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- W990572124 abstract "This chapter discusses concepts related to scintillation measurements. Radio sources having angular diameters less than about 1 arc sec show fluctuations of intensity, having a time scale of a few seconds, when observed within 90° of the Sun. The fluctuations are produced by scattering of the radiation from irregularities of plasma density in interplanetary space, and the phenomenon is known as interplanetary scintillation. In addition, fluctuations of intensity of the radiation from pulsars, having a time scale of a number of minutes, result from a similar mechanism operating in the interstellar medium, which is known as interstellar scintillation. Observations of the intensity fluctuations have proved useful in determining the electron density variations and scales of the plasma irregularities producing the scintillation. Enhancements of interplanetary scintillation have been correlated with the presence of sector structure in the solar wind. The chapter outlines the diffraction effects, which occur when radiation traverses an extended medium containing randomly distributed phase-changing irregularities. It analyzes diffraction by thin layers and presents an overview of interplanetary scintillation and radio source structure." @default.
- W990572124 created "2016-06-24" @default.
- W990572124 creator A5075869792 @default.
- W990572124 date "1976-01-01" @default.
- W990572124 modified "2023-09-27" @default.
- W990572124 title "4.7. Scintillation Measurements" @default.
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- W990572124 doi "https://doi.org/10.1016/s0076-695x(08)60706-1" @default.
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