Resonance of a wire antenna near the lower hybrid frequency in an RF-generated magnetoplasma

1979 ◽  
Vol 67 (1) ◽  
pp. 170-171
Author(s):  
A. Hoyano ◽  
S. Ohnuki ◽  
S. Adachi ◽  
T. Ohnuma
Keyword(s):  
Wire Antenna ◽  
Lower Hybrid ◽  
Hybrid Frequency

Practical Considerations for the CW Power Amplifier Design for Lower Hybrid Frequency Applications

2020 ◽  
Author(s):  
Sandeep R. Sainkar ◽  
Alice N. Cheeran ◽  
Gajendrakumar Shinde ◽  
Promod K. Sharma ◽  
Harish V. Dixit
Keyword(s):  
Power Amplifier ◽  
Lower Hybrid ◽  
Hybrid Frequency ◽  
Amplifier Design

scholarly journals RF-heating near the lower hybrid frequency in the FM-1 spherator

1976 ◽  
Vol 16 (3) ◽  
pp. 419-426 ◽  
Author(s):  
R.J. Hawryluk ◽  
S.L. Davis ◽  
J.A. Schmidt
Keyword(s):  
Lower Hybrid ◽  
Rf Heating ◽  
Hybrid Frequency

Anomalous plasma heating at lower hybrid frequency

1974 ◽  
Vol 14 (1) ◽  
pp. 19-23 ◽  
Author(s):  
Y. Satya ◽  
A. Sen ◽  
P. Kaw
Keyword(s):  
Plasma Heating ◽  
Lower Hybrid ◽  
Hybrid Frequency

scholarly journals Observations of lower hybrid cavities in the inner magnetosphere by the Cluster and Viking satellites

2004 ◽  
Vol 22 (8) ◽  
pp. 2961-2972 ◽  
Author(s):  
A. Tjulin ◽  
M. André ◽  
A. I. Eriksson ◽  
M. Maksimovic
Keyword(s):  
Time Scales ◽  
Sounding Rocket ◽  
Lower Hybrid ◽  
High Altitudes ◽  
Frequency Range ◽  
General Shape ◽  
Lower Altitude ◽  
Inner Magnetosphere ◽  
Hybrid Frequency ◽  
The Individual

Abstract. Observations by the Viking and Cluster satellites at altitudes up to 35000km show that Lower Hybrid Cavities (LHCs) are common in the inner magnetosphere. LHCs are density depletions filled with waves in the lower hybrid frequency range. The LHCs have, until recently, only been found at altitudes up to 2000km. Statistics of the locations and general shape of the LHCs is performed to obtain an overview of some of their properties. In total, we have observed 166 LHCs on Viking during 27h of data, and 535 LHCs on Cluster during 87h of data. These LHCs are found at invariant latitudes from the auroral region to the plasmapause. A comparison with lower altitude observations shows that the LHC occurrence frequency does not scale with the flux tube radius, so that the LHCs are moderately rarer at high altitudes. This indicates that the individual LHCs do not reach from the ionosphere to 35000km altitude, which gives an upper bound for their length. The width of the LHCs perpendicular to the geomagnetic field at high altitudes is a few times the ion gyroradius, consistent with observations at low altitudes. The estimated depth of the density depletions vary with altitude, being larger at altitudes of 20000-35000km (Cluster, 10-20%), smaller around 1500-13000km (Viking and previous Freja results, a few percent) and again larger around 1000km (previous sounding rocket observations, 10-20%). The LHCs in the inner magnetosphere are situated in regions with background electrostatic hiss in the lower hybrid frequency range, consistent with investigations at low altitudes. Individual LHCs observed at high altitudes are stable at least on time scales of 0.2s (about the ion gyro period), which is consistent with previous results at lower altitudes, and observations by the four Cluster satellites show that the occurrence of LHCs in a region in space is a stable phenomenon, at least on time scales of an hour.

scholarly journals Excitation of fast waves by slow waves near the lower-hybrid frequency

1976 ◽  
Vol 19 (9) ◽  
pp. 1392 ◽  
Author(s):  
R. L. Berger ◽  
Liu Chen
Keyword(s):  
Slow Waves ◽  
Lower Hybrid ◽  
Hybrid Frequency ◽  
Fast Waves
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