Magneto-seismological insights into the penumbral chromosphere and evidence for wave damping in spicules
arXiv:1405.3203 · doi:10.1051/0004-6361/201423718
Abstract
The observation of propagating magneto-hydrodynamic kink waves in magnetic structures and measurement of their properties (amplitude, phase speed) can be used to diagnose the plasma conditions in the neighbourhood of the magnetic structure via magneto-seismology (MS). We aim to reveal properties of the chromosphere/Transition Region above the sunspot penumbra using this technique. Hinode observed a sunspot as it was crossing the limb, providing a unique side on view of the sunspot atmosphere. The presence of large spicule-like jets is evident in \ion{Ca}{II} H images. The jets are found to support transverse wave motions that displace the central axis, which can be interpreted as a kink wave. The properties of a wave event are measured and used to determine the magnetic and density stratification along the structure. We also measure the width of the spicule and the intensity profile along the structure. The measured wave properties reveal an initial rapid increase in amplitude with height above the solar surface, followed by a decrease in amplitude. The MS inversion suggests this initial increase corresponds to large changes in density and magnetic field strength. In addition, we provide the first measurements of spicule width with height, which confirm that the spicule under goes rapid expansion. The measured expansion shows good agreement with the results from the MS. The observed variations in plasma parameters are suggested to be partly due to the presence of a gravitational stratified, ambient atmosphere. Combining width measurements with phase speed measurements implies the observed decrease in wave amplitude at greater heights can be explained by wave damping. Hence, we provide the first direct evidence of wave damping in chromospheric spicules and the quality factor of the damping is found to be significantly smaller than estimated coronal values.
13 pages, 10 figures - Accepted in A&A
References in corpus (12)
- Observations of ubiquitous compressive waves in the Sun's chromosphere
- Analytic approximate seismology of transversely oscillating coronal loops
- Point spread functions for the Solar Optical Telescope onboard Hinode
- The generation and damping of propagating MHD kink waves in the solar atmosphere
- Hi-C & AIA observations of transverse MHD waves in active regions
- A statistical study of transverse oscillations in a quiescent prominence
- Characteristics of transverse waves in chromospheric mottles
- The Ly-alpha profile and center-to-limb variation of the quiet Sun
- Solar transition region above sunspots
- Hydrogen Lyman-alpha and Lyman-beta spectral radiance profiles in the quiet Sun
- Calibrating Data from the Hinode/X-Ray Telescope and Associated Uncertainties
- Solar Magnetic Carpet III: Coronal Modelling of Synthetic Magnetograms
Cited by in corpus (13)
- Wave Heating of the Solar Atmosphere
- Waves in the lower solar atmosphere: the dawn of next-generation solar telescopes
- Transverse Oscillations in Slender Ca II H Fibrils Observed with Sunrise/SuFI
- Overdamped Alfven waves due to ion-neutral collisions in the solar chromosphere
- Forward Modelling of Standing Kink Modes in Coronal Loops I. Synthetic Views
- MHD wave modes resolved in fine-scale chromospheric magnetic structures
- Dynamics of internetwork chromospheric fibrils: Basic properties and MHD kink waves
- An overall view of temperature oscillations in the solar chromosphere with ALMA
- Transverse motions in sunspot super-penumbral fibrils
- Possible Evolution of Minifilament-Eruption-Produced Solar Coronal Jets, Jetlets, and Spicules, into Magnetic-Twist-Wave "Switchbacks" Observed by the Parker Solar Probe (PSP)
- Propagating Kink Waves in an Open Coronal Magnetic Flux Tube with Gravitational Stratification: Magnetohydrodynamic Simulation and Forward Modelling
- Semi-empirical models of spicule from inversion of Ca II 8542 Å line
- Model fitting of kink waves in the solar atmosphere: Gaussian damping and time-dependence