Spectropolarimetric investigation of magnetohydrodynamic wave modes in the photosphere: First results from PHI on board Solar Orbiter
arXiv:2304.14155 · doi:10.1051/0004-6361/202245826
Abstract
In November 2021, Solar Orbiter started its nominal mission phase. The remote-sensing instruments on board the spacecraft acquired scientific data during three observing windows surrounding the perihelion of the first orbit of this phase. The aim of the analysis is the detection of magnetohydrodynamic (MHD) wave modes in an active region by exploiting the capabilities of spectropolarimetric measurements. The High Resolution Telescope (HRT) of the Polarimetric and Helioseismic Imager (SO/PHI) on board the Solar Orbiter acquired a high-cadence data set of an active region. This is studied in the paper. B- and phase-difference analyses are applied on line-of-sight velocity and circular polarization maps and other averaged quantities. We find that several MHD modes at different frequencies are excited in all analysed structures. The leading sunspot shows a linear dependence of the phase lag on the angle between the magnetic field and the line of sight of the observer in its penumbra. The magnetic pore exhibits global resonances at several frequencies, which are also excited by different wave modes. The SO/PHI measurements clearly confirm the presence of magnetic and velocity oscillations that are compatible with one or more MHD wave modes in pores and a sunspot. Improvements in modelling are still necessary to interpret the relation between the fluctuations of different diagnostics.
References in corpus (23)
- The Solar Orbiter mission -- Science overview
- The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Overview and Performance
- Coronal heating by MHD waves
- Multiwavelength studies of MHD waves in the solar chromosphere: An overview of recent results
- Inversion of the radiative transfer equation for polarized light
- The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action
- Structure and Dynamics of Isolated Internetwork Ca II H Bright Points Observed by Sunrise
- The usefulness of analytic response functions
- 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
- High-frequency Oscillations in Small Magnetic Elements Observed with Sunrise/SuFI
- An Inside Look at Sunspot Oscillations with Higher Azimuthal Wavenumbers
- Alfvenic Perturbations in a Sunspot Chromosphere Linked to Fractionated Plasma in the Corona
- Internal Gravity Waves in the Magnetized Solar Atmosphere. I. Magnetic Field Effects
- The Propagation of Coherent Waves Across Multiple Solar Magnetic Pores
- A novel approach to identify resonant MHD wave modes in solar pores and sunspot umbrae: analysis
- The small-scale structure of photospheric convection retrieved by a deconvolution technique applied to Hinode/SP data
- Accuracy analysis of the on-board data reduction pipeline for the Polarimetric and Helioseismic Imager on the Solar Orbiter mission
- The non-LTE formation of the Fe I 6173 A line in the solar atmosphere
- Magnetic fields inferred by Solar Orbiter: A comparison between SO/PHI-HRT and SDO/HMI
- On the Origin of Magnetic Pertubations associated with the FIP effect
- Plasma composition measurements in an active region from Solar Orbiter/SPICE and Hinode/EIS
- The ratio of horizontal to vertical displacement in solar oscillations estimated from combined SO/PHI and SDO/HMI observations
Cited by in corpus (5)
- Wavefront error of PHI/HRT on Solar Orbiter at various heliocentric distances
- Sausage, kink, and fluting MHD wave modes identified in solar magnetic pores by Solar Orbiter/PHI
- Stereoscopic disambiguation of vector magnetograms: first applications to SO/PHI-HRT data
- Data-constrained 3D MHD Simulation of a Spiral Jet Caused by an Unstable Flux Rope Embedded in Fan-spine Configuration
- Solar photospheric velocities measured in space: a comparison between SO/PHI-HRT and SDO/HMI