Faraday rotation in Jupiter's decametric radio emission used for remote sensing of the terrestrial ionosphere and the emission's source region at Jupiter

1995 ◽  
Vol 43 (12) ◽  
pp. 1595-1605 ◽  
Author(s):  
H.P. Ladreiter ◽  
G. Litvinenko ◽  
M.Y. Boudjada ◽  
H.O. Rucker
Keyword(s):  
Remote Sensing ◽  
Radio Emission ◽  
Faraday Rotation ◽  
Source Region

scholarly journals Numerical simulations of unbounded cyclotron-maser emissions

2013 ◽  
Vol 79 (6) ◽  
pp. 999-1001 ◽  
Author(s):  
DAVID C. SPEIRS ◽  
S. L. McCONVILLE ◽  
K. M. GILLESPIE ◽  
A. D. R. PHELPS ◽  
K. RONALD
Keyword(s):  
Radio Emission ◽  
Numerical Simulations ◽  
Source Region ◽  
Radio Emissions ◽  
Cyclotron Maser ◽  
Thermal Radio ◽  
Thermal Radio Emission ◽  
Electron Cyclotron Masers ◽  
Coupling Characteristics ◽  
Significant Bearing

AbstractNumerical simulations have been conducted to study the spatial growth rate and emission topology of the cyclotron-maser instability responsible for stellar/planetary auroral magnetospheric radio emission and intense non-thermal radio emission in other astrophysical contexts. These simulations were carried out in an unconstrained geometry, so that the conditions existing within the source region of some natural electron cyclotron masers could be more closely modelled. The results have significant bearing on the radiation propagation and coupling characteristics within the source region of such non-thermal radio emissions.

scholarly journals The Influence of Antenna Pattern on Faraday Rotation in Remote Sensing at L-Band

2007 ◽  
Vol 45 (9) ◽  
pp. 2737-2746 ◽  
Author(s):  
D.M. Le Vine ◽  
S.D. Jacob ◽  
E.P. Dinnat ◽  
P. de Matthaeis ◽  
S. Abraham
Keyword(s):  
Remote Sensing ◽  
Faraday Rotation ◽  
Antenna Pattern ◽  
L Band

scholarly journals Pulse Emission Mechanisms

2004 ◽  
Vol 218 ◽  
pp. 349-356 ◽  
Author(s):  
Don Melrose
Keyword(s):  
Radio Emission ◽  
Source Region ◽  
High Energy ◽  
Pair Creation ◽  
Emission Mechanism ◽  
Pulse Emission ◽  
Energy Emission ◽  
High Energy Emission

High-energy and radio emission mechanisms for pulsars are reviewed. The source region for high energy emission remains uncertain. Two preferred radio emission mechanism are identified. Some difficulties may be resolved by appealing to nonstationary pair creation distributed widely in height.

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