http://www.igpp.ucla.edu/public/mkivelso/refs/PUBLICATIONS/staciewicz%20AW%202400%20SpaceSciRev.pdf 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.
What happens when the Alfven velocity exceeds light speed
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 … WebDec 12, 2009 · Small-scale structures last less than 10 s and gradually become larger structures. [19] These structures and the time variations observed for brightening auroras … ray whaling obituary
Small Scale Alfv??nic Structure in the Aurora - ResearchGate
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 … 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 … WebApr 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 scales to small Alfvén wave scales of several electron skin depths and less. simply southern bbq in myrtle beach sc