Waves with harmonic structure below and above the lower hybrid resonance observed on the CENTAUR 35.001 and 35.002 rockets

1986 ◽  
Vol 64 (10) ◽  
pp. 1437-1445 ◽  
Author(s):  
T. Neubert ◽  
G. Holmgren ◽  
E. Ungstrup ◽  
K. Melgård

Measurements obtained from the 0- to 10-kHz electric-wave experiment and the 0- to 4.2-kHz electron-density fluctuation experiment on the CENTAUR 35.001 and 35.002 rockets launched in December 1981 are presented. The observations include (i) spectacular narrow-banded signals with harmonic structure related to the proton gyrofrequency. The bands are observed both below and above the lower hybrid frequency, from 2 to 10 kHz, and are modulated in frequency during a rocket spin, typically by 2 kHz. The character of the signals indicate that they are generated by the presence of the payload in the plasma. The source of free energy remains unidentified; we suggest, however, a perpendicular ion beam emitted by or created by the presence of the payload, generating flute-mode ion cyclotron harmonic waves. (ii) Bursts of harmonic waves are received primarily below 2 kHz. The fundamental frequency of these emissions varies over a large range, from 47 to 700 Hz, and is rarely at any of the characteristic frequencies of the plasma. (iii) Waves with a clear lower cutoff at the lower hybrid frequency are also observed. The lower hybrid frequency estimated from magnetic field and density measurements and from the wave measurements agree within 6% (500 Hz).

1986 ◽  
Vol 29 (4) ◽  
pp. 1087 ◽  
Author(s):  
Toshitaka Idehara ◽  
Naoyoshi Tomita

2001 ◽  
Vol 19 (2) ◽  
pp. 147-157 ◽  
Author(s):  
F. Jiřiček ◽  
D. R. Shklyar ◽  
P. Třiska

Abstract. VLF-ELF broadband measurements onboard the MAGION 4 and 5 satellites at heights above 1 Re in plasmasphere provide new data on various known phenomena related to ducted and nonducted whistler wave propagation. Two examples are discussed: magnetospherically reflected (MR) whistlers and lower hybrid resonance (LHR) noise band. We present examples of rather complicated MR whistler spectrograms not reported previously and argue the conditions for their generation. Analytical consideration, together with numerical modelling, yield understanding of the main features of those spectrograms. LHR noise band, as well as MR whistlers, is a phenomenon whose source is the energy propagating in the nonducted way. At the plasmaspheric heights, where hydrogen (H+) is the prevailing ion, and electron plasma frequency is much larger than gyrofrequency, the LHR frequency is close to its maximumvalue in a given magnetic field. This frequency is well followed by the observed noise bands. The lower cutoff frequency of this band is somewhat below that maximum value. The reason for this, as well as the possibility of using the LHR noise bands for locating the plasma through position, are discussed.Key words. Magnetospheric physics (plasmasphere; wave propagation)


Author(s):  
Sandeep R. Sainkar ◽  
Alice N. Cheeran ◽  
Gajendrakumar Shinde ◽  
Promod K. Sharma ◽  
Harish V. Dixit

1976 ◽  
Vol 16 (3) ◽  
pp. 419-426 ◽  
Author(s):  
R.J. Hawryluk ◽  
S.L. Davis ◽  
J.A. Schmidt

1979 ◽  
Vol 67 (1) ◽  
pp. 170-171
Author(s):  
A. Hoyano ◽  
S. Ohnuki ◽  
S. Adachi ◽  
T. Ohnuma

1974 ◽  
Vol 14 (1) ◽  
pp. 19-23 ◽  
Author(s):  
Y. Satya ◽  
A. Sen ◽  
P. Kaw

1998 ◽  
Vol 38 (5) ◽  
pp. 661-671 ◽  
Author(s):  
E.V Suvorov ◽  
E Holzhauer ◽  
W Kasparek ◽  
A.B Burov ◽  
Y.A Dryagin ◽  
...  

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