0000000000248838
AUTHOR
M. Van Noort
Photospheric response to an ellerman bomb-like event—an analogy of Sunrise/IMaX observations and MHD simulations
S. Danilovic et. al.
Power spectrum of turbulent convection in the solar photosphere
The solar photosphere provides us with a laboratory for understanding turbulence in a layer where the fundamental processes of transport vary rapidly and a strongly superadiabatic region lies very closely to a subadiabatic layer. Our tools for probing the turbulence are high-resolution spectropolarimetric observations such as have recently been obtained with the two balloon-borne SUNRISE missions, and numerical simulations. Our aim is to study photospheric turbulence with the help of Fourier power spectra that we compute from observations and simulations. We also attempt to explain some properties of the photospheric overshooting flow with the help of its governing equations and simulations…
A tale of two emergences: Sunrise II observations of emergence sites in a solar active region
R. Centeno et. al.
Oscillations on Width and Intensity of Slender Ca ii H Fibrils from Sunrise/SuFI
R. Gafeira et. al.
The Second Flight of the Sunrise Balloon-borne Solar Observatory: Overview of Instrument Updates, the Flight, the Data, and First Results
S. K. Solanki et. al.
Morphological Properties of Slender Ca ${\rm{II}}$ H Fibrils Observed by Sunrise II
R. Gafeira et. al.
Transverse Oscillations in Slender Ca II H Fibrils Observed with Sunrise/SuFI
S. Jafarzadeh et. al.
A new MHD-assisted Stokes inversion technique
©2017 The American Astronomical Society. All rights reserved. We present a new method of Stokes inversion of spectropolarimetric data and evaluate it by taking the example of a Sunrise/IMaX observation. An archive of synthetic Stokes profiles is obtained by the spectral synthesis of state-of-the-art magnetohydrodynamics (MHD) simulations and a realistic degradation to the level of the observed data. The definition of a merit function allows the archive to be searched for the synthetic Stokes profiles that best match the observed profiles. In contrast to traditional Stokes inversion codes, which solve the Unno–Rachkovsky equations for the polarized radiative transfer numerically and fit the …
Solar Coronal Loops Associated with Small-scale Mixed Polarity Surface Magnetic Fields
L. P. Chitta et. al.
Slender Ca II H fibrils mapping magnetic fields in the low solar chromosphere
S. Jafarzadeh et. al.
Spectropolarimetric evidence for a siphon flow along an emerging magnetic flux tube
©2017 The American Astronomical Society. All rights reserved.We study the dynamics and topology of an emerging magnetic flux concentration using high spatial resolution spectropolarimetric data acquired with the Imaging Magnetograph eXperiment on board the sunrise balloon-borne solar observatory. We obtain the full vector magnetic field and the line of sight (LOS) velocity through inversions of the Fe i line at 525.02 nm with the SPINOR code. The derived vector magnetic field is used to trace magnetic field lines. Two magnetic flux concentrations with different polarities and LOS velocities are found to be connected by a group of arch-shaped magnetic field lines. The positive polarity footp…
Maximum Entropy Limit of Small-scale Magnetic Field Fluctuations in the Quiet Sun
The observed magnetic field on the solar surface is characterized by a very complex spatial and temporal behavior. Although feature-tracking algorithms have allowed us to deepen our understanding of this behavior, subjectivity plays an important role in the identification and tracking of such features. In this paper, we continue studies Gorobets, A. Y., Borrero, J. M., & Berdyugina, S. 2016, ApJL, 825, L18 of the temporal stochasticity of the magnetic field on the solar surface without relying either on the concept of magnetic features or on subjective assumptions about their identification and interaction. We propose a data analysis method to quantify fluctuations of the line-of-sight …
Kinematics of Magnetic Bright Features in the Solar Photosphere
S. Jafarzadeh et. al.