Zobrazeno 1 - 10
of 297
pro vyhledávání: '"Uitenbroek, H"'
Autor:
Kuridze, D., Uitenbroek, H., Wöger, F., Mathioudakis, M., Morgan, H., Campbell, R., Fischer, C., Cauzzi, G., Schad, T., Reardon, K., Santos, J. M. da Silva, Beck, C., Tritschler, A., Rimmele, T.
The strongly coupled hydrodynamic, magnetic, and radiation properties of the plasma in the solar chromosphere makes it a region of the Sun's atmosphere that is poorly understood. We use data obtained with the high-resolution Visible Broadband Imager
Externí odkaz:
http://arxiv.org/abs/2402.04545
Autor:
Santos, J. M. da Silva, Reardon, K., Cauzzi, G., Schad, T., Pillet, V. Martinez, Tritschler, A., Wöger, F., Hofmann, R., Stauffer, J., Uitenbroek, H.
Plage regions are patches of concentrated magnetic field in the Sun's atmosphere where hot coronal loops are rooted. While previous studies have shed light on the properties of plage magnetic fields in the photosphere, there are still challenges in m
Externí odkaz:
http://arxiv.org/abs/2308.10983
Autor:
Noda, C. Quintero, Khomenko, E., Collados, M., Cobo, B. Ruiz, Gafeira, R., Vitas, N., Rempel, M., Campbell, R. J., Yabar, A. Pastor, Uitenbroek, H., Suárez, D. Orozco
In this work, we study the accuracy that can be achieved when inferring the atmospheric information from realistic numerical magneto-hydrodynamic simulations that reproduce the spatial resolution we will obtain with future observations made by the 4m
Externí odkaz:
http://arxiv.org/abs/2306.01422
Autor:
Tripathy, S. C., Jain, K., Braun, D., Cally, P., Dikpati, M., Felipe, T., Jain, R., Kholikov, S., Khomenko, E., Komm, R., Leibacher, J., Martinez-Pillet, V., Pevtsov, A., Rajaguru, S. P., Roth, M., Uitenbroek, H., Zhao, J.
The goal of helioseismology is to provide accurate information about the Sun's interior from the observations of the wave field at its surface. In the last three decades, both global and local helioseismology studies have made significant advances an
Externí odkaz:
http://arxiv.org/abs/2305.07585
Autor:
Grant, S. D. T., Jess, D. B., Stangalini, M., Jafarzadeh, S., Fedun, V., Verth, G., Keys, P. H., Rajaguru, S. P., Uitenbroek, H., Macbride, C. D., Bate, W., Gilchrist-Millar, C. A.
Solar pores are efficient magnetic conduits for propagating magnetohydrodynamic wave energy into the outer regions of the solar atmosphere. Pore observations often contain isolated and/or unconnected structures, preventing the statistical examination
Externí odkaz:
http://arxiv.org/abs/2209.06280
Autor:
Cobo, B. Ruiz, Noda, C. Quintero, Gafeira, R., Uitenbroek, H., Suárez, D. Orozco, Mañá, E. Páez
Publikováno v:
A&A 660, A37 (2022)
Future ground-based telescopes, such as the 4-metre class facilities DKIST and EST, will dramatically improve on current capabilities for simultaneous multi-line polarimetric observations in a wide range of wavelength bands, from the near-ultraviolet
Externí odkaz:
http://arxiv.org/abs/2202.02226
Autor:
Noda, C. Quintero, Barklem, P. S., Gafeira, R., Cobo, B. Ruiz, Collados, M., Carlsson, M., Pillet, V. Martínez, Suárez, D. Orozco, Uitenbroek, H., Katsukawa, Y.
Publikováno v:
A&A 652, A161 (2021)
Future ground-based telescopes will expand our capabilities for simultaneous multi-line polarimetric observations in a wide range of wavelengths, from the near-ultraviolet to the near-infrared. This creates a strong demand to compare candidate spectr
Externí odkaz:
http://arxiv.org/abs/2106.05084
In this work, we discuss the application of convolutional neural networks (CNNs) as a tool to advantageously initialize Stokes profile inversions. To demonstrate the usefulness of CNNs, we concentrate in this paper on the inversion of LTE Stokes prof
Externí odkaz:
http://arxiv.org/abs/2103.09651
Publikováno v:
A&A 646, A79 (2021)
The Mg I 12.32 and 12.22 $\mu$m lines are a pair of emission lines that present a great advantage for accurate solar magnetic field measurement. They potentially contribute to the diagnosis of solar atmospheric parameters through their high magnetic
Externí odkaz:
http://arxiv.org/abs/2012.08912
Publikováno v:
A&A 623, A74 (2019)
The inference of the underlying state of the plasma in the solar chromosphere remains extremely challenging because of the nonlocal character of the observed radiation and plasma conditions in this layer. Inversion methods allow us to derive a model
Externí odkaz:
http://arxiv.org/abs/1810.08441