Zobrazeno 1 - 10
of 721
pro vyhledávání: '"Noda C"'
Autor:
Noda, C. Quintero, Shchukina, N. G., Ramos, A. Asensio, González, M. J. Martínez, Alemán, T. del Pino, Arjona, J. C. Trelles, Collados, M.
Inferring the coupling of different atmospheric layers requires observing spectral lines sensitive to the atmospheric parameters, particularly the magnetic field vector, at various heights. The best way to tackle this goal is to perform multi-line ob
Externí odkaz:
http://arxiv.org/abs/2411.12397
Publikováno v:
A&A 686, A244 (2024)
We analyse the spatial distribution and vertical stratification of the physical parameters of the solar atmosphere when an X-class flare occurs. We made use of observations acquired by the Interferometric Bidimensional Spectropolarimeter instrument w
Externí odkaz:
http://arxiv.org/abs/2404.06231
Publikováno v:
2023, MNRAS, 523, 1
Chromospheric jets are plausible agents of energy and mass transport in the solar chromosphere, although their driving mechanisms have not yet been elucidated. Magnetic field measurements are key for distinguishing the driving mechanisms of chromosph
Externí odkaz:
http://arxiv.org/abs/2310.01692
Publikováno v:
Neuropsychiatric Disease and Treatment, Vol 2015, Iss default, Pp 2953-2958 (2015)
Yoko Komada,1 Raoul Breugelmans,2 Stephany Fulda,3 Sae Nakano,4 Aya Watanabe,4,5 Chieri Noda,4,6 Shingo Nishida,1 Yuichi Inoue1 1Department of Somnology, 2Department of Medical Education, Tokyo Medical University, Tokyo, Japan; 3Sleep and Epilepsy Ce
Externí odkaz:
https://doaj.org/article/f3fa22a92ead4c15bd7cfbd533966553
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:
Noda, C. Quintero, Schlichenmaier, R., Rubio, L. R. Bellot, Löfdahl, M. G., Khomenko, E., Jurcak, J., Leenaarts, J., Kuckein, C., Manrique, S. J. González, Gunar, S., Nelson, C. J., Rodríguez, J. de la Cruz, Tziotziou, K., Tsiropoula, G., Aulanier, G., Collados, M., team, the EST
Publikováno v:
A&A 666, A21 (2022)
The European Solar Telescope (EST) is a project aimed at studying the magnetic connectivity of the solar atmosphere, from the deep photosphere to the upper chromosphere. Its design combines the knowledge and expertise gathered by the European solar p
Externí odkaz:
http://arxiv.org/abs/2207.10905
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
Publikováno v:
A&A 659, A156 (2022)
The Milne-Eddington approximation provides an analytic and simple solution to the radiative transfer equation. It can be easily implemented in inversion codes that are used to fit spectro-polarimetric observations to infer average values of the magne
Externí odkaz:
http://arxiv.org/abs/2112.14536
Publikováno v:
A&A 656, L20 (2021)
We aim at demonstrating the capabilities of a newly developed method for determining electric currents in the solar photosphere. We employ three-dimensional radiative magneto-hydrodynamic (MHD) simulations to produce synthetic Stokes profiles in seve
Externí odkaz:
http://arxiv.org/abs/2112.04356
Autor:
Kuckein, C., Balthasar, H., Noda, C. Quintero, Diercke, A., Arjona, J. C. Trelles, Cobo, B. Ruiz, Felipe, T., Denker, C., Verma, M., Kontogiannis, I., Sobotka, M.
Publikováno v:
A&A 653, A165 (2021)
The spectral window, containing Fraunhofer lines formed in the solar photosphere, around the magnetically sensitive Cr I lines at 5780.9, 5781.1, 5781.7, 5783.0, and 5783.8 \r{A}, with Land\'e g-factors between 1.6 and 2.5, is explored. The goal is t
Externí odkaz:
http://arxiv.org/abs/2107.11116