I. Introduction
In the 1.4-GHz frequency band, also known as the L-band, the radiometric brightness temperature (BT) is sensitive to the variations in surface salinity over the oceans. The sensitivity of this frequency makes it highly valuable for monitoring and measuring changes in ocean salinity levels [1], [2]. However, due to the longer wavelength associated with this frequency band, there is a need for improved spatial resolution in the antenna aperture to meet the higher demand. This demand has led to the introduction of the synthetic aperture interferometric radiometer (SAIR), which provides enhanced resolution capabilities [3]. The concept of “aperture synthesis” not only improves spatial resolution but also addresses the limitation of finite aperture in traditional radiometers. This means that it can overcome the challenges posed by the physical size of the antenna, allowing for better data capture and higher quality imaging [4]. The SAIRs use interferometric measurements to operate spatial frequency sampling, also known as visibility sampling, and SAIRs retrieve the BT through Fourier transformation and other algorithms [5]. Microwave imaging radiometer using aperture synthesis (MIRAS), specifically designed for observing sea surface salinity and soil moisture, is an airborne SAIR [6].