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Open AccessJournal ArticleDOI

Transverse Wave Induced Kelvin-Helmholtz Rolls in Spicules

TLDR
In this article, the role of transverse MHD waves and associated instabilities in spicule-like features was analyzed and it was shown that transverse wave induced TWIKH rolls lead to coherence of strand-like structure in imaging and spectral maps, as seen in some observations.
Abstract
In addition to their jet-like dynamic behavior, spicules usually exhibit strong transverse speeds, multi-stranded structure, and heating from chromospheric to transition region temperatures. In this work we first analyze Hinode and IRIS observations of spicules and find different behaviors in terms of their Doppler velocity evolution and collective motion of their sub-structure. Some have a Doppler shift sign change that is rather fixed along the spicule axis, and lack coherence in the oscillatory motion of strand-like structure, matching rotation models, or long-wavelength torsional Alfven waves. Others exhibit a Doppler shift sign change at maximum displacement and coherent motion of their strands, suggesting a collective magnetohydrodynamic (MHD) wave. By comparing with an idealized 3D MHD simulation combined with radiative transfer modeling, we analyze the role of transverse MHD waves and associated instabilities in spicule-like features. We find that transverse wave induced Kelvin–Helmholtz (TWIKH) rolls lead to coherence of strand-like structure in imaging and spectral maps, as seen in some observations. The rapid transverse dynamics and the density and temperature gradients at the spicule boundary lead to ring-shaped Mg ii k and Ca ii H source functions in the transverse cross-section, potentially allowing IRIS to capture the Kelvin–Helmholtz instability dynamics. Twists and currents propagate along the spicule at Alfvenic speeds, and the temperature variations within TWIKH rolls, produce the sudden appearance/disappearance of strands seen in Doppler velocity and in Ca ii H intensity. However, only a mild intensity increase in higher-temperature lines is obtained, suggesting there is an additional heating mechanism at work in spicules.

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Citations
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Alfven Waves in the Solar Corona

TL;DR: An estimate of the energy carried by the waves that are spatially resolved indicates that they are too weak to heat the solar corona; however, unresolved Alfvén waves may carry sufficient energy.
Journal ArticleDOI

Achievements of Hinode in the first eleven years

TL;DR: In this article, an open access article distributed under the terms of the Creative Commons CC BY license, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Journal ArticleDOI

A New View of the Solar Interface Region from the Interface Region Imaging Spectrograph (IRIS)

TL;DR: The Interface Region Imaging Spectrograph (IRIS) has been obtaining near and far-ultraviolet images and spectra of the solar atmosphere since July 2013 and has enabled research into the fundamental physical processes thought to play a role in the low solar atmosphere such as ion-neutral interactions, magnetic reconnection, the generation, propagation, and dissipation of waves, the acceleration of non-thermal particles, and various small-scale instabilities as discussed by the authors.
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Heating Effects from Driven Transverse and Alfvén Waves in Coronal Loops

TL;DR: In this article, the authors show that wave heating effects in coronal loops can be modelled with a mixture of kink and Alfven modes, and that the mixing of the two modes can lead to a more efficient energy dissipation.
References
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Journal ArticleDOI

The Interface Region Imaging Spectrograph (IRIS)

TL;DR: The Interface Region Imaging Spectrograph (IRIS) as mentioned in this paper provides simultaneous spectra and images of the photosphere, chromosphere, transition region, and corona with 0.33 arcsec and up.
Journal ArticleDOI

The Solar Optical Telescope for the Hinode Mission: An Overview

Saku Tsuneta
- 12 Nov 2007 - 
TL;DR: The Solar Optical Telescope (SOT) as mentioned in this paper is a 50 cm diffraction-limited Gregorian telescope, and includes the narrow-band (NFI) and wideband (BFI) filtergraphs.
Journal ArticleDOI

The Interface Region Imaging Spectrograph (IRIS)

TL;DR: The Interface Region Imaging Spectrograph (IRIS) as mentioned in this paper is a small explorer spacecraft that provides simultaneous spectra and images of the photosphere, chromosphere, transition region, and corona with 0.33-0.4 arcsec spatial resolution, 2 s temporal resolution and 1 km/s velocity resolution over a field-of-view of up to 175 arcsec.
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