Solar and heliospheric disturbances that resulted in the strongest magnetic storm of November 20, 2003

Yu I. Ermolaev; L. M. Zelenyi; G. N. Zastenker; A. A. Petrukovich; I. G. Mitrofanov; M. L. Litvak; I. S. Veselovsky; M. I. Panasyuk; L. L. Lazutin; A. V. Dmitriev; A. N. Zhukov; S. N. Kuznetsov; I. N. Myagkova; B. Yu Yushkov; V. G. Kurt; A. A. Gnezdilov; R. V. Gorgutsa; A. K. Markeev; D. E. Sobolev; V. V. Fomichev; V. D. Kuznetsov; S. I. Boldyrev; I. M. Chertok; K. A. Boyarchuk; I. V. Krasheninnikov; O. P. Kolomiitsev; L. N. Leshchenko; A. V. Belov; S. P. Gaidash; Kh D. Kanonidi; S. A. Bogachev; I. A. Zhitnik; A. P. Ignat'ev; S. V. Kuzin; S. N. Oparin; A. A. Pertsov; V. A. Selemzin; N. K. Sukhodrev; S. V. Shestov; V. I. Vlasov; I. V. Chashei; E. V. Vashenyuk; Ya A. Sakharov; A. N. Danilin; V. M. Bogod; S. Kh Tokhchukova; A. V. Mikhalev; A. B. Beletskii; N. V. Kostyleva; M. A. Chernigovskaya; V. V. Grechnev; K. Kudela

Solar and heliospheric disturbances that resulted in the strongest magnetic storm of November 20, 2003

Yu I. Ermolaev, L. M. Zelenyi, G. N. Zastenker, A. A. Petrukovich, I. G. Mitrofanov, M. L. Litvak, I. S. Veselovsky, M. I. Panasyuk, L. L. Lazutin, A. V. Dmitriev, A. N. Zhukov, S. N. Kuznetsov, I. N. Myagkova, B. Yu Yushkov, V. G. Kurt, A. A. Gnezdilov, R. V. Gorgutsa, A. K. Markeev, D. E. Sobolev, V. V. FomichevV. D. Kuznetsov, S. I. Boldyrev, I. M. Chertok, K. A. Boyarchuk, I. V. Krasheninnikov, O. P. Kolomiitsev, L. N. Leshchenko, A. V. Belov, S. P. Gaidash, Kh D. Kanonidi, S. A. Bogachev, I. A. Zhitnik, A. P. Ignat'ev, S. V. Kuzin, S. N. Oparin, A. A. Pertsov, V. A. Selemzin, N. K. Sukhodrev, S. V. Shestov, V. I. Vlasov, I. V. Chashei, E. V. Vashenyuk, Ya A. Sakharov, A. N. Danilin, V. M. Bogod, S. Kh Tokhchukova, A. V. Mikhalev, A. B. Beletskii, N. V. Kostyleva, M. A. Chernigovskaya, V. V. Grechnev, K. Kudela

Department of Space Science and Engineering

Research output: Contribution to journal › Article › peer-review

38 Scopus citations

Abstract

The main data on observations of the Sun, interplanetary medium, and magnetosphere, obtained mainly by home researchers during the strongest magnetic storm of November 20, 2003 (Dst = -472 nT), are presented in the work. This period corresponds to the next earthward turning of the active side of the Sun that generated the series of the strongest solar flares (including flares of class > X17) and the magnetic storm with Dst = -401 nT from the end of October to the beginning of November 2003. Although the number and power of the flares were much smaller during the period under study, the magnetic storm was the second strongest for the entire period of observation of the Dst index and was apparently caused by the interaction of frequently occurred coronal mass ejections in the interplanetary space, as a result of which the region of interaction compressed and the southern IMF component increased to less than -45 nT.

Original language	English
Pages (from-to)	20-46
Number of pages	27
Journal	Geomagnetism and Aeronomy
Volume	45
Issue number	1
State	Published - Jan 2005

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Ermolaev, Y. I., Zelenyi, L. M., Zastenker, G. N., Petrukovich, A. A., Mitrofanov, I. G., Litvak, M. L., Veselovsky, I. S., Panasyuk, M. I., Lazutin, L. L., Dmitriev, A. V., Zhukov, A. N., Kuznetsov, S. N., Myagkova, I. N., Yushkov, B. Y., Kurt, V. G., Gnezdilov, A. A., Gorgutsa, R. V., Markeev, A. K., Sobolev, D. E., ... Kudela, K. (2005). Solar and heliospheric disturbances that resulted in the strongest magnetic storm of November 20, 2003. Geomagnetism and Aeronomy, 45(1), 20-46.

