Zobrazeno 1 - 10
of 90
pro vyhledávání: '"A. A. Ruzmaĭkin"'
Autor:
Gómez, Jenny M. Rodríguez, Podladchikova, Tatiana, Veronig, Astrid, Ruzmaikin, Alexander, Feynman, Joan, Petrukovich, Anatoly
We study the clustering properties of fast Coronal Mass Ejections (CMEs) that occurred during solar cycles 23 and 24. We apply two methods: the Max spectrum method can detect the predominant clusters and the de-clustering threshold time method provid
Externí odkaz:
http://arxiv.org/abs/2006.10404
Publikováno v:
Journal of Plasma Physics, 2018, v. 84, No. 3, 735840306
We apply a nonlinear mean-field dynamo model which includes a budget equation for the dynamics of Wolf numbers to predict solar activity. This dynamo model takes into account the algebraic and dynamic nonlinearities of the alpha effect, where the equ
Externí odkaz:
http://arxiv.org/abs/1712.07501
Mutual quasi-periodicities near the solar-rotation period appear in time series based on the Earth's magnetic field, the interplanetary magnetic field, and signed solar-magnetic fields. Dominant among these is one at 27.03 +/- 0.02 days that has been
Externí odkaz:
http://arxiv.org/abs/0803.3260
Principal Components Analysis (PCA) and Independent Component Analysis (ICA) are used to identify global patterns in solar and space data. PCA seeks orthogonal modes of the two-point correlation matrix constructed from a data set. It permits the iden
Externí odkaz:
http://arxiv.org/abs/0709.3263
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics May 2018 170:21-34
Autor:
Bigazzi, Alberto, Ruzmaikin, Alexander
Publikováno v:
Astrophys.J. 604 (2004) 944-959
Observations show that solar activity is distributed non-axisymmetrically, concentrating at "preferred longitudes". This indicates the important role of non-axisymmetric magnetic fields in the origin of solar activity. We investigate the generation o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312212
Publikováno v:
Proc. of SOHO 12/GONG+ 2002 'Local and Global Helioseismology: The Present and Future', Big Bear Lake, California (U.S.A.), 27 October - 1 November 2002 (ESA SP-517, February 2003) ISSN 0379-6566 / ISBN 92-9092-827-1
One of the key questions in solar physics that remains to be answered concerns the strength and the distribution of the magnetic fields at the base of the convection zone. The flux tube dynamics requires that toroidal fields of strength as large as 1
Externí odkaz:
http://arxiv.org/abs/astro-ph/0211116
Below the scale of supergranules we find that cellular flows are present in the solar photosphere at two distinct size scales, approximately 2 Mm and 4 Mm, with distinct characteristic times. Simultaneously present in the flow is a non-cellular compo
Externí odkaz:
http://arxiv.org/abs/astro-ph/0104354
Publikováno v:
Phys. Rev. Letters, 86, 5894 (2001)
The Sun provides an excellent natural laboratory for nonlinear phenomena. We use motions of magnetic bright points on the solar surface, at the smallest scales yet observed, to study the small scale dynamics of the photospheric plasma. The paths of t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0101224
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics September 2013 102:99-104