Magnetic storms in october 2003

M. I. Panasyuk; S. N. Kuznetsov; L. L. Lazutin; S. I. Avdyushin; I. I. Alexeev; P. P. Ammosov; A. E. Antonova; D. G. Baishev; E. S. Belenkaya; A. B. Beletsky; A. V. Belov; V. V. Benghin; S. Yu Bobrovnikov; V. A. Bondarenko; K. A. Boyarchuk; I. S. Veselovsky; T. Yu Vyushkova; G. A. Gavrilieva; S. P. Gaidash; E. A. Ginzburg; Yu I. Denisov; A. V. Dmitriev; G. A. Zherebtsov; L. M. Zelenyi; G. S. Ivanov-Kholodny; V. V. Kalegaev; Kh D. Kanonidi; N. G. Kleimenova; O. V. Kozyreva; O. P. Kolomiitsev; I. A. Krasheninnikov; A. A. Krivolutsky; A. P. Kropotkin; A. A. Kuminov; L. N. Leshchenko; B. V. Mar'in; V. G. Mitrikas; A. V. Mikhalev; V. A. Mullayarov; E. A. Muravieva; I. N. Myagkova; V. M. Petrov; A. A. Petrukovich; A. N. Podorolsky; M. I. Pudovkin; S. N. Samsonov; Ya A. Sakharov; P. M. Svidsky; V. D. Sokolov; S. I. Soloviev; E. N. Sosnovets; G. V. Starkov; L. I. Starostin; L. V. Tverskaya; M. V. Teltsov; O. A. Troshichev; V. V. Tsetlin; B. Yu Yushkov

doi:10.1023/B:COSM.0000046230.62353.61

Magnetic storms in october 2003

M. I. Panasyuk, S. N. Kuznetsov, L. L. Lazutin, S. I. Avdyushin, I. I. Alexeev, P. P. Ammosov, A. E. Antonova, D. G. Baishev, E. S. Belenkaya, A. B. Beletsky, A. V. Belov, V. V. Benghin, S. Yu Bobrovnikov, V. A. Bondarenko, K. A. Boyarchuk, I. S. Veselovsky, T. Yu Vyushkova, G. A. Gavrilieva, S. P. Gaidash, E. A. GinzburgYu I. Denisov, A. V. Dmitriev, G. A. Zherebtsov, L. M. Zelenyi, G. S. Ivanov-Kholodny, V. V. Kalegaev, Kh D. Kanonidi, N. G. Kleimenova, O. V. Kozyreva, O. P. Kolomiitsev, I. A. Krasheninnikov, A. A. Krivolutsky, A. P. Kropotkin, A. A. Kuminov, L. N. Leshchenko, B. V. Mar'in, V. G. Mitrikas, A. V. Mikhalev, V. A. Mullayarov, E. A. Muravieva, I. N. Myagkova, V. M. Petrov, A. A. Petrukovich, A. N. Podorolsky, M. I. Pudovkin, S. N. Samsonov, Ya A. Sakharov, P. M. Svidsky, V. D. Sokolov, S. I. Soloviev, E. N. Sosnovets, G. V. Starkov, L. I. Starostin, L. V. Tverskaya, M. V. Teltsov, O. A. Troshichev, V. V. Tsetlin, B. Yu Yushkov

太空科學與工程學系

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

50 引文斯高帕斯（Scopus）

摘要

Preliminary results of an analysis of satellite and ground-based measurements during extremely strong magnetic storms at the end of October 2003 are presented, including some numerical modeling. The geo-synchronous satellites Ekspress-A2 and Ekspress-A3, and the low-altitude polar satellites Coronas-F and Meteor-3M carried out measurements of charged particles (electrons, protons, and ions) of solar and magnetospheric origin in a wide energy range. Disturbances of the geomagnetic field caused by extremely high activity on the Sun were studied at more than twenty magnetic stations from Lovozero (Murmansk region) to Tixie (Sakha-Yakutia). Unique data on the dynamics of the ionosphere, riometric absorption, geomagnetic pulsations, and aurora observations at mid-latitudes are obtained.

