Abstract:We have developed an active ground-based technique to estimate the steady state field-aligned anomalous electric field (E*) in the topside ionosphere, up to~600 km, using the European Incoherent Scatter (EISCAT) ionospheric modification facility and UHF incoherent scatter radar. When pumping the ionosphere with high-power high-frequency radio waves, the F region electron temperature is significantly raised, increasing the plasma pressure gradient in the topside ionosphere, resulting in ion upflow along the mag… Show more
“…In our experiment, the F region electron temperature is raised up to 3,000 K, and the current density reaches 0.02 μA/m 2 . This value is smaller but of the same order as the downward current density observed by Kosch et al () (0.06 μA/m 2 ) during the ionospheric modification experiments performed in the auroral latitudes. Kosch et al () suggested the mechanism for anomalous resistivity due to low‐frequency ion acoustic waves generated by the pump‐induced flux of suprathermal electrons, which are produced near the pump wave reflection altitude by plasma resonance and also result in artificially induced optical emissions.…”
Section: Interpretation Of the Observational Resultssupporting
confidence: 62%
“…This value is smaller but of the same order as the downward current density observed by Kosch et al () (0.06 μA/m 2 ) during the ionospheric modification experiments performed in the auroral latitudes. Kosch et al () suggested the mechanism for anomalous resistivity due to low‐frequency ion acoustic waves generated by the pump‐induced flux of suprathermal electrons, which are produced near the pump wave reflection altitude by plasma resonance and also result in artificially induced optical emissions. During the SURA heating experiment reported here, the SWARM satellite discovers a more complex signature, implying generation of eddy electric currents, which are likely associated with another physical mechanism, namely, unipolar diffusion with the formation of eddy currents.…”
Section: Interpretation Of the Observational Resultssupporting
A series of experiments were conducted with a conjunction between the midlatitude SURA ionospheric heating facility and the multisatellite SWARM mission. We present the first observations made by SWARM on the plasma perturbations and electric currents induced in the F2 region ionosphere by the high‐power high‐frequency O‐mode radio wave pumping. In the heated region, significant effects include a localized increase of the electron temperature accompanied by stratification of the electron density and the magnetic signatures of field‐aligned currents (FACs). The spatial structure and amplitude of FACs indicate that the current system is likely associated with the unipolar diffusion and excitation of eddy electric currents in the ionosphere. Similar effects are revealed in the laboratory experiment but not previously observed in space.
“…In our experiment, the F region electron temperature is raised up to 3,000 K, and the current density reaches 0.02 μA/m 2 . This value is smaller but of the same order as the downward current density observed by Kosch et al () (0.06 μA/m 2 ) during the ionospheric modification experiments performed in the auroral latitudes. Kosch et al () suggested the mechanism for anomalous resistivity due to low‐frequency ion acoustic waves generated by the pump‐induced flux of suprathermal electrons, which are produced near the pump wave reflection altitude by plasma resonance and also result in artificially induced optical emissions.…”
Section: Interpretation Of the Observational Resultssupporting
confidence: 62%
“…This value is smaller but of the same order as the downward current density observed by Kosch et al () (0.06 μA/m 2 ) during the ionospheric modification experiments performed in the auroral latitudes. Kosch et al () suggested the mechanism for anomalous resistivity due to low‐frequency ion acoustic waves generated by the pump‐induced flux of suprathermal electrons, which are produced near the pump wave reflection altitude by plasma resonance and also result in artificially induced optical emissions. During the SURA heating experiment reported here, the SWARM satellite discovers a more complex signature, implying generation of eddy electric currents, which are likely associated with another physical mechanism, namely, unipolar diffusion with the formation of eddy currents.…”
Section: Interpretation Of the Observational Resultssupporting
A series of experiments were conducted with a conjunction between the midlatitude SURA ionospheric heating facility and the multisatellite SWARM mission. We present the first observations made by SWARM on the plasma perturbations and electric currents induced in the F2 region ionosphere by the high‐power high‐frequency O‐mode radio wave pumping. In the heated region, significant effects include a localized increase of the electron temperature accompanied by stratification of the electron density and the magnetic signatures of field‐aligned currents (FACs). The spatial structure and amplitude of FACs indicate that the current system is likely associated with the unipolar diffusion and excitation of eddy electric currents in the ionosphere. Similar effects are revealed in the laboratory experiment but not previously observed in space.
“…The procedure for obtaining the spectra is the same as described by 249 Blagoveshchenskaya et al (2014). possible to make such a comparison between two heater pulses of different durations obtained 255 from two different experiments under different background conditions.…”
Section: Experiments On 28 October 2013 216mentioning
Abstract. We present experimental results concentrating on a variety of phenomena in 1 the high latitude ionosphere F2 layer induced by an extraordinary (X-mode) HF pump wave at 2 high heater frequencies (fH = 6.2 -8.0 MHz), depending on the pump frequency proximity to the 3 ordinary and extraordinary mode critical frequencies, foF2 and fxF2. The experiments were 4 carried out at the EISCAT HF heating facility with an effective radiated power of in October 2012 and October -November 2013. Their distinctive feature is a wide diapason of 6 critical frequency changes, when the fH /foF2 ratio was varied through a wide range from 0.9 to 7 1.35. It provides both a proper comparison of X-mode HF-induced phenomena excited under 8 different ratios of fH /foF2 and an estimation of the frequency range above foF2 in which such X-9 mode phenomena are still possible. It was shown that the HF-enhanced ion and plasma lines are 10 excited above foF2 when the HF pump frequency is lying in a range between the foF2 and fxF2, 11 foF2 ≤ fH ≤ fxF2, whereas small-scale field-aligned irregularities continued to be generated even 12 when fH exceeded fxF2 by up to 1 MHz and an X-polarized pump wave cannot be reflected from 13 the ionosphere. Another parameter of importance is the magnetic zenith effect (HF beam/radar 14 angle direction) which is typical for X-mode phenomena under fH /foF2 >1 as well as fH / foF2≤ 15 1. We have shown for the first time that an X-mode HF pump wave is able to generate strong 16 narrow band spectral components in the SEE spectra (within 1 kHz of pump frequency) in the 17 ionosphere F region, which were recorded far away from the HF heating facility. The observed 18 spectral lines can be associated with the ion acoustic, electrostatic ion cyclotron, and electrostatic 19 ion cyclotron harmonic waves (otherwise known as neutralized ion Bernstein waves). It is 20 suggested that these spectral components can be attributed to the stimulated Brillion scatter 21 (SBS) process. The comparison between the O-and X-mode narrow band spectra clearly 22 demonstrated that only an X-polarized pump wave scattered by SBS can propagate more than 23 one thousand km without significant deterioration. 24 25
“…However, the SAMI2 simulations with moderate peak heating rates up to 5000 K/s do not explain the fast appearance of artificial ducts and O + ion outflows in the topside ionosphere. Kosch et al [2010;2014b] have shown that in order to match the observations of the HFinduced ion outflows from the EISCAT UHF ISR, a 1-2 µV/m downward electric field is needed in addition to the electron pressure gradient. The latter, however, does not explain the fast timescale as the average upward speed does not exceed ~0.5 km/s.…”
Section: Numerical Modeling Of Artificial Ductsmentioning
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