On fibrils and field lines: The nature of H fibrils in the solar chromosphere
arXiv:1502.00295 · doi:10.1088/0004-637X/802/2/136
Abstract
Observations of the solar chromosphere in the line-core of the \Halpha\ line show dark elongated structures called fibrils that show swaying motion. We performed a 3D radiation-MHD simulation of a network region, and computed synthetic \Halpha\ images from this simulation to investigate the relation between fibrils and the magnetic field lines in the chromosphere. The periods, amplitudes and phase-speeds of the synthetic fibrils are consistent with those observed. We analyse the relation between the synthetic fibrils and the field lines threading through them, and find that some fibrils trace out the same field line along the fibril's length, but there are also fibrils that sample different field lines at different locations along their length. Fibrils sample the same field lines on a time scale of ~s. This is shorter than their own lifetime. We analysed the evolution of the atmosphere along a number of field lines that thread through fibrils and find that they carry slow-mode waves that load mass into the field line, as well as transverse waves that propagate with the Alfvén speed. Transverse waves propagating in opposite directions cause an interference pattern with complex apparent phase speeds. The relationship between fibrils and field lines is complex. It is governed by constant migration and swaying of the field lines, their mass loading by slow modes and subsequent draining, and their actual visibility in \Halpha. Field lines are visible where they lie close to the optical depth unity surface. The location of the latter is governed by the height at which the column mass in the chromosphere reaches a certain value. We conclude that using the swaying motion of fibrils as a tracer of chromospheric transverse oscillations must be done with caution.
arXiv commentAccepted for publication in ApJ. Abstract shortened because of astro-ph's character limit. A PDF with full-resolution figures and the associated movies are available for download at http://folk.uio.no/jorritl/fibrils_fieldlines/fibrils_fieldlines.tar.gz
References in corpus (26)
- The stellar atmosphere simulation code Bifrost
- CRISP Spectropolarimetric Imaging of Penumbral Fine Structure
- Time-Distance Seismology of the Solar Corona with CoMP
- The formation of the Halpha line in the solar chromosphere
- Dynamic Fibrils are driven by Magnetoacoustic Shocks
- High Resolution Observations and Modeling of Dynamic Fibrils
- CRISPRED: A data pipeline for the CRISP imaging spectropolarimeter
- The formation of IRIS diagnostics II. The formation of the Mg II h&k lines in the solar atmosphere
- Ubiquitous torsional motions in type II spicules
- Solar fine-scale structures. I. Spicules and other small-scale, jet-like events at the chromospheric level: observations and physical parameters
- Solar Oscillations and Convection: II. Excitation of Radial Oscillations
- The formation of IRIS diagnostics I. A quintessential model atom of Mg II and general formation properties of the Mg II h&k lines
- The formation of IRIS diagnostics. III. Near-ultraviolet Spectra and Images
- Magnetoacoustic shocks as driver of quiet Sun mottles
- Evidence for the photospheric excitation of incompressible chromospheric waves
- Transverse oscillations in chromospheric mottles
- Transverse oscillations of loops with coronal rain observed by Hinode/SOT
- Are solar chromospheric fibrils tracing the magnetic field?
- On-disk coronal rain
- The generation and damping of propagating MHD kink waves in the solar atmosphere
- Can We Improve the Preprocessing of Photospheric Vector Magnetograms by the Inclusion of Chromospheric Observations?