原文	???core.languages.en_GB???
頁（從 - 到）	489-534
頁數	46
期刊	Cosmic Research
卷	42
發行號	5
DOIs	https://doi.org/10.1023/B:COSM.0000046230.62353.61
出版狀態	已出版 - 9月 2004

存取文件

10.1023/B:COSM.0000046230.62353.61

引用此

Panasyuk, M. I., Kuznetsov, S. N., Lazutin, L. L., Avdyushin, S. I., Alexeev, I. I., Ammosov, P. P., Antonova, A. E., Baishev, D. G., Belenkaya, E. S., Beletsky, A. B., Belov, A. V., Benghin, V. V., Bobrovnikov, S. Y., Bondarenko, V. A., Boyarchuk, K. A., Veselovsky, I. S., Vyushkova, T. Y., Gavrilieva, G. A., Gaidash, S. P., ... Yushkov, B. Y. (2004). Magnetic storms in october 2003. Cosmic Research, 42(5), 489-534. https://doi.org/10.1023/B:COSM.0000046230.62353.61

@article{93b0f5ca230340fdb3949a09d8e9f1ef,

title = "Magnetic storms in october 2003",

abstract = "Preliminary results of an analysis of satellite and ground-based measurements during extremely strong magnetic storms at the end of October 2003 are presented, including some numerical modeling. The geo-synchronous satellites Ekspress-A2 and Ekspress-A3, and the low-altitude polar satellites Coronas-F and Meteor-3M carried out measurements of charged particles (electrons, protons, and ions) of solar and magnetospheric origin in a wide energy range. Disturbances of the geomagnetic field caused by extremely high activity on the Sun were studied at more than twenty magnetic stations from Lovozero (Murmansk region) to Tixie (Sakha-Yakutia). Unique data on the dynamics of the ionosphere, riometric absorption, geomagnetic pulsations, and aurora observations at mid-latitudes are obtained.",

author = "Panasyuk, {M. I.} and Kuznetsov, {S. N.} and Lazutin, {L. L.} and Avdyushin, {S. I.} and Alexeev, {I. I.} and Ammosov, {P. P.} and Antonova, {A. E.} and Baishev, {D. G.} and Belenkaya, {E. S.} and Beletsky, {A. B.} and Belov, {A. V.} and Benghin, {V. V.} and Bobrovnikov, {S. Yu} and Bondarenko, {V. A.} and Boyarchuk, {K. A.} and Veselovsky, {I. S.} and Vyushkova, {T. Yu} and Gavrilieva, {G. A.} and Gaidash, {S. P.} and Ginzburg, {E. A.} and Denisov, {Yu I.} and Dmitriev, {A. V.} and Zherebtsov, {G. A.} and Zelenyi, {L. M.} and Ivanov-Kholodny, {G. S.} and Kalegaev, {V. V.} and Kanonidi, {Kh D.} and Kleimenova, {N. G.} and Kozyreva, {O. V.} and Kolomiitsev, {O. P.} and Krasheninnikov, {I. A.} and Krivolutsky, {A. A.} and Kropotkin, {A. P.} and Kuminov, {A. A.} and Leshchenko, {L. N.} and Mar'in, {B. V.} and Mitrikas, {V. G.} and Mikhalev, {A. V.} and Mullayarov, {V. A.} and Muravieva, {E. A.} and Myagkova, {I. N.} and Petrov, {V. M.} and Petrukovich, {A. A.} and Podorolsky, {A. N.} and Pudovkin, {M. I.} and Samsonov, {S. N.} and Sakharov, {Ya A.} and Svidsky, {P. M.} and Sokolov, {V. D.} and Soloviev, {S. I.} and Sosnovets, {E. N.} and Starkov, {G. V.} and Starostin, {L. I.} and Tverskaya, {L. V.} and Teltsov, {M. V.} and Troshichev, {O. A.} and Tsetlin, {V. V.} and Yushkov, {B. Yu}",

