1997
DOI: 10.1007/s00585-997-0878-4
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Propagation and dispersion of electrostatic waves in the ionospheric E region

Abstract: Abstract. Low-frequency electrostatic¯uctuations in the ionospheric E region were detected by instruments on the ROSE rockets. The phase velocity and dispersion of plasma waves in the ionospheric E region are determined by band-pass ®ltering and cross-correlating data of the electric-®eld¯uctuations detected by the probes on the ROSE F4 rocket. The results were con®rmed by a dierent method of analysis of the same data. The results show that the waves propagate in the Hall-current direction with a velocity some… Show more

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Cited by 11 publications
(25 citation statements)
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“…4, the increase in T e is expected to be minute, but for the somewhat larger down-leg fields, E 0 ≈60-70 mV/m, nontrivial enhancements of T e are anticipated, but not observed for the present conditions. The wave propagation velocities, for instance, as found by Iranpour et al (1997), Krane et al (2000) and Dyrud et al (2006) are best explained by an electron temperature of approximately 400 K. Also other reports (Pfaff et al, 1992) noted the lack of electron temperature enhancements for conditions similar to ours. A previous study (Dyrud et al, 2006) attempted to explain the low electron temperatures by thermal conduction to the colder regions below the enhanced wave activity, but used too low numerical values for the electron energy loss per collision, by taking this energy loss to be at most an order of magnitude larger than for inelastic collisions.…”
Section: Numerical Simulationssupporting
confidence: 84%
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“…4, the increase in T e is expected to be minute, but for the somewhat larger down-leg fields, E 0 ≈60-70 mV/m, nontrivial enhancements of T e are anticipated, but not observed for the present conditions. The wave propagation velocities, for instance, as found by Iranpour et al (1997), Krane et al (2000) and Dyrud et al (2006) are best explained by an electron temperature of approximately 400 K. Also other reports (Pfaff et al, 1992) noted the lack of electron temperature enhancements for conditions similar to ours. A previous study (Dyrud et al, 2006) attempted to explain the low electron temperatures by thermal conduction to the colder regions below the enhanced wave activity, but used too low numerical values for the electron energy loss per collision, by taking this energy loss to be at most an order of magnitude larger than for inelastic collisions.…”
Section: Numerical Simulationssupporting
confidence: 84%
“…U 6 and U 2 being small, these two difference signals referring to probe-sets perpendicular to the rocket axis. For the small time separations relevant for the present analysis we do not find significant differences between signals such as U 6 and U 5 either, but note that the correlation times for these signals are somewhat different (Iranpour et al, 1997;Krane et al, 2000).…”
Section: Analysis Of Rocket Datamentioning
confidence: 51%
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“…Values for positive spectral indices have been reported by Prakash et al (1971), but these apply only to some unspecified narrow spectral subranges and they are not included in the present summary. Some rocket experiments (Pécseli et al, 1989Iranpour et al, 1997) report E region turbulent spectra in a colour-coded version, where a spectral index is not readily determined with any significant accuracy. Within the uncertainty, the results do not, however, in contradiction with similar data in Table 2.…”
Section: Space Observationsmentioning
confidence: 99%
“…We can see from (14) that the phase velocities of these waves are smaller than the ion-acoustic velocity and since the growth rate for these waves is maximal their amplitudes must be maximal. Iranpour et al [3], analyzing rocket measurements of ionospheric waves during the ROSE project [6], found low-velocity waves with large amplitudes. Phase velocities of the waves increase with increasing frequency.…”
Section: Ion-acoustic Instabilitymentioning
confidence: 99%