- Short dynamic fibrils in sunspot chromospheres
- Characteristics of transverse waves in chromospheric mottles
- DOT Tomography of the Solar Atmosphere VII. Chromospheric Response to Acoustic Events
- The Hanle effect of Ly in an MHD model of the Solar Transition Region
- Helical motion of magnetic flux tubes in the solar atmosphere
Cited by in corpus (51)
- A publicly available simulation of an enhanced network region of the Sun
- Radiative diagnostics in the solar photosphere and chromosphere
- Spectropolarimetric capabilities of Ca II 8542 A line
- H-alpha features with hot onsets. I. Ellerman bombs
- Transverse Oscillations in Slender Ca II H Fibrils Observed with Sunrise/SuFI
- Real-time multiframe blind deconvolution of solar images
- Inference of the chromospheric magnetic field orientation in the Ca II 8542 A line fibrils
- Slender Ca II H Fibrils Mapping Magnetic Fields in the Low Solar Chromosphere
- Three-dimensional modeling of chromospheric spectral lines in a simulated active region
- Forced field extrapolation of the magnetic structure of the Halpha fibrils in solar chromosphere
- Casting the Coronal Magnetic Field Reconstruction Tools in 3D Using MHD Bifrost Model
- Millimeter radiation from a 3D model of the solar atmosphere II. Chromospheric magnetic field
- H-alpha features with hot onsets III. Fibrils in Lyman-alpha and with ALMA
- Chromospheric polarimetry through multi-line observations of the 850 nm spectral region
- Self-consistent 3D radiative MHD simulations of coronal rain formation and evolution
- Stirring the Base of the Solar Wind: On Heat Transfer and Vortex Formation
- A comparative study of two X2.2 and X9.3 solar flares observed with HARPS-N: Reconciling Sun-as-a-star spectroscopy and high-spatial resolution solar observations in the context of the solar-stellar connection
- Tracing the Chromospheric and Coronal Magnetic Field with AIA, IRIS, IBIS, and ROSA Data
- Solar polarimetry through the K I lines at 770 nm
- Measurements of Photospheric and Chromospheric Magnetic Field Structures Associated with Chromospheric Heating over a Solar Plage Region
- Physical properties of bright Ca II K fibrils in the solar chromosphere
- Automated Spatiotemporal Analysis of Fibrils and Coronal Rain using the Rolling Hough Transform
- Active region chromospheric magnetic fields
- Force-Free Field Reconstructions Enhanced by Chromospheric Magnetic Field Data
- The Gaia-ESO survey: Hydrogen lines in red giants directly trace stellar mass
- Dynamics of internetwork chromospheric fibrils: Basic properties and MHD kink waves
- Transverse motions in sunspot super-penumbral fibrils
- Multi-wavelength Study of Transition Region Penumbral Subarcsecond Bright Dots Using IRIS and NST
- Three-dimensional magnetic field structure of a flux emerging region in the solar atmosphere
- Influence of NLTE effects in Fe I lines on inverted atmosphere II. 6301 A and 6302 A lines formed in 3DNLTE
- Tracing Halpha Fibrils through Bayesian Deep Learning
- Small-scale solar jet formation and their associated waves and instabilities
- Disentangling flows in the solar transition region
- Identifying and Tracking Solar Magnetic Flux Elements with Deep Learning
- Chromospheric observations and magnetic configuration of a supergranular structure
- Magnetohydrostatic modeling of AR11768 based on a SUNRISE/IMaX vector magnetogram
- Small-scale loops heated to transition region temperatures and their chromospheric signatures in the simulated solar atmosphere
- Excitation and evolution of coronal oscillations in self-consistent 3D radiative MHD simulations of the solar atmosphere
- SunnyNet: A neural network approach to 3D non-LTE radiative transfer
- Unveiling the True Nature of Plasma Dynamics from the Reference Frame of a Super-penumbral Fibril
- The magnetic topology of the inverse Evershed flow
- The formation and heating of chromospheric fibrils in a radiation-MHD simulation
- Magnetic field extrapolation in active region well comparable with observations in multiple layers
- Probing chromospheric fine structures with a Hα proxy using MURaM-ChE
- Rapid Blue- and Red-shifted Excursions in H line profiles synthesized from realistic 3D MHD simulations
- Temperature diagnostics of chromospheric fibrils
- Tracing the evolution of radiation-MHD simulations of solar and stellar atmospheres in the Lagrangrian frame
- The Sun at millimeter wavelengths IV. Magnetohydrodynamic waves in small-scale bright features
- Damping of coronal oscillations in self-consistent 3D radiative MHD simulations of the solar atmosphere
- Transverse oscillations in 3D along Ca II K bright fibrils in the solar chromosphere
- On the formation of Lyman and the O I 1027 and 1028 Å spectral lines