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Magnetic Field Enhancement of an Electromechanical-Magnetic Antenna for ELF Cross-Medium Communication via a Parallel Configuration. [PDF]
Leung CM, Chen H, Liu M.
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Formation of high-aspect-ratio nanocavity in LiF crystal using a femtosecond X-ray free-electron laser pulse. [PDF]
Makarov SS +32 more
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ULF Waves Observed by Lunar Prospector
Journal of Geophysical Research: Space Physics, 2021AbstractWe have studied the spatial distribution of ultra‐low frequency (ULF) in the vicinity of the Moon using Lunar Prospector (LP) magnetometer data obtained at ∼100 km altitude during the period from February 20, 1998 to November 30, 1998. The lunar ULF waves are mostly identified over a broad frequency range of 10–60 mHz in the spacecraft frame ...
Seul‐Min Baek +4 more
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Ionospheric Feedback and ULF Quarter‐Waves
Journal of Geophysical Research: Space Physics, 2022AbstractThis paper presents results from the numerical investigation of nonlinear feedback interactions between ULF field‐aligned currents (FACs) and the ionospheric plasma in the global magnetospheric resonator with a non‐symmetrical distribution of the plasma density in the conjugate hemispheres.
Anatoly V. Streltsov, Evgeny V. Mishin
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ULF Waves: Conjugated Ground-Satellite Relationships
Space Science Reviews, 1978We study the simultaneous occurrence of ULF waves observed on board GEOS and at two of its ‘conjugated’ stations: Husafell (Iceland) and Skibotn (Norway). We try to deduce some properties of the regions in which these waves are generated. The few number of simultaneous observations of ‘pearl’ events indicates that such structured oscillations can occur
Roger Gendrin +4 more
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A study of ULF wave foreshock morphology—II: spatial variation of ULF waves
Planetary and Space Science, 1992Abstract Two case studies are used to show the evolution of upstream ULF waves in the Earth's foreshock region. During these two intervals the IMF cone angle was nearly constant over an extended time period and the ISEE spacecraft was in the foreshock region and traveled a large distance through it.
G. Le, C.T. Russell
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Advances in Space Research, 1995
Plasma waves observed in the VLF range upstream of planetary bow shocks not only modify the particle distributions, but also provide important information about the acceleration processes that occur at the bow shock. Electron plasma oscillations observed near the tangent field line in the electron foreshock are generated by electrons reflected at the ...
E.W Greenstadt, G Le, R.J Strangeway
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Plasma waves observed in the VLF range upstream of planetary bow shocks not only modify the particle distributions, but also provide important information about the acceleration processes that occur at the bow shock. Electron plasma oscillations observed near the tangent field line in the electron foreshock are generated by electrons reflected at the ...
E.W Greenstadt, G Le, R.J Strangeway
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