Продолжая использовать данный сайт, Вы даете согласие на обработку файлов cookie, пользовательских данных (сведения о местоположении; тип и версия ОС; тип и версия браузера; тип устройства и разрешение его экрана; источник откуда пользователь перешел на сайт; с какого сайта или по какой рекламе; язык ОС и браузера; какие страницы открывает и на какие кнопки нажимает пользователь; IP-адрес) в целях функционирования сайта и проведения статистических исследований и обзоров. Если вы не хотите, чтобы Ваши данные обрабатывались, Вы должны покинуть данный сайт.
Документы 21 - 30 из 1475
По заглавию По автору По году издания
21.
Обложка
Авторы:
Hori Tomoaki, Shinbori Atsuki , Nishitani Nozomu, Kikuchi Takashi, Fujita S. , Nagatsuma Tsutomu , Troshichev Oleg Alexandrovich, Yumoto Kiyohumi, Moiseyev Aleksey Vladimirovich, Seki K.
Заглавие: Evolution of negative SI-induced ionospheric flows observed by SuperDARN King Salmon HF radar

Количество страниц: 14 с.

The spatial evolution of vortex-like flow structures induced by a negative sudden impulse (SI-) is studied on the basis of SuperDARN King Salmon HF radar (KSR) with other ground and satellite data. A large dip in the solar wind density induced a fairly large SI- with a SYM-H amplitude of ~40 nT. The SI-induced ionospheric flow signatures in the evening sector (MLT ~ 19 h) were observed by KSR as a westward flow associated with the preliminary impulse (PI) followed by a more intense eastward flow with the main impulse (MI) in the sub-auroral region on the magnetic latitude ~60-70 deg, consistent with the local ground magnetic field observations. Following the first PI-MI flow sequence, KSR saw a second and possibly third sequence of flow variation which were much smaller in flow amplitude than the first pair but showed qualitatively very similar flow variations and latitudinal/longitudinal propagation characterististics/ These observations can be interpreted as aftershocks of the first PI-MI; the same sequence of vortices and field-aligned currents were generated and then drifted anti-sunward with the same mechanism, namely the pumping motion of dayside magnetosphere. These results are qualitatively consistent with predictions suggested by recent numerical simulations.

Evolution of negative SI-induced ionospheric flows observed by SuperDARN King Salmon HF radar / T. Hori, A. Shinbori, N. Nishitani, T. Kikuchi, S. Fujita, T. Nagatsuma, O. Troshichev, K. Yumoto, A. Moiseyev, and K. Seki // Journal of Geophysical Research: Space Physics. – 1978. – 2012 (December), vol. 117, N 12. – P. A12223.
DOI: 10.1029/2012JA018093

Подробнее
22.
Обложка
Автор:
Ivanova Oksana I.
Заглавие: Organization of space and time in the story "Makar’s Dream" and the story "Without Language" by V. G. Korolenko = Организация пространства и времени в рассказе "Сон Макара" и повести "Без языка" В. Г. Короленко

Количество страниц: 10 с.

Актуальность статьи определяется тем, что ее тема находится в русле работ отечественных исследователей творчества В. Г. Короленко Н. Н. Закировой, С. Л. Скопкаревой, А. В. Труханенко, В. Н. Крылова, Е. Г. Савельевой, посвященных проблеме организации пространства и времени в творчестве писателя. Методологической базой исследования послужили труды М. М. Бахтина, Ю. М. Лотмана. Целью работы является выявление своеобразия хронотопа в рассказе "Сон Макара" и повести "Без языка". Отмечается, что в обоих произведениях автор обращается к хронотопу дороги и дорожных встреч. Если в рассказе "Сон Макара" хронотопу Амги противопоставляется пространство и время загробного мира, то в повести "Без языка" хронотоп Нью-Йорка представлен в оппозиции к хронотопу родных героям Лозищей. В обоих произведениях можно констатировать "лиминальное" состояние героя - "обмирание" Макара, его "сон" и состояние Матвея Лозинского на пороге смерти в парке Нью-Йорка.

Ivanova, O. I. Organization of space and time in the story "Makar’s Dream" and the story "Without Language" by V. G. Korolenko / O. I. Ivanova ; M. K. Ammosov North-Eastern Federal University // Вестник Северо-Восточного федерального университета им. М. К. Аммосова. Серия: Серия "Вопросы национальных литератур". - 2023. - N 4 (12). - С. 14-23. - DOI: 10.25587/2782-6635-2023-4-14-23
DOI: 10.25587/2782-6635-2023-4-14-23

Подробнее
23.
Обложка
Авторы:
Jin-Bin Cao , Chunxiao Yan, Dunlop Malcolm, Reme Henri , Dandouras Iannis , Tielong Zhang, Dongmei Yang, Moiseyev Aleksey Vladimirovich, Solovyev Stepan Ivanovich, Wang Z. Q., Leonoviche Anatoly Sergeevich, Zolotukhina N. A., Mishin Vilen M.
Заглавие: Geomagnetic signatures of current wedge produced by fast flows in a plasma sheet

Количество страниц: 6 с.

