Results 1 to 10 of about 192,436 (221)
Interaction of Radio Waves [PDF]
Nature, 1934 PRIOR to the observation of the interaction of radio waves1, the study of the propagation of such waves through the atmosphere was concerned only with the effect of the ionosphere on them. The converse effect, namely, the influence of electric waves on the ionosphere, has already been considered by us in a theory of radio interaction2.
V. A. Bailey, D. F. Martyn
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“Velocity of Light and of Radio Waves” [PDF]
Nature, 1950 I SHOULD like to direct attention to the fact that in my article on the velocity of light and of radio waves1 the result announced by Houstoun2 was unfortunately omitted. It had not been published when my article was prepared, but could have been inserted had I noticed it in time.
L. Essen
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THE PRODUCTION OF DAMPED RADIO‐WAVES [PDF]
School Science and Mathematics, 1920 n ...
William Schrieyer
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Simulations of radio-wave anisotropic scattering to interpret type III radio bursts measurements by Solar Orbiter, Parker Solar Probe, STEREO and Wind [PDF]
A&A 656, A34 (2021), 2021 We use multi-spacecraft observations of invididual type III radio bursts in order to calculate the directivity of the radio emission, to be compared to the results of ray-tracing simulations of the radio-wave propagation and probe the plasma properties of the inner heliosphere.
arxiv +1 more source
Radio-Wave Communication With Chaos [PDF]
IEEE Access, 2020 6 pages 8 ...
Chao Bai +3 more
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Large scale simulations of solar type III radio bursts: flux density, drift rate, duration and bandwidth [PDF]
A&A 572, A111 (2014), 2014 Non-thermal electrons accelerated in the solar corona can produce intense coherent radio emission, known as solar type III radio bursts. This intense radio emission is often observed from hundreds of MHz in the corona down to the tens of kHz range in interplanetary space.
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On the Formation of Cluster Radio Relics [PDF]
Mon.Not.Roy.Astron.Soc. 331 (2002) 1011, 2001 (abridged) We present detailed 3-dimensional magneto-hydrodynamical simulations of the passage of a radio plasma cocoon filled with turbulent magnetic fields through a shock wave. Taking into account synchrotron, inverse Compton and adiabatic energy losses and gains we evolved the relativistic electron population to produce synthetic polarisation radio
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Forward Modeling of the Type III Radio Burst Exciter [PDF]
Sol Phys (2019) 294: 62, 2019 In this work, we propose a forward-modeling method to study the trajectory and speed of the interplanetary (IP) Type-III radio burst exciter. The model assumes that the source of an IP Type-III radio burst moves outward from the Sun following the Parker spiral field line.
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Nature of microstructure in pulsar radio emission [PDF]
Mon.Not.Roy.Astron.Soc. 327 (2001) 984, 2000 We present a model for microstructure in pulsar radio emission. We propose that micropulses result from the alteration of the radio wave generation region by nearly transverse drift waves propagating across the pulsar magnetic field and encircling the bundle of the open magnetic field lines.
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Scattering of ultrastrong electromagnetic waves by magnetized particles [PDF]
, 2021 Observations of powerful radio waves from neutron star magnetospheres raise the question of how strong waves interact with particles in a strong background magnetic field $B_{bg}$. This problem is examined by solving the particle motion in the wave.
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