A year later: Solar, heliospheric, and magnetospheric disturbances in November 2004

Yu I. Yermolaev; L. M. Zelenyi; G. N. Zastenker; A. A. Petrukovich; M. Yu Yermolaev; N. S. Nikolaeva; M. I. Panasyuk; S. N. Kuznetsov; I. N. Myagkova; E. A. Murav'eva; B. Yu Yushkov; I. S. Veselovsky; A. V. Dmitriev; A. N. Zhukov; O. S. Yakovchouk; V. D. Kuznetsov; I. M. Chertok; V. N. Ishkov; A. V. Belov; E. A. Eroshenko; V. G. Yanke; S. P. Gaidash; Kh D. Kanonidi; S. V. Kuzin; I. A. Zhitnik; A. P. Ignat'ev; V. A. Slemzin; N. K. Sukhodrev; S. A. Shestov; M. V. Eselevich; V. G. Eselevich; G. V. Rudenko; V. M. Dvornikov; V. E. Sdobnov; M. V. Kravtsova; V. M. Bogod; V. S. Kotel'nikov; L. A. Pershakov; M. I. Beloglazov; V. I. Vlasov; I. V. Chashei; N. G. Kleimenova; O. V. Kozyreva; V. I. Kozlov; V. A. Parkhomov; Yu A. Kugaenko; R. Z. Khisamov; V. L. Yanchukovskii; K. Kudela

A year later: Solar, heliospheric, and magnetospheric disturbances in November 2004

Yu I. Yermolaev, L. M. Zelenyi, G. N. Zastenker, A. A. Petrukovich, M. Yu Yermolaev, N. S. Nikolaeva, M. I. Panasyuk, S. N. Kuznetsov, I. N. Myagkova, E. A. Murav'eva, B. Yu Yushkov, I. S. Veselovsky, A. V. Dmitriev, A. N. Zhukov, O. S. Yakovchouk, V. D. Kuznetsov, I. M. Chertok, V. N. Ishkov, A. V. Belov, E. A. EroshenkoV. G. Yanke, S. P. Gaidash, Kh D. Kanonidi, S. V. Kuzin, I. A. Zhitnik, A. P. Ignat'ev, V. A. Slemzin, N. K. Sukhodrev, S. A. Shestov, M. V. Eselevich, V. G. Eselevich, G. V. Rudenko, V. M. Dvornikov, V. E. Sdobnov, M. V. Kravtsova, V. M. Bogod, V. S. Kotel'nikov, L. A. Pershakov, M. I. Beloglazov, V. I. Vlasov, I. V. Chashei, N. G. Kleimenova, O. V. Kozyreva, V. I. Kozlov, V. A. Parkhomov, Yu A. Kugaenko, R. Z. Khisamov, V. L. Yanchukovskii, K. Kudela

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

47 引文斯高帕斯（Scopus）

摘要

A year after the extreme events on the Sun, in the heliosphere, and on the Earth in October-November 2003 [Veselovsky et al., 2004; Panasyuk et al., 2004; Yermolaev et al., 2005], a similar situation was also observed in November 2004. The main data observed when the strongest magnetic storm with Dst = -373 nT occurred on the Earth are presented in the paper prepared mainly by the participants of the last year's collaboration of native researchers of extreme events. The disturbance of the Sun, solar wind, and magnetosphere during the considered period was weaker than during the similar period in 2003 with respect to a number of parameters; nevertheless, the presented data indicate that the decline phase of solar cycle 23 is one of the most active intervals over the entire period of comprehensive studies of the solar-terrestrial coupling owing to the events that occurred in autumn 2003 and 2004.

原文	???core.languages.en_GB???
頁（從 - 到）	681-719
頁數	39
期刊	Geomagnetism and Aeronomy
卷	45
發行號	6
出版狀態	已出版 - 11月 2005

引用此

Yermolaev, Y. I., Zelenyi, L. M., Zastenker, G. N., Petrukovich, A. A., Yermolaev, M. Y., Nikolaeva, N. S., Panasyuk, M. I., Kuznetsov, S. N., Myagkova, I. N., Murav'eva, E. A., Yushkov, B. Y., Veselovsky, I. S., Dmitriev, A. V., Zhukov, A. N., Yakovchouk, O. S., Kuznetsov, V. D., Chertok, I. M., Ishkov, V. N., Belov, A. V., ... Kudela, K. (2005). A year later: Solar, heliospheric, and magnetospheric disturbances in November 2004. Geomagnetism and Aeronomy, 45(6), 681-719.

