Results 171 to 180 of about 4,735 (200)

Ohm's Law, the Reconnection Rate, and Energy Conversion in Collisionless Magnetic Reconnection. [PDF]

Space Sci Rev
Liu YH, Hesse M, Genestreti K, Nakamura R, Burch JL, Cassak PA, Bessho N, Eastwood JP, Phan T, Swisdak M, Toledo-Redondo S, Hoshino M, Norgren C, Ji H, Nakamura TKM.   +14 more
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Section 7. Magnetospheric Radio Emissions

Section 7. Magnetospheric Radio Emissions
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An interpretation of banded magnetospheric radio emissions

Journal of Geophysical Research, 2001
Recently published Active Magnetospheric Particle Tracer Explorers/Ion Release Module (AMPTE/IRM) banded magnetospheric emissions, commonly referred to as “(n + 1/2)fce” emissions, where fce is the electron gyrofrequency, are analyzed by treating them as analogous to sounder‐stimulated ionospheric emissions.
Robert F Benson, J Fainberg
exaly   +2 more sources

Magnetospheric Radio Emissions from Exoplanets with the SKA [PDF]

Proceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14), 2015
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P Zarka, Joseph Lazio, Gregg Hallinan
exaly   +4 more sources

Chaotic Temporal Variability of Magnetospheric Radio Emissions

Space Science Reviews, 2003
Nonthermal magnetospheric radio emissions provide the radio signatures of solar-terrestrial connection and may be used for space weather forecasting. A three-wave model of auroral radio emissions at the fundamental plasma frequency was proposed by (1994) involving resonant interactions of Langmuir, whistler and Alfven waves.
Erico L Rempel, Abraham C -L Chian, F A Borotto   +2 more
exaly   +3 more sources

Numerical simulation of auroral magnetospheric radio emission

2012 37th International Conference on Infrared, Millimeter, and Terahertz Waves, 2012
Simulations have been conducted at the University of Strathclyde to study the electrodynamics of the cyclotron maser instability responsible for generating auroral magnetospheric radio emission from stars and planets with a dipole like magnetic field configuration.
D C Speirs, S L McConville, A D R Phelps   +2 more
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Phenomenology of magnetospheric radio emissions

1983
Jupiter has now been observed over 24 octaves of the radio spectrum, from about 0.01 MHz to 300,000 MHz. Its radio emissions fill the entire spectral region where interplanetary electromagnetic propagation is possible at wavelengths longer than infrared. Three distinct types of radiation are responsible for this radio spectrum.
T. D. Carr, M. D. Desch, J. K. Alexander
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The main source of radio emission from the magnetosphere of Uranus

Journal of Geophysical Research: Space Physics, 1987
Observations of kilometric radiation from Uranus made with the planetary radio astronomy experiment on the Voyager 2 spacecraft are presented and discussed. Similarities between the auroral kilometric radiation from Earth and the observed Uranus emission are pointed out.
S, Gulkis, T D, Carr
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Magnetospheres: Jupiter, Radio Emissions

2004
International ...
Zarka, Philippe, Murdin, P.
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Numerical investigation of auroral magnetospheric radio emission

2012 Abstracts IEEE International Conference on Plasma Science, 2012
Summary form only given. In recent years, there has been considerable published research and debate on an instability produced within an electron beam transported into an increasing magnetic field. Due to conservation of energy and magnetic moment, a velocity distribution is produced having a significant pitch spread and effective population inversion ...
D. C. Speirs, K. M. Gillespie, S. L. McConville, A. D. R. Phelps, A. W. Cross, K. Ronald, R. Bingham, B. J. Kellett, R. A. Cairns, I. Vorgul   +9 more
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