Abstract
Abstract The formation of the temporal spectrum of scintillations is considered for electromagnetic waves propagating in a moving continuous random medium with wave turbulence. The relative contributions of the motion of the medium and turbulent wave propagation to the transformation of the spatial spectrum into a temporal one are discussed. Some results obtained from radio occultation by solar wind plasma at small solar elongations are used for choosing a suitable model for wave turbulence.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
