@article{85eaf684170447d4985909480e879e27,
title = "Global variations and asymmetry of the sun during extremely high activity in October-November 2003",
abstract = "The data of the Coronas F satellite and other spacecraft were used to show that, in October-November 2003, global variations in brightness occurred in all spectral regions of the solar electromagnetic radiation. The variations were asymmetric in heliolongitude. This phenomenon was accompanied by an extremely strong energy release in the form of coronal-mass ejections and solar flares. The most powerful of them took place on the solar side that was characterized by an enhanced brightness even before these events. As a result, superimposed corotating and sporadic disturbances, which are partly correlated, can be traced in parameters of the solar atmospheric radiation, flows of the solar-wind plasma, and heliospheric magnetic field.",
author = "Veselovsky, {I. S.} and Dmitriev, {A. V.} and Zhitnik, {I. A.} and Zhukov, {A. N.} and Zel'dovich, {M. A.} and Kuzin, {S. V.} and Naumkin, {A. A.} and Persiantsev, {I. G.} and Ryazanov, {A. Yu} and Shugai, {Yu S.} and Yakovchuk, {O. S.} and Bogachev, {S. V.} and Shestov, {S. V.}",
note = "Funding Information: ACKNOWLEDGMENTS This work was supported in part by the Russian Foundation for Basic Research (project no. 04-02-16736), the Universities of Russia program (project no. 1877-04), the Scientific Schools program (grant no. NSh-2046.2003.02), the National Astronomy program, the “Non-Stationary Events in Astronomy” program of the Presidium of the Russian Academy of Sciences, and the Solar Wind program of the Department of Physical Sciences of the Russian Academy of Sciences.",
year = "2005",
month = may,
doi = "10.1007/s11208-005-0032-3",
language = "???core.languages.en_GB???",
volume = "39",
pages = "169--175",
journal = "Solar System Research",
issn = "0038-0946",
number = "3",
}