Zobrazeno 1 - 10
of 109
pro vyhledávání: '"Cerrato Y"'
Publikováno v:
Proceedings of the International Astronomical Union, 2015, Volume 305 'Polarimetry: From the Sun to Stars and Stellar Environments'
Flux emergence phenomena are relevant at different temporal and spatial scales. We have studied a flux emergence region underneath a filament. This filament elevated itself smoothly, and the associated CME reached Earth. In this study we investigate
Externí odkaz:
http://arxiv.org/abs/1704.00681
Autor:
Palacios, J., Cid, C., Guerrero, A., Saiz, E., Cerrato, Y., Rodríguez-Bouza, M., Rodríguez-Bilbao, I., Herraiz, M., Rodríguez-Caderot, G.
Publikováno v:
ASP Conference Series, 2016, volume 504: Ground based solar observations in the space instrumentation era
The Spanish Space Weather Service SeNMEs, \url{www.senmes.es}, is a portal created by the SRG-SW of the Universidad de Alcal\'a, Spain, to meet societal needs of near real-time space weather services. This webpage-portal is divided in different secti
Externí odkaz:
http://arxiv.org/abs/1704.00684
Publikováno v:
A&A 583, A47 (2015)
Here we report evidence of a large solar filament eruption on 2013, September 29. This smooth eruption, which passed without any previous flare, formed after a two-ribbon flare and a coronal mass ejection towards Earth. The coronal mass ejection gene
Externí odkaz:
http://arxiv.org/abs/1509.05602
In September 1859 the Colaba observatory measured the most extreme geomagnetic disturbance ever recorded at low latitudes related to solar activity: the Carrington storm. This paper describes a geomagnetic disturbance case with a profile extraordinar
Externí odkaz:
http://arxiv.org/abs/1505.07028
Publikováno v:
J. Geophys. Res., (2010), 115, A07220
What one commonly considers for reproducing the recovery phase of magnetosphere, as seen by the Dst index, is exponential function. However, the magnetosphere recovers faster in the first hours than in the late recovery phase. The early steepness fol
Externí odkaz:
http://arxiv.org/abs/1405.4996
Publikováno v:
J. Geophys. Res. Space Physics, 2013, 118, 1-8
The recovery phase of the largest storms ever recorded has been studied. These events provide an extraordinary opportunity for two goals: (1) to validate the hyperbolic model by Aguado et al. [2010] for the recovery phase after disturbances as severe
Externí odkaz:
http://arxiv.org/abs/1405.4804
Publikováno v:
Highlights of Spanish Astrophysics VII, may 2013, pages 792-797
We investigate the geoeffective events happened from 8 to 20 Sept 2011, analysing the most plausible solar sources of these events, where coronal mass ejections and coronal holes play a fundamental role. The physical properties of the coronal holes,
Externí odkaz:
http://arxiv.org/abs/1401.1721
Autor:
Dasso, S., Mandrini, C. H., Schmieder, B., Cremades, H., Cid, C., Cerrato, Y., Saiz, E., Démoulin, P., Zhukov, A. N., Rodriguez, L., Aran, A., Menvielle, M., Poedts, S.
Publikováno v:
Dasso et al., Linking two consecutive non-merging magnetic clouds with their solar sources, Journal of Geophysical Research (ISSN 0148-0227), 114, CiteID A02109, 2009
On 15 May 2005, a huge interplanetary coronal mass ejection (ICME) was observed near Earth. It triggered one of the most intense geomagnetic storms of solar cycle 23 (Dst peak = -263 nT). This structure has been associated with the two-ribbon flare,
Externí odkaz:
http://arxiv.org/abs/1212.5546
Akademický článek
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Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics May 2012 80:111-123