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title = "Solar and heliospheric disturbances that resulted in the strongest magnetic storm of November 20, 2003",

abstract = "The main data on observations of the Sun, interplanetary medium, and magnetosphere, obtained mainly by home researchers during the strongest magnetic storm of November 20, 2003 (Dst = -472 nT), are presented in the work. This period corresponds to the next earthward turning of the active side of the Sun that generated the series of the strongest solar flares (including flares of class > X17) and the magnetic storm with Dst = -401 nT from the end of October to the beginning of November 2003. Although the number and power of the flares were much smaller during the period under study, the magnetic storm was the second strongest for the entire period of observation of the Dst index and was apparently caused by the interaction of frequently occurred coronal mass ejections in the interplanetary space, as a result of which the region of interaction compressed and the southern IMF component increased to less than -45 nT.",

author = "Ermolaev, {Yu I.} and Zelenyi, {L. M.} and Zastenker, {G. N.} and Petrukovich, {A. A.} and Mitrofanov, {I. G.} and Litvak, {M. L.} and Veselovsky, {I. S.} and Panasyuk, {M. I.} and Lazutin, {L. L.} and Dmitriev, {A. V.} and Zhukov, {A. N.} and Kuznetsov, {S. N.} and Myagkova, {I. N.} and Yushkov, {B. Yu} and Kurt, {V. G.} and Gnezdilov, {A. A.} and Gorgutsa, {R. V.} and Markeev, {A. K.} and Sobolev, {D. E.} and Fomichev, {V. V.} and Kuznetsov, {V. D.} and Boldyrev, {S. I.} and Chertok, {I. M.} and Boyarchuk, {K. A.} and Krasheninnikov, {I. V.} and Kolomiitsev, {O. P.} and Leshchenko, {L. N.} and Belov, {A. V.} and Gaidash, {S. P.} and Kanonidi, {Kh D.} and Bogachev, {S. A.} and Zhitnik, {I. A.} and Ignat'ev, {A. P.} and Kuzin, {S. V.} and Oparin, {S. N.} and Pertsov, {A. A.} and Selemzin, {V. A.} and Sukhodrev, {N. K.} and Shestov, {S. V.} and Vlasov, {V. I.} and Chashei, {I. V.} and Vashenyuk, {E. V.} and Sakharov, {Ya A.} and Danilin, {A. N.} and Bogod, {V. M.} and Tokhchukova, {S. Kh} and Mikhalev, {A. V.} and Beletskii, {A. B.} and Kostyleva, {N. V.} and Chernigovskaya, {M. A.} and Grechnev, {V. V.} and K. Kudela",

year = "2005",

month = jan,

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

volume = "45",

pages = "20--46",

journal = "Geomagnetism and Aeronomy",

issn = "0016-7932",

number = "1",

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Ermolaev, YI, Zelenyi, LM, Zastenker, GN, Petrukovich, AA, Mitrofanov, IG, Litvak, ML, Veselovsky, IS, Panasyuk, MI, Lazutin, LL, Dmitriev, AV, Zhukov, AN, Kuznetsov, SN, Myagkova, IN, Yushkov, BY, Kurt, VG, Gnezdilov, AA, Gorgutsa, RV, Markeev, AK, Sobolev, DE, Fomichev, VV, Kuznetsov, VD, Boldyrev, SI, Chertok, IM, Boyarchuk, KA, Krasheninnikov, IV, Kolomiitsev, OP, Leshchenko, LN, Belov, AV, Gaidash, SP, Kanonidi, KD, Bogachev, SA, Zhitnik, IA, Ignat'ev, AP, Kuzin, SV, Oparin, SN, Pertsov, AA, Selemzin, VA, Sukhodrev, NK, Shestov, SV, Vlasov, VI, Chashei, IV, Vashenyuk, EV, Sakharov, YA, Danilin, AN, Bogod, VM, Tokhchukova, SK, Mikhalev, AV, Beletskii, AB, Kostyleva, NV, Chernigovskaya, MA, Grechnev, VV & Kudela, K 2005, 'Solar and heliospheric disturbances that resulted in the strongest magnetic storm of November 20, 2003', Geomagnetism and Aeronomy, vol. 45, no. 1, pp. 20-46.

