Description
Solar cooking uses solar thermal or photovoltaic energy to achieve temperatures from 70 °C for slow‑cooking to 300 °C for searing, enabling efficient protein denaturation and Maillard browning while drastically reducing fossil‑fuel emissions.
Technical
During solar cooking, proteins unfold and aggregate at 60–80 °C, while Maillard browning reactions between reducing sugars and amino acids occur at 140–165 °C, producing melanoidins that impart flavor and color. At 170–180 °C caramelization of sugars begins, generating volatile compounds that contribute to aroma. The high temperatures also drive moisture loss, concentrating flavors and reducing microbial load.
Science
Primary Reaction
Protein denaturation, Maillard browning, caramelization
Sensory Profile
Aroma ()