This paper uses the plasma data from Cluster and TC-1 and geomagnetic data to study the geomagnetic signatures of current wedge produced by fast-flow braking in the plasma sheet. The three fast flows studied here occurred in a very quiet background and were accompanied by no (or weak) particle injections, thus avoiding the influences from other disturbances. All the geomagnetic signatures of a substorm current wedge can be found in geomagnetic signatures of a current system produced by the braking of fast flows, indicating that the fast flows can produce a complete current wedge which contains postmidnight downward and premidnight upward field-aligned currents, as well as a westward electrojet. The Pi2 precursors exist not only at high latitudes but also at midlatitudes. The starting times of midlatitude Pi2 precursors can be identified more precisely than those of high-latitude Pi2 precursors, providing a possible method to determine the starting time of fast flows in their source regions. The AL drop that a bursty bulk flow produces is proportional to its velocity and duration. In three cases, the AL drops are 200 nT, whether a substorm can be triggered depends mainly on the conditions of the braking regions before fast flows. The observations of solar wind before the three fast flows suggest that it is difficult for the fast flows to trigger a substorm when the interplanetary magnetic field Bz of solar wind is weakly southward.

Geomagnetic signatures of current wedge produced by fast flows in a plasma sheet / Jin-Bin Cao, Chunxiao Yan, Malcolm Dunlop, Henri Reme, Iannis Dandouras, Tielong Zhang, Dongmei Yang, Alexey Moiseyev, Stepan I. Solovyev, Z. Q. Wang, A. Leonoviche, N. Zolotukhina, and V. Mishin // Journal of Geophysical Research: Space Physics. – 1978. – 2010 (August), vol. 115, N 8. – P. A08205.

Подробнее
24.
Обложка
Авторы:
Khalipov Victor L., Galperin Yury Ilyich, Stepanov Alexander E., Bondar Elena D.
Заглавие: Formation of polarization jet during injection of ions into the inner magnetosphere

Количество страниц: 4 с.

Long-lasting ground based measurements of a polarization jet (PJ) by the latitudinal chain of ionospheric stations in Yakutia (3 < L < 5; MLT = UT + 9 h) and by 5 subauroral Russian stations were analyzed. A number of cases were found when PJ was recorded simultaneously with energetic ion observations by AMPTE/CCE and INTERBALL 2. The data comparison shows that at least in the considered cases of strong magnetic substorms, PJ was accompanied by strong injection of ions with the energy of ~20-50 keV and intensity of ~10 cm-² c-¹ sr-¹keV-¹. Close to the injection region in the near midnight sector no ion dispersion was observed, but in the evening sector nose events were detected. In accordance with the mechanism suggested by Southwood and Wolf (JGR, 1978, 83, 5227) PJ was observed near the equatorial boundary of energetic ion penetration into the magnetosphere. Measurements by ionosonds at different longitudes show that the westward velocity of the frontt of PJ development is close to the gradient drift velocity of 20 keV ions (forming nose events). Thus, the physical mechanism of PJ formation due to energetic ion injection during a strong substorm burst is experimentally confirmed. Satellite measurements show that in the near midnight sector energetic ions reach the shell L=3.0 in 20-30 minutes after a substorm commencement with AE>500 nT.

Formation of polarization jet during injection of ions into the inner magnetosphere / V. L. Khalipov, Yu. I. Galperin, A. E. Stepanov, E. D. Bondar // Physics of auroral phenomena : proceedings of the 25th annual seminar, Apatity, 26 February – 1 March 2002. – 2002. – P. 43-46.
DOI: 10.1016/S0273-1177(03)00016-4

Подробнее
25.
Обложка
Авторы:
Kyuregyan Karen K., Kichatova Vera S., Isaeva Olga V., Potemkin Ilya A., Malinnikova Elena Y., Karlsen Anastasia A., Mikhailov Mikhail I., Lopatukhina Maria A., Mobarhan Arman A., Mullin Evgeny V., Slukinova Olga Sergeevna, Ignateva Margarita E., Sleptsova Snezhana, Oglezneva Elena E., Shibrik E. V., Isaguliants Maria G.
Заглавие: Coverage with Timely Administered Vaccination against Hepatitis B Virus and Its Influence on the Prevalence of HBV Infection in the Regions of Different Endemicity

Количество страниц: 15 с.