note = "Funding Information: The work was supported by a president grant for leading scientific schools NSh-2046.2003.2 and by the grant “Universities of Russia” no. UR.02.03.035. Funding Information: The work on section 3 was carried out with support of Russian Foundation for Basic Research (grants 01-05-65003, 00-15-96623, 01-07-90117, and 02-05-74643) and a grant of Swedish Academy of sciences. Funding Information: The works on sections 3.1.1 and 3.1.2 were partially supported by RFBR grant 03-05-39011. Irkutsk team was supported by RFBR grant 03-05-64744 and grant NSh-272.2003.5 of State support for leading scientific schools of Russian Federation. Funding Information: The team from Central Aerological Observatory was supported by RFBR grant 03-05-64675. Funding Information: The work on section 3.1.3 was supported by the Program of fundamental research of Division of physical sciences of Russian Academy of sciences “Solar wind: generation and interaction with the Earth and other planets (OFN-18)” and by the RFBR grant 02-05-64386.",

year = "2004",

month = sep,

doi = "10.1023/B:COSM.0000046230.62353.61",

language = "???core.languages.en_GB???",

volume = "42",

pages = "489--534",

journal = "Cosmic Research",

issn = "0010-9525",

number = "5",

}

Panasyuk, MI, Kuznetsov, SN, Lazutin, LL, Avdyushin, SI, Alexeev, II, Ammosov, PP, Antonova, AE, Baishev, DG, Belenkaya, ES, Beletsky, AB, Belov, AV, Benghin, VV, Bobrovnikov, SY, Bondarenko, VA, Boyarchuk, KA, Veselovsky, IS, Vyushkova, TY, Gavrilieva, GA, Gaidash, SP, Ginzburg, EA, Denisov, YI, Dmitriev, AV, Zherebtsov, GA, Zelenyi, LM, Ivanov-Kholodny, GS, Kalegaev, VV, Kanonidi, KD, Kleimenova, NG, Kozyreva, OV, Kolomiitsev, OP, Krasheninnikov, IA, Krivolutsky, AA, Kropotkin, AP, Kuminov, AA, Leshchenko, LN, Mar'in, BV, Mitrikas, VG, Mikhalev, AV, Mullayarov, VA, Muravieva, EA, Myagkova, IN, Petrov, VM, Petrukovich, AA, Podorolsky, AN, Pudovkin, MI, Samsonov, SN, Sakharov, YA, Svidsky, PM, Sokolov, VD, Soloviev, SI, Sosnovets, EN, Starkov, GV, Starostin, LI, Tverskaya, LV, Teltsov, MV, Troshichev, OA, Tsetlin, VV & Yushkov, BY 2004, 'Magnetic storms in october 2003', Cosmic Research, 卷 42, 編號 5, 頁 489-534. https://doi.org/10.1023/B:COSM.0000046230.62353.61

TY - JOUR

T1 - Magnetic storms in october 2003

AU - Panasyuk, M. I.

AU - Kuznetsov, S. N.

AU - Lazutin, L. L.

AU - Avdyushin, S. I.

AU - Alexeev, I. I.

AU - Ammosov, P. P.

AU - Antonova, A. E.

AU - Baishev, D. G.

AU - Belenkaya, E. S.

AU - Beletsky, A. B.

AU - Belov, A. V.

AU - Benghin, V. V.

AU - Bobrovnikov, S. Yu

AU - Bondarenko, V. A.

AU - Boyarchuk, K. A.

AU - Veselovsky, I. S.

AU - Vyushkova, T. Yu

AU - Gavrilieva, G. A.

AU - Gaidash, S. P.

AU - Ginzburg, E. A.

AU - Denisov, Yu I.

AU - Dmitriev, A. V.

AU - Zherebtsov, G. A.

AU - Zelenyi, L. M.

AU - Ivanov-Kholodny, G. S.

AU - Kalegaev, V. V.

AU - Kanonidi, Kh D.

AU - Kleimenova, N. G.

AU - Kozyreva, O. V.

AU - Kolomiitsev, O. P.

