry and wet-bulb temperatures. Especially in the case of the clear day investigation, a series of empirical and physical-theoretical models were tested and proved to be rather realistic in comparison with actual observations in the field. Such models were less successful during the storm when the city surface received extremely low amounts of energy. Especially striking were the multitude of energy processes and their probable causes during the storm. The frontal passage caused a reduction of 92 ~ of the absorbed solar radiation as compared to the clear day. Infrared components of the budget were much less affected.