Coverage with Timely Administered Vaccination against Hepatitis B Virus and Its Influence on the Prevalence of HBV Infection in the Regions of Different Endemicity / K. K. Kyuregyan, V. S. Kichatova, O. V.Isaeva [and etc.] // Vaccines. - 2021. - Т. 9, N 2. - С. 1-15. - DOI: 10.3390/vaccines9020082
DOI: 10.3390/vaccines9020082

Подробнее
26.
Обложка
Авторы:
Makarov George A., Baishev Dmitriy G., Moiseyev Aleksey V., Solovyev Stepan I., Pilipenko V. A., Engebretson Mark, Yumoto Kiyohumi
Заглавие: High-latitude peculiarities of the geomagnetic SI impulse propagation meridional velocity during sharp decrease of solar wind density

Количество страниц: 4 с.

The geomagnetic manifestation of sudden impulse (SI) caused by a sharp decrease of the solar wind dynamic pressure due to the plasma density reduction is considered. The observational data of the magnetometer world network have been analysed. The propagation velocities of the SI signal in the meridional direction by using data of the horizontal component of geomagnetic field in the high-latitude region have been calculated. It is found that at a sharp decrease of the solar wind density the meridional propagation of the SI signal is in the northern direction. In this case, on the day side the propagation velocity is constant but there is a tendency of its increasing in the MLT morning sector. It has been established that the meridional propagation velocity of the SI signal at a sharp decrease of the solar wind density depends on the geomagnetic latitude, i.e. with the rise of latitude the velocity in the auroral zone decreases and in the polar cap it increases.

High-latitude peculiarities of the geomagnetic SI impulse propagation meridional velocity during sharp decrease of solar wind density / G. A. Makarov, D. G. Baishev, A. V. Moiseyev, S. I. Solovyev, V. A. Pilipenko, M. J. Engebretson, K. Yumoto // Proceedings of the Fifth International Conference on Substorms : 16-20 May 2000 Congress Centre of the Arctic and Antarctic Research Institute, St. Petersburg, Russia. − Noordwijk, Netherlands : European Space Agency, 2000. − P. 523-526.

Подробнее
27.
Обложка
Авторы:
Makarov George Afanasyevich, Moiseyev Aleksey Vladimirovich, Solovyev Stepan Ivanovich
Заглавие: Propagation velocities of geomagnetic sudden impulses caused by sharp changes jf solar wind dinamic pressure at high latitudes

Количество страниц: 1 с.

Makarov, G. A. Propagation velocities of geomagnetic sudden impulses caused by sharp changes jf solar wind dinamic pressure at high latitudes / G. A. Makarov, V. Moiseev, and S. I. Solovyev // The First S-Ramp Conference, October 2-6, 2000: Sapporo, Japan. – Sapporo, 2000. – P. 122.

Подробнее
28.
Обложка
Авторы:
Malov Sergey I., Baatarkhuu Oidov, Sleptsova Snezhana S., Savilov E. D., Rasulov Rodion I., Malov Igor V.
Заглавие: Risk factors for hepatocellular carcinoma in men of northeast regions of Asia with high, medium, and low incidence rates

Количество страниц: 1 с.

Risk factors for hepatocellular carcinoma in men of northeast regions of Asia with high, medium, and low incidence rates / Malov Sergey, Baatarkhuu Oidov, Sleptsova Snezhana [and etc.] // Hepatology International. - 2020. - Т. 14, N S1. - С. 252.
DOI: 10.1007/s12072-020-10030-4

Подробнее
29.
Обложка
Авторы:
Mishin Vilen M., Foerster M., Saifudinova Tamara Ivanovna, Bazarzhapov Alexander Dashitsyrenovich, Sapronova Lyudmila Alexandrovna, Golovkov Vadim Petrovich, Stauning P., Watermann J., Solovyev Stepan Ivanovich
Заглавие: Dynamics of the Field-Aligned Current Systems Observed during The Super-Storm on Nov. 20, 2003

Количество страниц: 4 с.

Spatial distribution in the polar ionosphere of field-aligned currents density is studied by using data of the events on 20.11.03. Observable distributions are described in terms of three Regions of Iijima and Potemra, with taken into account in each Region of three types of spatial inhomogeneities. These inhomogeneitie were overlooked earlier. Dynamics of classical substorm current wedge SCW1, and the "current wedges" SCW2 and SCW3, both creating a polarization and amplification of the westward auroral electrojet, are described.

Dynamics of the Field-Aligned Current Systems Observed during The Super-Storm on Nov. 20, 2003 / 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. 79-82.

Подробнее
30.
Обложка
Авторы:
Mishin Vilen M., Foerster M., Saifudinova Tamara Ivanovna, Bazarzhapov Alexander Dashitsyrenovich, Sapronova Lyudmila Alexandrovna, Golovkov Vadim Petrovich, Stauning P., Watermann J., Solovyev Stepan Ivanovich
Заглавие: Basic Regimes of the Super-Storm on Nov 20, 2003 and the Problems Substorms-Storm

Количество страниц: 4 с.

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.

Подробнее