The Planetary Fourier Spectrometer (PFS) is an instrument designed for the analysis of planetary atmospheres. It utilizes Fourier transform spectroscopy principles to measure the infrared spectra of planetary atmospheres and surfaces. The PFS can capture a wide range of wavelengths simultaneously, making it efficient in detecting various molecular signatures present in the atmosphere, such as gases and particles.
Articles by others on the same topic
There are currently no matching articles.