Pojava magle na moru uzduž američko-pacifičke obale je često povezana s premještanjem istočno-pacifičke anticiklone na kopno. U tom slučaju prisutno je višednevno zagrijavanje kopna i razvoj »vruće kaplje« (»hot spell«) te vjetrova koji pušu s kopna na more neposredno prije pojave magle. Cilj ove studije je modeliranje stvaranja i razvoja magle na moru kao posljedice interakcije vrućeg i suhog vjetra s kopna i hladnog i vlažnog maritimnog graničnog sloja. Simulacije potvrđuju izloženi temeljni teorijski model formiranja i razvoja magle nad morem koji je temeljen na fizikalnim procesima u kojima vjetrovi s kopna spuštaju maritimnu inverziju neposredno do morske površine. Usprkos advekciji suhog i toplog zraka, magla nad morem nastaje u plitkom površinskom sloju koji je zatvoren s gornje strane s inverzijom od 10 °C(K) ili više te slojem vrućeg zraka iznad inverzije. Prije formiranja magle na moru, negativni površinski senzibilni fluks topline uzrokuje hlađenje i kondenzaciju dok latentni toplinski fluks doprinosi povećanju vlage i turbulencije u površinskom sloju. Suhoća toplog sloja zraka nad maritimnim slojem uzrokuje pojačano dugovalno radijacijsko ohlađivanje na vrhu maritimnog sloja i pospješava kondenzaciju. Isprva se formira tanki oblak koji se ubrzano razvija prema površini mora te se pretvara u maglu nad morem. Čim se magla formira, radijacijsko ohlađivanje gornje granice stvara turbulentna gibanja i razvoj magle kao sloj miješanja. Uslijed radijacijskog ohlađivanja, magla postaje u početku hladnija od površine. U kasnijoj fazi razvoja magle, stalno miješanje hladnog i vlažnog maritimnog zraka s toplim i suhim slojem iznad inverzije ograničava turbulentno miješanje. Uslijed toga podiže se visina kondenzacijskog nivoa te dolazi do razbijanja magle ili njezine transformacije u stratus. The occurrence of sea fog along the U.S. Pacific Coast in summer is frequently associated with the movement of a high pressure system from the eastern Pacific to the land. Subsequently there is strong heating of the land over several days or more and development of »hot spells« and offshore flows in the coastal region preceding sea fog formation. This study focuses on modeling the formation and evolution of sea fog in response to interaction between the warm and dry offshore flows and the cool and moist marine atmospheric boundary layer. Simulation results support a conceptual model of fog formation and evolution based on physical processes initiated by offshore flows that efficiently lower the marine inversion near the sea surface. In spite of the warm and dry advection, fog formed in the shallow, near-surface marine layer capped by a strong temperature inversion of 10 °C or more and a hot-air layer above the inversion. Prior to sea fog formation, negative surface heat flux initiates cooling and condensation, while the surface moisture flux contributes to increased humidity and turbulence within the surface layer. The dryness of the hot-air layer overlying the shallow and moist marine layer triggers enhanced radiative cooling at the marine layer top and facilitates the marine layer’s saturation. The thin cloud forms, rapidly propagates downward, and transforms into fog. As soon as the fog is formed, longwave radiative cooling at its top generates turbulent mixing and the growth of the fog as a mixed layer. Due to the fog-top radiative cooling, the fog layer is initially colder than the underlying surface. In the later stage of the fog evolution, continuous mixing of the cool and moist near-surface air with the dry and warm layer above the inversion during the fog growth generally curtails turbulence. This process elevates the lifting condensation level and can lead to sea fog dissipation or generation of stratus.