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Magnetic Flux Emergence and its Interaction with AN Existing Coronal FieldGalsgaard, K. et al.112005
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Magnetic Flux Emergence and its Interaction with AN Existing Coronal Field
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Galsgaard, K. et al.Fecha de publicación:
112005 -
Magnetic flux emergence into the solar photosphere and chromosphere
Aims: We model the emergence of magnetized plasma across granular convection cells and the low atmosphere, including layers up to the mid-chromosphere. Methods: Three-dimensional numerical experiments are carried out in which the equations of MHD and radiative transfer are solved self-consistently. We use the MURaM code, which assumes local
Tortosa-Andreu, A. et al.Fecha de publicación:
112009 -
Magnetic Loops in the Quiet Sun
We investigate the fine structure of magnetic fields in the atmosphere of the quiet Sun. We use photospheric magnetic field measurements from SUNRISE/IMaX with unprecedented spatial resolution to extrapolate the photospheric magnetic field into higher layers of the solar atmosphere with the help of potential and force-free extrapolation techniques
Wiegelmann, T. et al.Fecha de publicación:
112010 -
Magneto-acoustic wave energy in sunspots: observations and numerical simulations
We have reproduced some sunspot wave signatures obtained from spectropolarimetric observations through 3D MHD numericalsimulations. The results of the simulations arecompared with the oscillations observed simultaneously at different heights from the SiI lambda10827Å line, HeI lambda10830Å line, the CaII H core and the FeI blends at the wings of
Felipe, T. et al.Fecha de publicación:
112011 -
Mapping diffuse interstellar bands in the local ISM on small scales via MUSE 3D spectroscopy. A pilot study based on globular cluster NGC 6397
Context. We map the interstellar medium (ISM) including the diffuse interstellar bands (DIBs) in absorption toward the globular cluster NGC 6397 using VLT/MUSE. Assuming the absorbers are located at the rim of the Local Bubble we trace structures on the order of mpc (milliparsec, a few thousand AU). Aims: We aimed to demonstrate the feasibility to
Wendt, M. et al.Fecha de publicación:
112017