Weak kinetic Alfvén waves turbulence during the 14 November 2012 geomagnetic storm: Van Allen Probes observations

In the dawn sector, L ∼ 5.5 and MLT ∼ 4–7, from 01:30 to 06:00 UT during the 14 November 2012 geomagnetic storm, both Van Allen Probes observed an alternating sequence of locally quiet and disturbed intervals with two strikingly different power fluctuation levels and magnetic field orientations: eit...

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Veröffentlicht in:Journal of geophysical research. Space physics 2015-07, Vol.120 (7), p.5504-5523
Hauptverfasser: Moya, Pablo. S., Pinto, Víctor A., Viñas, Adolfo F., Sibeck, David G., Kurth, William S., Hospodarsky, George B., Wygant, John R.
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container_end_page 5523
container_issue 7
container_start_page 5504
container_title Journal of geophysical research. Space physics
container_volume 120
creator Moya, Pablo. S.
Pinto, Víctor A.
Viñas, Adolfo F.
Sibeck, David G.
Kurth, William S.
Hospodarsky, George B.
Wygant, John R.
description In the dawn sector, L ∼ 5.5 and MLT ∼ 4–7, from 01:30 to 06:00 UT during the 14 November 2012 geomagnetic storm, both Van Allen Probes observed an alternating sequence of locally quiet and disturbed intervals with two strikingly different power fluctuation levels and magnetic field orientations: either small (∼10−2 nT2) total power with strong GSM Bx and weak By or large (∼10 nT2) total power with weak Bx and strong By and Bz components. During both kinds of intervals the fluctuations occur in the vicinity of the local ion gyrofrequencies (0.01–10 Hz) in the spacecraft frame, propagate oblique to the magnetic field, (θ ∼ 60∘), and have magnetic compressibility C=|δB∥|/|δB⊥|∼1, where δB∥ (δB⊥) are the average amplitudes of the fluctuations parallel (perpendicular) to the mean field. Electric field fluctuations are present whenever the magnetic field is disturbed, and large electric field fluctuations follow the same pattern for quiet and disturbed intervals. Magnetic frequency power spectra at both spacecraft correspond to steep power laws ∼f−α with 4 < α < 5 for f≲2 Hz, and 1.1 < α < 1.7 for f≳ 2 Hz, spectral profiles that are consistent with weak kinetic Alfvén wave (KAW) turbulence. Electric power is larger than magnetic power for all frequencies above 0.1 Hz, and the ratio increases with increasing frequency. Vlasov linear analysis is consistent with the presence of compressive KAW with k⊥ρi≲1, right‐handed polarization and positive magnetic helicity, in the plasma frame, considering a multiion plasma. All these results suggest the presence of weak KAW turbulence which dissipates the energy associated with the intermittent sudden changes in the magnetic field during the main phase of the storm. Key Points Observation of striking magnetic fluctuations during the 14 November 2012 magnetic storm Spectral analysis suggests the presence of kinetic Alfvén waves turbulence The interpretation is consistent with Vlasov linear theory analysis
doi_str_mv 10.1002/2014JA020281
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Electric field fluctuations are present whenever the magnetic field is disturbed, and large electric field fluctuations follow the same pattern for quiet and disturbed intervals. Magnetic frequency power spectra at both spacecraft correspond to steep power laws ∼f−α with 4 &lt; α &lt; 5 for f≲2 Hz, and 1.1 &lt; α &lt; 1.7 for f≳ 2 Hz, spectral profiles that are consistent with weak kinetic Alfvén wave (KAW) turbulence. Electric power is larger than magnetic power for all frequencies above 0.1 Hz, and the ratio increases with increasing frequency. Vlasov linear analysis is consistent with the presence of compressive KAW with k⊥ρi≲1, right‐handed polarization and positive magnetic helicity, in the plasma frame, considering a multiion plasma. All these results suggest the presence of weak KAW turbulence which dissipates the energy associated with the intermittent sudden changes in the magnetic field during the main phase of the storm. 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Vlasov linear analysis is consistent with the presence of compressive KAW with k⊥ρi≲1, right‐handed polarization and positive magnetic helicity, in the plasma frame, considering a multiion plasma. All these results suggest the presence of weak KAW turbulence which dissipates the energy associated with the intermittent sudden changes in the magnetic field during the main phase of the storm. Key Points Observation of striking magnetic fluctuations during the 14 November 2012 magnetic storm Spectral analysis suggests the presence of kinetic Alfvén waves turbulence The interpretation is consistent with Vlasov linear theory analysis</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1002/2014JA020281</doi><tpages>20</tpages></addata></record>
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subjects Computational fluid dynamics
Electric fields
Electric power
Electric power generation
Fluctuation
Fluctuations
Fluid flow
Intervals
kinetic AlfvenAlfvén waves
Magnetic fields
magnetic storms
Probes
radiation belts
Spacecraft
Spectral analysis
Storms
Turbulence
Turbulent flow
Van Allen Probes
title Weak kinetic Alfvén waves turbulence during the 14 November 2012 geomagnetic storm: Van Allen Probes observations
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