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- W1552851457 abstract "When low frequency terrestrial radio waves are observed far from their source, in the remote magnetospheric tail or in the solar wind, strong frequency-dependent variations of their apparent source direction and/or angular size are observed. For instance, far in the tail, the Non Thermal Continuum (NTC) source appears nearly isotropic at the lowest frequencies. An observer located in the solar wind, at ≃ 03:00 LT, 200 R E from Earth sees the Auroral Kilometric Radiation (AKR) source away from the Earth's direction, the farther tailward, the lower the frequency. A similar phenomenon is observed from the Lagrange point: the AKR source appears to move to large angular distances away from the Earth's direction as the observing frequency decreases. In all these cases, large scale propagation effects (refraction and scattering) are most probably at work. These effects will be described and discussed. They are controlled by density structures. Their deconvolution is not easy but it can provide a way to remotely sound the electron density in the magnetosheath and the bow shock." @default.
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- W1552851457 date "2000-01-01" @default.
- W1552851457 modified "2023-09-25" @default.
- W1552851457 title "Radio wave propagation in the Earth's magnetosphere" @default.
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- W1552851457 doi "https://doi.org/10.1029/gm119p0075" @default.
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