Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Losada, I. R."'
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
Autor:
Pastorello, A., Chen, T. -W., Cai, Y. -Z., Morales-Garoffolo, A., Cano, Z., Mason, E., Barsukova, E. A., Benetti, S., Berton, M., Bose, S., Bufano, F., Callis, E., Cannizzaro, G., Cartier, R., Chen, Ping, Dong, Subo, Dyrbye, S., Elias-Rosa, N., Floers, A., Fraser, M., Geier, S., Goranskij, V. P., Kann, D. A., Kuncarayakti, H., Onori, F., Reguitti, A., Reynolds, T., Losada, I. R., Carracedo, A. Sagues, Schweyer, T., Smartt, S. J., Tatarnikov, A. M., Valeev, A. F., Vogl, C., Wevers, T., Postigo, A. de Ugarte, Izzo, L., Inserra, C., Kankare, E., Maguire, K., Smith, K. W., Stalder, B., Tartaglia, L., Thoene, C. C., Valerin, G., Young, D. R.
We present the results of our photometric and spectroscopic follow-up of the intermediate-luminosity optical transient AT 2017jfs. At peak, the object reaches an absolute magnitude of Mg=-15.46+-0.15 mag and a bolometric luminosity of 5.5x10^41 erg/s
Externí odkaz:
http://arxiv.org/abs/1906.00811
Autor:
Paliya, Vaidehi S., Ajello, M., Ojha, R., Angioni, R., Cheung, C. C., Tanada, K., Pursimo, T., Galindo, P., Losada, I. R., Siltala, L., Djupvik, A. A., Marcotulli, L., Hartmann, D.
High-redshift ($z>2$) blazars are the most powerful members of the blazar family. Yet, only a handful of them have both X-ray and $\gamma$-ray detection, thereby making it difficult to characterize the energetics of the most luminous jets. Here, we r
Externí odkaz:
http://arxiv.org/abs/1812.07350
Publikováno v:
A&A 621, A61 (2019)
The formation of sunspots and starspots is not yet fully understood and is therefore one of the major open problems in solar and stellar physics. Magnetic flux concentrations can be produced by the negative effective magnetic pressure instability (NE
Externí odkaz:
http://arxiv.org/abs/1803.04446
Publikováno v:
Astron. Astrophys. 564, A2 (2014)
Strongly stratified hydromagnetic turbulence has recently been identified as a candidate for explaining the spontaneous formation of magnetic flux concentrations by the negative effective magnetic pressure instability (NEMPI). Much of this work has b
Externí odkaz:
http://arxiv.org/abs/1307.4945
Publikováno v:
Astronomy and Astrophysics 556, A83 (2013)
In a strongly stratified turbulent layer, a uniform horizontal magnetic field can become unstable to spontaneously form local flux concentrations due to a negative contribution of turbulence to the large-scale (mean-field) magnetic pressure. This mec
Externí odkaz:
http://arxiv.org/abs/1212.4077
Autor:
Pastorello, A., Chen, T.-W., Cai, Y.-Z., Morales-Garoffolo, A., Cano, Z., Mason, E., Barsukova, E. A., Benetti, S., Berton, M., Bose, S., Bufano, F., Callis, E., Cannizzaro, G., Cartier, R., Chen, Ping, Dong, Subo, Dyrbye, S., Elias-Rosa, N., Flörs, A., Fraser, M., Geier, S., Goranskij, V. P., Kann, D. A., Kuncarayakti, H., Onori, F., Reguitti, A., Reynolds, T., Losada, I. R., Sagués Carracedo, A., Schweyer, T., Smartt, S. J., Tatarnikov, A. M., Valeev, A. F., Vogl, C., Wevers, T., de Ugarte Postigo, A., Izzo, L., Inserra, C., Kankare, E., Maguire, K., Smith, K. W., Stalder, B., Tartaglia, L., Thöne, C. C., Valerin, G., Young, D. R.
We present the results of our photometric and spectroscopic follow-up of the intermediate-luminosity optical transient AT 2017jfs. At peak, the object reaches an absolute magnitude of Mg = −15.46 ± 0.15 mag and a bolometric luminosity of 5.5 × 10
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::c79d5079efc4b2573d45c07ebfc60ded
https://orca.cardiff.ac.uk/id/eprint/123157/1/aa35511-19.pdf
https://orca.cardiff.ac.uk/id/eprint/123157/1/aa35511-19.pdf
Autor:
Losada, I. R.1,2,3 (AUTHOR) illa.rivero.losada@gmail.com, Warnecke, J.4 (AUTHOR), Glogowski, K.5 (AUTHOR), Roth, M.5 (AUTHOR), Brandenburg, A.1,2,6 (AUTHOR), Kleeorin, N.1,7 (AUTHOR), Rogachevskii, I.1,7 (AUTHOR)
Publikováno v:
Proceedings of the International Astronomical Union. Oct2016 Supplement, Vol. 12 Issue S327, p46-59. 14p. 1 Color Photograph, 1 Chart, 4 Graphs.
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