On the multi-threaded nature of solar spicules
H. Skogsrud, L. Rouppe van der Voort, B. De Pontieu

TL;DR
This study reveals the multi-threaded and torsional dynamics of solar spicules using high-resolution observations, showing asymmetric spectra and internal sub-structures that suggest complex flows and motions in the chromosphere.
Contribution
It provides new evidence of the multi-threaded and asymmetric spectral features of spicules, highlighting their complex internal dynamics and torsional components.
Findings
Many spicules display asymmetric spectra with multiple peaks.
Average velocity difference between components is 20-30 km/s.
Spectral tilts indicate complex internal motions within spicules.
Abstract
A dominant constituent in the dynamic chromosphere are spicules. Spicules at the limb appear as relatively small and dynamic jets that are observed to everywhere stick out. Many papers emphasize the important role spicules might play in the energy and mass balance of the chromosphere and corona. However, many aspects of spicules remain a mystery. In this Letter we shed more light on the multi-threaded nature of spicules and their torsional component. We use high spatial, spectral and temporal resolution observations from the Swedish 1-m Solar Telescope in the H{\alpha} spectral line. The data targets the limb and we extract spectra from spicules far out from the limb to reduce the line-of-sight superposition effect. We discover that many spicules display very asymmetric spectra with some even showing multiple peaks. To quantify this asymmetry we use a double Gaussian fitting procedure…
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