Evolution of ionospheric current systems for the geomagnetic impulse SI/SC by the magnetometer global network data : [тезисы докладов] / S. I. Solovyev, A. V. Moiseyev, M. Engebretson, K. Yumoto // Physics of auroral phenomena : 24 annual seminar, 27 February - 2 March 2001. – 2001. – P. 36.

Стародубцев, С. А. Прогноз прихода межпланетных ударных волн по измерениям флуктуаций космических лучей в солнечном ветре : [тезисы докладов] / С. А. Стародубцев, В. Г. Григорьев // Космические лучи и гелиосфера. – Якутск : Сфера, 2012. – С. 21-22.

Комарицына, Е. С. Геоэффективность магнитных облаков различных типов / Е. С. Комарицына, С. З. Кершенгольц, Е. С. Баркова // Динамика сплошной среды. – 2004. – Вып. 122 : Доклады Всероссийской школы-семинара "Фундаментальные и прикладные проблемы физики на Севере", Якутск, 24-28 июня 2003. – С. 67-70.

The geomagnetic severe storm on November 7-11, 2004 had Dst=-383 nT and had probably caused by the coronal mass ejection (CME) in interplanetary space. The burst of solar X-ray preceded the halo-ejection of solar plasma. The experimental fact testifying the global response of the geomagnetic field ("crochet" type) observed after the solar flare on November 6, 2004 is given. The reaction in the geomagnetic field lasted for several hours as well as X-ray bursts registered aboard GEOS-12.

Solar X-ray Bursts as a Possible Predictor of the Magnetic Storm in November 2004 / V. A. Velichko, D. G. Baishev, I. Ya. Plotnikov, N. G. Skryabin, R. N. Boroev // Solar Extreme Events Fundamental Science and Applied Aspects Nor-Amberd, Armenia 26-30 September 2005 : proceedings of the Second International Symposium / edited by A. Chilingarian and G. Karapetyan. − Erevan : Cosmic Ray Division, Alikhanyan Physics Institute, 2006. − P. 107-108.

The 20.11.03 super-storm is described on the basis of the quantitative estimations of input and output parameters of the magnetospheric disturbance energetics. Two input parameters are ε'- Poynting flux from solar wind into the magnetosphere, and the polar cap potential drop Upc. The output parameters (indicators the magnetospheric responses) are the total power of the magnetospheric disturbance (Qt), and the powers consumed in the ionosphere (Qi) and in the ring current (Qdr). Different modes of the magnetosphere disturbances are shortly described: substorms, driven mode, Null Events by Lyons et. al., saturation of the ionosphere, and responses to a strong s. w. pressure pulses. The problem of the substorms-storm relationship is also addressed.

Basic Regimes of the Super-Storm on Nov 20, 2003 and the Problems Substorms-Storm / V. M. Mishin, M. Foerster, T. I. Saifudinova, A. D. Bazarzhapov, L. A. Sapronova, V. P. Golovkov, P. Stauning, J. Watermann, and S. I. Solovyev // Solar Extreme Events Fundamental Science and Applied Aspects Nor-Amberd, Armenia 26-30 September 2005 : proceedings of the Second International Symposium / edited by A. Chilingarian and G. Karapetyan. − Erevan : Cosmic Ray Division, Alikhanyan Physics Institute, 2006. − P. 86-89.

In the accompanying Papers 1 and 2 was fulfilled timing of the 20.11.05 super-storm. Were detected 4 various types of the magnetospheric disturbances observable at southward IMF, and presented a new model of the field-aligned currents density spatial distribution in the polar ionosphere. In this paper are described the ionospheric convection systems, characteristic for the above various types. Are mentioned the mesoscale spatial inhomogeneities, which are observed more or less regularly but have not been mentioned in the past literature.

Dynamics of the Ionospheric Convection Systems Observed during The Super-Storm on Nov. 20, 2003 / M. Foerster, V. M. Mishin, T. I. Saifudinova, A. D. Bazarzhapov, L. A. Sapronova, V. P. Golovkov, P. Stauning, J. Watermann, and S. I. Solovyev // Solar Extreme Events Fundamental Science and Applied Aspects Nor-Amberd, Armenia 26-30 September 2005 : proceedings of the Second International Symposium / edited by A. Chilingarian and G. Karapetyan. − Erevan : Cosmic Ray Division, Alikhanyan Physics Institute, 2006. − P. 83-85.

Galactic cosmic ray (GCR) diffusion in interplanetary space depends in a certain way on the degree of regularity of the interplanetary magnetic field (IMF). The sector IMF structure is manifested in inhomogeneous GCR distribution in the heliosphere. In parallel with the usual sectors associated with solar activity, one should take into account the sectors, which are caused by the Jupiter activity. It is known that the Jupiter is a powerful regular source of high-energy electrons (0.2-40 MeV), the density of which, on the average, is many times higher than that of solar cosmic rays. The high-energy electrons are systematically registed with the 399-day period in the near-Earth space. According to estimations of the particle energy density their flux is sufficient to decrease the magnetic field in the Jovian sector and can due to corresponding large-scale inhomogeneity in the GKL distribution. Hereby, we present the evidences that the GCR diffusion is noticeably stronger in the sector where there are Jovian electrons. By data on periodic passage of those sectors near the Earth, we have treated neutron monitor data using the superposed epoch technique. The day of the Earth and Jupiter opposition is taken as a zero epoch. At large statistical data (9925 days) it is found that the GCR intensity in that period increases with an amplitude near 1%. The groud effect is manifested with the period of 399 days and its maximum time is in a certain way shifted relative to the planet opposite moment.

Skryabin, N. G. Influence of Jupiter on cosmic ray intensity variations / N. G. Skryabin, S. N. Samsonov, I. Ya. Plotnikov // Physics of auroral phenomena : proceedings of the 25th annual seminar, Apatity, 26 February – 1 March 2002. – 2002. – P. 137-139.

Ковалев, А. А. Результаты моделирования эффектов солнечных затмений в среднеширотной ионосфере / А. А. Ковалев, В. И. Попов // Физика окружающей среды : материалы VIII Международной школы молодых ученых. – Томск : ТГУ, 2010. – С. 83-86.

Моделирование эффекта влияния локальных электрических полей магнитосферного происхождения на структуру субавроральной ионосферы / Е. Д. Бондарь, И. А. Голиков, В. И. Попов, А. Е. Степанов, В. Л. Халипов // Физика окружающей среды : материалы VIII Международной школы молодых ученых. – Томск : ТМЛ-Пресс, 2010. – С. 30-33.

Переходный процесс распада крупномасштабного магнитного поля Солнца на стадии его переполюсовки проявляется в виде гигантской "волны переполюсовки" с полугодовым периодом. Максимумы волны в индексе мерцаний космических лучей предшествуют минимумам интенсивности галактических космических лучей (ГКЛ) в среднем на три оборота Солнца. Полугодовая волна выявлена и в параметрах межпланетного магнитного поля ( в дисперсии ММП). Наличие волны переполюсовки объясняет единым образом "провал" в значениях большинства параметров как в максимуме солнечной активности ( эффект Гневышева), так и в начале ветви спада 11-летнего цикла.

Марков, В. В. Волна переполюсовки магнитного поля солнца во флуктациях космических лучей / В. В. Марков, В. И. Козлов // Труды VI сессии молодых ученых "Волновые процессы в проблеме космической погоды" [15-20 сентября 2003 г.]. - Иркутск : ИСЗФ, 2003. - С. 150-154.