Zobrazeno 1 - 10
of 642
pro vyhledávání: '"P Terradas"'
Autor:
Luna, Manuel, Joshi, Reetika, Schmieder, Brigitte, Moreno-Insertis, Fernando, Liakh, Valeriia, Terradas, Jaume
Large amplitude oscillations commonly occur in solar prominences, triggered by energetic phenomena such as jets and flares. On March 14-15, 2015, a filament partially erupted in two stages, leading to oscillations in different parts. This study explo
Externí odkaz:
http://arxiv.org/abs/2410.10223
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
In recent studies on ultrastrong coupling between matter and light in cavities, the significance of gauge choice when employing the widely-used two-level approximation has been highlighted. Expanding upon these investigations, we extend the analysis
Externí odkaz:
http://arxiv.org/abs/2309.06500
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
Publikováno v:
A&A 676, A25 (2023)
The fine structure of solar prominences is made by thin threads that outline the magnetic field lines. Observations show that transverse waves of Alfv\'enic nature are ubiquitous in prominence threads. These waves are driven at the photosphere and pr
Externí odkaz:
http://arxiv.org/abs/2306.13434
Autor:
Terradas, Jaume, Neukirch, Thomas
Publikováno v:
A&A 671, A31 (2023)
Active regions (ARs) are typical magnetic structures found in the solar atmosphere. We calculate several magnetohydrostatic (MHS) equilibrium models that include the effect of a finite plasma-$\beta$ and gravity and that are representative of these s
Externí odkaz:
http://arxiv.org/abs/2212.04735
Autor:
Noemi Gonzalez-Abuin, Tirso Pons, Teresa Fuster, Isabel Quintana, Mariona Terradas, Gemma Aiza, Joan Brunet, Gabriel Capellá, Heather Hampel, Laura Valle
Publikováno v:
Genes and Diseases, Vol 11, Iss 2, Pp 524-527 (2024)
Externí odkaz:
https://doaj.org/article/16e1192c4ed846748ba330ceefad6fb1
Autor:
Terradas-Briansó, Sergi, González-Gutiérrez, Carlos A., Nori, Franco, Martín-Moreno, Luis, Zueco, David
Quantum optics with giant emitters has shown a new route for the observation and manipulation of non-Markovian properties in waveguide-QED. In this paper we extend the theory of giant atoms, hitherto restricted to the perturbative light-matter regime
Externí odkaz:
http://arxiv.org/abs/2205.07915
Autor:
Gerard Terradas, Jaime Manzano-Alvarez, Chiara Vanalli, Kristine Werling, Isabella M. Cattadori, Jason L. Rasgon
Publikováno v:
Parasites & Vectors, Vol 17, Iss 1, Pp 1-13 (2024)
Abstract Background Increasing global temperatures and unpredictable climatic extremes have contributed to the spread of vector-borne diseases. The mosquito Aedes aegypti is the main vector of multiple arboviruses that negatively impact human health,
Externí odkaz:
https://doaj.org/article/592167bc0fc4464490c0cc034145b3e6
Publikováno v:
A&A 660, A54 (2022)
Longitudinal oscillations in prominences are common phenomena on the Sun. These oscillations can be used to infer the geometry and intensity of the filament magnetic field. Previous theoretical studies of longitudinal oscillations made two simplifyin
Externí odkaz:
http://arxiv.org/abs/2202.07957