Abstract
A method of recording internal gravitational waves (IGWs) from spacecraft by observing disturbances in the atmospheric emission layer, formed in the vicinity of the solar terminator and emitted in the atmospheric molecular oxygen system (762 ± 5 nm), is considered. The possibility of such observations and the efficiency of recording various characteristics of IGWs passing through the observed emission layer are estimated.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have