Zobrazeno 1 - 10
of 2 498
pro vyhledávání: '"Soler R"'
Autor:
Antolín S, Acea B, Albaina L, Concha Á, Santiago P, García-Caballero T, Mosquera JJ, Varela JR, Soler R, Calvo L
Publikováno v:
Breast Cancer: Targets and Therapy, Vol Volume 11, Pp 29-42 (2018)
Silvia Antolín,1 Benigno Acea,2 Luis Albaina,2 Ángel Concha,3 Paz Santiago,3 Tomás García-Caballero,4 Joaquín J Mosquera,5 José Ramón Varela,5 Rafaela Soler,5 Lourdes Calvo1 1Medical Oncology Department, Breast Unit, A Coruña University Hospi
Externí odkaz:
https://doaj.org/article/baccee9a46d042eca38ea148ccbfb013
Autor:
Piantschitsch, I., Terradas, J., Soubrie, E., Heinemann, S. G., Hofmeister, S. J., Soler, R., Temmer, M.
The geometry of a coronal hole (CH) affects the density profile of the reflected part of an incoming global coronal wave (CW). In this study, we perform for the first time magnetohydrodynamic (MHD) simulations of fast-mode MHD waves interacting with
Externí odkaz:
http://arxiv.org/abs/2403.06614
Autor:
Piantschitsch, I., Terradas, J., Soubrie, E., Heinemann, S. G., Hofmeister, S. J., Soler, R., Temmer, M.
Interactions between global coronal waves (CWs) and coronal holes (CHs) reveal many interesting features of reflected waves and coronal hole boundaries (CHB) but have fairly been studied so far. Magnetohydrodynamic (MHD) simulations can help us to be
Externí odkaz:
http://arxiv.org/abs/2308.08928
Autor:
Terradas, J., Soler, R., Oliver, R., Antolin, P., Arregui, I., Luna, M., Piantschitsch, I., Soubrié, E., L., J., Ballester
Coronal holes and active regions are typical magnetic structures found in the solar atmosphere. We propose several magnetohydrostatic equilibrium solutions that are representative of these structures in two dimensions. Our models include the effect o
Externí odkaz:
http://arxiv.org/abs/2202.06800
Publikováno v:
A&A 653, A95 (2021)
Threads are the building blocks of solar prominences and very often show longitudinal oscillatory motions that are strongly attenuated with time. The damping mechanism responsible for the reported oscillations is not fully understood yet. To understa
Externí odkaz:
http://arxiv.org/abs/2106.06327
Autor:
Stangalini, M., Jess, D. B., Verth, G., Fedun, V., Fleck, B., Jafarzadeh, S., Keys, P. H., Murabito, M., Calchetti, D., Aldhafeeri, A. A., Berrilli, F., Del Moro, D., Jefferies, S. M., Terradas, J., Soler, R.
Publikováno v:
A&A 649, A169 (2021)
The umbral regions of sunspots and pores in the solar photosphere are generally dominated by $3$~mHz oscillations, which are due to $p$-modes penetrating the magnetic region. In these locations, wave power is also significantly reduced with respect t
Externí odkaz:
http://arxiv.org/abs/2103.11639
Autor:
Diaz-Suarez, S., Soler, R.
Publikováno v:
A&A 648, A22 (2021)
Both observations and numerical simulations suggest that Alfvenic waves may carry sufficient energy to sustain the hot temperatures of the solar atmospheric plasma. However, the thermalization of wave energy is inefficient unless very short spatial s
Externí odkaz:
http://arxiv.org/abs/2102.06464
Publikováno v:
A&A, 641, A106 (2020)
This paper investigates the changes in spatial properties when magnetohydrodynamic (MHD) waves undergo resonant damping in the Alfv\'en continuum. The analysis is carried out for a 1D cylindrical pressure-less plasma with a straight magnetic field. T
Externí odkaz:
http://arxiv.org/abs/2009.08152
Publikováno v:
Psychology Research and Behavior Management, Vol Volume 16, Pp 1365-1378 (2023)
Rocio Collado-Soler,1 Rubén Trigueros,1 Jose M Aguilar-Parra,1 Noelia Navarro2 1Department of Psychology, Hum-878 Research Team, Health Research Centre, University of Almeria, Almeria, 04120, Spain; 2Department of Psychology, Hum-760 Research Team,
Externí odkaz:
https://doaj.org/article/24853c67e66a45f4a323cbd8cb3d1fd6
Publikováno v:
In Powder Technology 1 July 2023 425