TY - JOUR

T1 - Solar and heliospheric disturbances that resulted in the strongest magnetic storm of November 20, 2003

AU - Ermolaev, Yu I.

AU - Zelenyi, L. M.

AU - Zastenker, G. N.

AU - Petrukovich, A. A.

AU - Mitrofanov, I. G.

AU - Litvak, M. L.

AU - Veselovsky, I. S.

AU - Panasyuk, M. I.

AU - Lazutin, L. L.

AU - Dmitriev, A. V.

AU - Zhukov, A. N.

AU - Kuznetsov, S. N.

AU - Myagkova, I. N.

AU - Yushkov, B. Yu

AU - Kurt, V. G.

AU - Gnezdilov, A. A.

AU - Gorgutsa, R. V.

AU - Markeev, A. K.

AU - Sobolev, D. E.

AU - Fomichev, V. V.

AU - Kuznetsov, V. D.

AU - Boldyrev, S. I.

AU - Chertok, I. M.

AU - Boyarchuk, K. A.

AU - Krasheninnikov, I. V.

AU - Kolomiitsev, O. P.

AU - Leshchenko, L. N.

AU - Belov, A. V.

AU - Gaidash, S. P.

AU - Kanonidi, Kh D.

AU - Bogachev, S. A.

AU - Zhitnik, I. A.

AU - Ignat'ev, A. P.

AU - Kuzin, S. V.

AU - Oparin, S. N.

AU - Pertsov, A. A.

AU - Selemzin, V. A.

AU - Sukhodrev, N. K.

AU - Shestov, S. V.

AU - Vlasov, V. I.

AU - Chashei, I. V.

AU - Vashenyuk, E. V.

AU - Sakharov, Ya A.

AU - Danilin, A. N.

AU - Bogod, V. M.

AU - Tokhchukova, S. Kh

AU - Mikhalev, A. V.

AU - Beletskii, A. B.

AU - Kostyleva, N. V.

AU - Chernigovskaya, M. A.

AU - Grechnev, V. V.

AU - Kudela, K.

PY - 2005/1

Y1 - 2005/1

N2 - The main data on observations of the Sun, interplanetary medium, and magnetosphere, obtained mainly by home researchers during the strongest magnetic storm of November 20, 2003 (Dst = -472 nT), are presented in the work. This period corresponds to the next earthward turning of the active side of the Sun that generated the series of the strongest solar flares (including flares of class > X17) and the magnetic storm with Dst = -401 nT from the end of October to the beginning of November 2003. Although the number and power of the flares were much smaller during the period under study, the magnetic storm was the second strongest for the entire period of observation of the Dst index and was apparently caused by the interaction of frequently occurred coronal mass ejections in the interplanetary space, as a result of which the region of interaction compressed and the southern IMF component increased to less than -45 nT.

AB - The main data on observations of the Sun, interplanetary medium, and magnetosphere, obtained mainly by home researchers during the strongest magnetic storm of November 20, 2003 (Dst = -472 nT), are presented in the work. This period corresponds to the next earthward turning of the active side of the Sun that generated the series of the strongest solar flares (including flares of class > X17) and the magnetic storm with Dst = -401 nT from the end of October to the beginning of November 2003. Although the number and power of the flares were much smaller during the period under study, the magnetic storm was the second strongest for the entire period of observation of the Dst index and was apparently caused by the interaction of frequently occurred coronal mass ejections in the interplanetary space, as a result of which the region of interaction compressed and the southern IMF component increased to less than -45 nT.

UR - http://www.scopus.com/inward/record.url?scp=20144386126&partnerID=8YFLogxK

M3 - 期刊論文

AN - SCOPUS:20144386126

SN - 0016-7932

VL - 45

SP - 20

EP - 46

JO - Geomagnetism and Aeronomy

JF - Geomagnetism and Aeronomy

IS - 1

ER -

Solar and heliospheric disturbances that resulted in the strongest magnetic storm of November 20, 2003

Abstract

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