AU - Krasheninnikov, I. A.

AU - Krivolutsky, A. A.

AU - Kropotkin, A. P.

AU - Kuminov, A. A.

AU - Leshchenko, L. N.

AU - Mar'in, B. V.

AU - Mitrikas, V. G.

AU - Mikhalev, A. V.

AU - Mullayarov, V. A.

AU - Muravieva, E. A.

AU - Myagkova, I. N.

AU - Petrov, V. M.

AU - Petrukovich, A. A.

AU - Podorolsky, A. N.

AU - Pudovkin, M. I.

AU - Samsonov, S. N.

AU - Sakharov, Ya A.

AU - Svidsky, P. M.

AU - Sokolov, V. D.

AU - Soloviev, S. I.

AU - Sosnovets, E. N.

AU - Starkov, G. V.

AU - Starostin, L. I.

AU - Tverskaya, L. V.

AU - Teltsov, M. V.

AU - Troshichev, O. A.

AU - Tsetlin, V. V.

AU - Yushkov, B. Yu

N1 - Funding Information: The work was supported by a president grant for leading scientific schools NSh-2046.2003.2 and by the grant “Universities of Russia” no. UR.02.03.035. Funding Information: The work on section 3 was carried out with support of Russian Foundation for Basic Research (grants 01-05-65003, 00-15-96623, 01-07-90117, and 02-05-74643) and a grant of Swedish Academy of sciences. Funding Information: The works on sections 3.1.1 and 3.1.2 were partially supported by RFBR grant 03-05-39011. Irkutsk team was supported by RFBR grant 03-05-64744 and grant NSh-272.2003.5 of State support for leading scientific schools of Russian Federation. Funding Information: The team from Central Aerological Observatory was supported by RFBR grant 03-05-64675. Funding Information: The work on section 3.1.3 was supported by the Program of fundamental research of Division of physical sciences of Russian Academy of sciences “Solar wind: generation and interaction with the Earth and other planets (OFN-18)” and by the RFBR grant 02-05-64386.

PY - 2004/9

Y1 - 2004/9

N2 - Preliminary results of an analysis of satellite and ground-based measurements during extremely strong magnetic storms at the end of October 2003 are presented, including some numerical modeling. The geo-synchronous satellites Ekspress-A2 and Ekspress-A3, and the low-altitude polar satellites Coronas-F and Meteor-3M carried out measurements of charged particles (electrons, protons, and ions) of solar and magnetospheric origin in a wide energy range. Disturbances of the geomagnetic field caused by extremely high activity on the Sun were studied at more than twenty magnetic stations from Lovozero (Murmansk region) to Tixie (Sakha-Yakutia). Unique data on the dynamics of the ionosphere, riometric absorption, geomagnetic pulsations, and aurora observations at mid-latitudes are obtained.

AB - Preliminary results of an analysis of satellite and ground-based measurements during extremely strong magnetic storms at the end of October 2003 are presented, including some numerical modeling. The geo-synchronous satellites Ekspress-A2 and Ekspress-A3, and the low-altitude polar satellites Coronas-F and Meteor-3M carried out measurements of charged particles (electrons, protons, and ions) of solar and magnetospheric origin in a wide energy range. Disturbances of the geomagnetic field caused by extremely high activity on the Sun were studied at more than twenty magnetic stations from Lovozero (Murmansk region) to Tixie (Sakha-Yakutia). Unique data on the dynamics of the ionosphere, riometric absorption, geomagnetic pulsations, and aurora observations at mid-latitudes are obtained.

UR - http://www.scopus.com/inward/record.url?scp=7544222913&partnerID=8YFLogxK

U2 - 10.1023/B:COSM.0000046230.62353.61

DO - 10.1023/B:COSM.0000046230.62353.61

M3 - 期刊論文

AN - SCOPUS:7544222913

SN - 0010-9525

VL - 42

SP - 489

EP - 534

JO - Cosmic Research

JF - Cosmic Research

IS - 5

ER -

Magnetic storms in october 2003

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