Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Sieyra, M V"'
Autor:
Sieyra, M. V., Prasad, S. Krishna, Stenborg, G., Khomenko, E., Van Doorsselaere, T., Costa, A., Esquivel, A., Riedl, J. M.
Publikováno v:
A&A 667, A21 (2022)
Recurrent, arc-shaped intensity disturbances were detected by EUV channels in an active region. The fronts were observed to propagate along a coronal loop bundle rooted in a small area within a sunspot umbra. Previous works have linked these intensit
Externí odkaz:
http://arxiv.org/abs/2208.10857
Publikováno v:
A&A 662, A113 (2022)
A critical aspect of solar activity is the coupling between eruptions and the surrounding coronal magnetic field, which determines the trajectory and morphology of the eruptive event. Pseudostreamers (PSs) are coronal magnetic structures formed by ar
Externí odkaz:
http://arxiv.org/abs/2205.07936
Autor:
Morgado, B. E., Sicardy, B., Braga-Ribas, F., Desmars, J., Gomes-Júnior, A. R., Bérard, D., Leiva, R., Ortiz, J. L., Vieira-Martins, R., Benedetti-Rossi, G., Santos-Sanz, P., Camargo, J. I. B., Duffard, R., Rommel, F. L., Assafin, M., Boufleur, R. C., Colas, F., Kretlow, M., Beisker, W., Sfair, R., Snodgrass, C., Morales, N., Fernández-Valenzuela, E., Amaral, L. S., Amarante, A., Artola, R. A., Backes, M., Bath, K-L., Bouley, S., Buie, M. W., Cacella, P., Colazo, C. A., Colque, J. P., Dauvergne, J-L., Dominik, M., Emilio, M., Erickson, C., Evans, R., Fabrega-Polleri, J., Garcia-Lambas, D., Giacchini, B. L., Hanna, W., Herald, D., Hesler, G., Hinse, T. C., Jacques, C., Jehin, E., Jørgensen, U. G., Kerr, S., Kouprianov, V., Levine, S. E., Linder, T., Maley, P. D., Machado, D. I., Maquet, L., Maury, A., Melia, R., Meza, E., Mondon, B., Moura, T., Newman, J., Payet, T., Pereira, C. L., Pollock, J., Poltronieri, R. C., Quispe-Huaynasi, F., Reichart, D., de Santana, T., Schneiter, E. M., Sieyra, M. V., Skottfelt, J., Soulier, J. F., Starck, M., Thierry, P., Torres, P. J., Trabuco, L. L., Unda-Sanzana, E., Yamashita, T. A. R., Winter, O. C., Zapata, A., Zuluaga, C. A.
Publikováno v:
A&A 652, A141 (2021)
The Centaur (10199) Chariklo has the first rings system discovered around a small object. It was first observed using stellar occultation in 2013. Stellar occultations allow the determination of sizes and shapes with kilometre accuracy and obtain cha
Externí odkaz:
http://arxiv.org/abs/2107.07904
Autor:
Sieyra, M. V., Cécere, M., Cremades, H., Iglesias, F. A., Sahade, A., Mierla, M., Stenborg, G., Costa, A., West, M., D'Huys, E.
Motivated by the need to improve the ability to forecast whether a certain coronal mass ejection (CME) is to impact Earth, and by the insufficiency of statistical studies that analyze the whole erupting system with the focus on the governing conditio
Externí odkaz:
http://arxiv.org/abs/2007.14317
Slow waves are commonly observed on the entire solar atmosphere. Assuming a thin flux tube approximation, the cut-off periods of slow-mode magneto-acoustic-gravity waves that travel from the photosphere to the corona were obtained in Costa et al. (20
Externí odkaz:
http://arxiv.org/abs/2004.09609
Autor:
Velázquez, P. F., Schneiter, E. M., Reynoso, E. M., Esquivel, A., De Colle, F., Toledo-Roy, J. C., Gómez, D. O., Sieyra, M. V., Moranchel-Basurto, A.
Three dimensional magnetohydrodynamical simulations were carried out in order to perform a new polarization study of the radio emission of the supernova remnant SN 1006. These simulations consider that the remnant expands into a turbulent interstella
Externí odkaz:
http://arxiv.org/abs/1701.05589
Akademický článek
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Akademický článek
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Publikováno v:
Monthly Notices of the Royal Astronomical Society; Jun2020, Vol. 494 Issue 4, p5270-5278, 9p
