Small scale alfvénic structure in the aurora
WebJul 15, 2012 · Scaling index α derived from the slope of logarithmic diagrams (LD) constructed by the discrete wavelet transform of data can be estimated as α = 2.2 ± 0.3, which is close to α estimate earlier reported for scales 1–30 km by electric field observations of the Dynamics Explorer 2 satellite. WebSmall scale Alfvénic structure in the aurora. K Stasiewicz, P Bellan, C Chaston, C Kletzing, R Lysak, J Maggs, ... Space Science Reviews 92, 423-533, 2000. 543: 2000: Electron acceleration in the heart of the Van Allen radiation belts. GD Reeves, HE Spence, MG Henderson, SK Morley, RHW Friedel, ...
Small scale alfvénic structure in the aurora
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WebJul 24, 2024 · Kinetic Alfvén waves (KAWs) are believed to be capable of efficiently transporting energy and play an important role in facilitating magnetic reconnection. KAW eigenmode theory suggests that Hall fields can be considered as the components of KAW, providing a mechanism for the generation and dissipation of KAW in magnetic … http://www.igpp.ucla.edu/public/mkivelso/refs/PUBLICATIONS/staciewicz%20AW%202400%20SpaceSciRev.pdf
WebSep 27, 2005 · Since the aurora has a very similar appearance from the two sites, its altitude extent must be rather small. Knowledge of the altitude of the emissions allows us to estimate the scale sizes of the curls, which are about 1–5 km, with the arc thickness of ≈1 km. Figure 2 Open in figure viewer PowerPoint WebIGPP Home Page
WebThis paper presents a comprehensive review of dispersive Alfvén waves in space and laboratory plasmas. We start with linear properties of Alfvén waves and show how the … WebDec 5, 2008 · Another possibility is raised by Chust et al. [2005] is that small-scale Alfvén waves observed by Galileo may be evidence of a filamentation processes within the torus. Filamentation converts long Alfvénic pulses into small-scale waves which are reflected back to Io and also transmitted Jupiterward.
WebSmall-scale length density cavities have been observed in the auroral zone by Viking and Freja spacecrafts [ 35, 36 ]. For the auroral region, we observed the density fluctuations of ∼0.12 n0, consistent with the FAST observation reported by Chaston et al. [ 14, 15 ].
WebApr 21, 2010 · The small arrows in Figures 2b–2e show results of the application of this procedure to consecutive images of the Alfvénic and quasi-static aurora. These results … dickinson eclipse shotgun reviewWebApr 30, 2008 · Abstract It is demonstrated from observations that the Alfvénic aurora may be powered by a turbulent cascade transverse to the geomagnetic field from large MHD … citric acid price south africaWebApr 13, 2024 · Stasiewicz, K., Bellan, P., Chaston, C., et al., Small scale Alfvénic structure in the aurora, Space Sci. Rev., 2000, vol. 92, pp. 423–533. Article Google Scholar Tam, S.W.Y., Chang, T., Kintner, P.M., and Klatt, E., Intermittency analyses on the SIERRA measurements of the electric field fluctuations in the auroral zone, Geophys. Res. citric acid purity test methodWebA is the Alfvenic time. According to calcula-tions of Lessard and Knudsen (2001), Alfven waves with spatial scales less than a few km are strongly diffused and damped upon the reflection from the realistic ionosphere. There-fore, a possible occurrence in the IAR of small-scale Alfvenic structures with the transverse citric acid raw materialWebMay 7, 2010 · Spatio-temporal evolution of thin Alfven resonance layer - Volume 76 Issue 5 citric acid reaction with calcium carbonateWebThis paper presents a comprehensive review of dispersive Alfvén waves in space and laboratory plasmas. We start with linear properties of Alfvén waves and show how the inclusion of ion gyroradius, parallel electron inertia, and finite frequency effects modify the Alfvén wave properties. dickinson electricity providersWebJul 23, 2009 · Some recent observations of solar corona suggest that the kinetic Alfvén waves (KAWs) turbulence may be responsible for electron acceleration in solar corona and coronal heating. In the present research, we investigate the turbulent spectra of KAW due to filamentation process in the presence of Landau damping and particle energization. citric acid schädlich