Zobrazeno 1 - 10
of 78
pro vyhledávání: '"Bingert, S."'
Autor:
Brandenburg, A., Johansen, A., Bourdin, P. A., Dobler, W., Lyra, W., Rheinhardt, M., Bingert, S., Haugen, N. E. L., Mee, A., Gent, F., Babkovskaia, N., Yang, C. -C., Heinemann, T., Dintrans, B., Mitra, D., Candelaresi, S., Warnecke, J., Käpylä, P. J., Schreiber, A., Chatterjee, P., Käpylä, M. J., Li, X. -Y., Krüger, J., Aarnes, J. R., Sarson, G. R., Oishi, J. S., Schober, J., Plasson, R., Sandin, C., Karchniwy, E., Rodrigues, L. F. S., Hubbard, A., Guerrero, G., Snodin, A., Losada, I. R., Pekkilä, J., Qian, C.
Publikováno v:
Journal of Open Source Software 6, 2807 (2021)
The Pencil Code is a highly modular physics-oriented simulation code that can be adapted to a wide range of applications. It is primarily designed to solve partial differential equations (PDEs) of compressible hydrodynamics and has lots of add-ons ra
Externí odkaz:
http://arxiv.org/abs/2009.08231
The outer solar atmosphere, the corona, contains plasma at temperatures of more than a million K, more than 100 times hotter that solar surface. How this gas is heated is a fundamental question tightly interwoven with the structure of the magnetic fi
Externí odkaz:
http://arxiv.org/abs/1505.01174
We present the first model that couples the formation of the corona of a solar active region to a model of the emergence of a sunspot pair. This allows us to study when, where, and why active region loops form, and how they evolve. We use a 3D radiat
Externí odkaz:
http://arxiv.org/abs/1402.5343
Autor:
Peter, H., Bingert, S., Klimchuk, J. A., de Forest, C., Cirtain, J. W., Golub, L., Winebarger, A. R., Kobayashi, K., Korreck, K. E.
We will use new data from the High-resolution Coronal Imager (Hi-C) with unprecedented spatial resolution of the solar corona to investigate the structure of coronal loops down to 0.2 arcsec. During a rocket flight Hi-C provided images of the solar c
Externí odkaz:
http://arxiv.org/abs/1306.4685
Publikováno v:
A&A, 555, A123 (2013)
Aims. The goal is to employ a 3D magnetohydrodynamics (MHD) model including spectral synthesis to model the corona in an observed solar active region. This will allow us to judge the merits of the coronal heating mechanism built into the 3D model. Me
Externí odkaz:
http://arxiv.org/abs/1305.5693
We investigate the difference in the spatial distribution of the energy input for parametrizations of different mechanisms to heat the corona of the Sun and possible impacts on the coronal emission. We use a 3D MHD model of a solar active region as a
Externí odkaz:
http://arxiv.org/abs/1303.1371
Autor:
Peter, H., Bingert, S.
The corona of the Sun is dominated by emission from loop-like structures. When observed in X-ray or extreme ultraviolet emission, these million K hot coronal loops show a more or less constant cross section. In this study we show how the interplay of
Externí odkaz:
http://arxiv.org/abs/1209.0789
Publikováno v:
A&A 537, A152 (2012)
Condensations in the more than 10^6 K hot corona of the Sun are commonly observed in the extreme ultraviolet (EUV). While their contribution to the total solar EUV radiation is still a matter of debate, these condensations certainly provide a valuabl
Externí odkaz:
http://arxiv.org/abs/1112.3667
We investigate the processes that lead to the formation, ejection and fall of a confined plasma ejection that was observed in a numerical experiment of the solar corona. By quantifying physical parameters such as mass, velocity, and orientation of th
Externí odkaz:
http://arxiv.org/abs/1106.5972
Publikováno v:
International Journal on Advances in Security
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1874::57aa382250590a4ee218d100f4f7e53e
https://hdl.handle.net/21.11116/0000-000C-C79A-6
https://hdl.handle.net/21.11116/0000-000C-C79A-6