Convective blueshifts in the solar atmosphere II. High-accuracy observations of the Fe i 6173.3Å line and deviations of full-disk Dopplergrams
arXiv:1811.08685 · doi:10.1051/0004-6361/201834538
Abstract
Granular convective motions reach into the lower solar atmosphere, typically causing photospheric spectral lines to exhibit a differential line shift. This Doppler shift to shorter wavelength is commonly known as convective blueshift. We performed systematic observations of the quiet Sun with the Laser Absolute Reference Spectrograph (LARS) at the German Vacuum Tower Telescope. The solar disk was scanned along the meridian and the equator, from the disk center toward the limb. The solar spectrum around 6173Å was calibrated with a laser frequency comb on an absolute wavelength scale with an accuracy of a few m/s. We applied a bisector analysis on the spectral lines to reveal the changes of convective blueshift and line asymmetry at different heliocentric positions. Being a signature for convective motions, the bisector curve of Fe i 6173.3Å describes a C-shape at disk center. When approaching the solar limb, the bisector transforms into a \-shape. The analysis of the time- and bisector-averaged line shifts yields three distinct results. Firstly, the center-to-limb variation of Doppler velocities measured with LARS reveals a significant discrepancy (up to 200m/s) to the full-disk Dopplergrams of the Helioseismic and Magnetic Imager (HMI). Secondly, we obtained a significant decrease of convective blueshift toward the solar limb. Thirdly, the line-of-sight effect of solar activity leads to a scatter of up to 100m/s at intermediate heliocentric positions. The accurate observation of the absolute convective blueshift with LARS allows the identification of systematic discrepancy with Doppler velocities measured by HMI. The center-to-limb variation of HMI suffers from an additional blueshift toward the limb that is incompatible with our results. LARS measurements can be taken as reference for the correction of systematic errors in the synoptic HMI Dopplergrams.
arXiv comment9 pages, 9 figures
References in corpus (5)
- Solar velocity references from 3D HD photospheric models
- Convective blueshifts in the solar atmosphere, I. Absolute measurements with LARS of the spectral lines at 6302 Å
- Correlations between sunspots and their moat flows
- Achieving Consistent Doppler Measurements from SDO/HMI Vector Field Inversions
- LARS - An Absolute Reference Spectrograph for solar observations, Upgrade from a prototype to a turn-key system
Cited by in corpus (11)
- Observational constraints on the origin of the elements II. 3D non-LTE formation of Ba ii lines in the solar atmosphere
- Convective blueshifts in the solar atmosphere: III. High-accuracy observations of spectral lines in the visible
- The IAG spectral atlas of the spatially resolved Sun: Centre-to-limb observations
- SOAP-GPU: Efficient Spectral Modelling of Stellar Activity Using Graphical Processing Units
- A Machine Learning approach for correcting radial velocities using physical observables
- Spatially resolved spectroscopy across stellar surfaces. IV. F, G, & K-stars: Synthetic 3D spectra at hyper-high resolution
- How rare are counter Evershed flows?
- GRASS II: Simulations of Potential Granulation Noise Mitigation Methods
- Newly formed downflow lanes in exploding granules in the solar photosphere
- Average solar active region: I. Intensities, velocities, and the photospheric magnetic field
- Solar photospheric velocities measured in space: a comparison between SO/PHI-HRT and SDO/HMI