@article{61ac94e507a642288dfabdd67d78999b,

title = "A year later: Solar, heliospheric, and magnetospheric disturbances in November 2004",

abstract = "A year after the extreme events on the Sun, in the heliosphere, and on the Earth in October-November 2003 [Veselovsky et al., 2004; Panasyuk et al., 2004; Yermolaev et al., 2005], a similar situation was also observed in November 2004. The main data observed when the strongest magnetic storm with Dst = -373 nT occurred on the Earth are presented in the paper prepared mainly by the participants of the last year's collaboration of native researchers of extreme events. The disturbance of the Sun, solar wind, and magnetosphere during the considered period was weaker than during the similar period in 2003 with respect to a number of parameters; nevertheless, the presented data indicate that the decline phase of solar cycle 23 is one of the most active intervals over the entire period of comprehensive studies of the solar-terrestrial coupling owing to the events that occurred in autumn 2003 and 2004.",

author = "Yermolaev, {Yu I.} and Zelenyi, {L. M.} and Zastenker, {G. N.} and Petrukovich, {A. A.} and Yermolaev, {M. Yu} and Nikolaeva, {N. S.} and Panasyuk, {M. I.} and Kuznetsov, {S. N.} and Myagkova, {I. N.} and Murav'eva, {E. A.} and Yushkov, {B. Yu} and Veselovsky, {I. S.} and Dmitriev, {A. V.} and Zhukov, {A. N.} and Yakovchouk, {O. S.} and Kuznetsov, {V. D.} and Chertok, {I. M.} and Ishkov, {V. N.} and Belov, {A. V.} and Eroshenko, {E. A.} and Yanke, {V. G.} and Gaidash, {S. P.} and Kanonidi, {Kh D.} and Kuzin, {S. V.} and Zhitnik, {I. A.} and Ignat'ev, {A. P.} and Slemzin, {V. A.} and Sukhodrev, {N. K.} and Shestov, {S. A.} and Eselevich, {M. V.} and Eselevich, {V. G.} and Rudenko, {G. V.} and Dvornikov, {V. M.} and Sdobnov, {V. E.} and Kravtsova, {M. V.} and Bogod, {V. M.} and Kotel'nikov, {V. S.} and Pershakov, {L. A.} and Beloglazov, {M. I.} and Vlasov, {V. I.} and Chashei, {I. V.} and Kleimenova, {N. G.} and Kozyreva, {O. V.} and Kozlov, {V. I.} and Parkhomov, {V. A.} and Kugaenko, {Yu A.} and Khisamov, {R. Z.} and Yanchukovskii, {V. L.} and K. Kudela",

year = "2005",

month = nov,

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

volume = "45",

pages = "681--719",

journal = "Geomagnetism and Aeronomy",

issn = "0016-7932",

number = "6",

}

Yermolaev, YI, Zelenyi, LM, Zastenker, GN, Petrukovich, AA, Yermolaev, MY, Nikolaeva, NS, Panasyuk, MI, Kuznetsov, SN, Myagkova, IN, Murav'eva, EA, Yushkov, BY, Veselovsky, IS, Dmitriev, AV, Zhukov, AN, Yakovchouk, OS, Kuznetsov, VD, Chertok, IM, Ishkov, VN, Belov, AV, Eroshenko, EA, Yanke, VG, Gaidash, SP, Kanonidi, KD, Kuzin, SV, Zhitnik, IA, Ignat'ev, AP, Slemzin, VA, Sukhodrev, NK, Shestov, SA, Eselevich, MV, Eselevich, VG, Rudenko, GV, Dvornikov, VM, Sdobnov, VE, Kravtsova, MV, Bogod, VM, Kotel'nikov, VS, Pershakov, LA, Beloglazov, MI, Vlasov, VI, Chashei, IV, Kleimenova, NG, Kozyreva, OV, Kozlov, VI, Parkhomov, VA, Kugaenko, YA, Khisamov, RZ, Yanchukovskii, VL & Kudela, K 2005, 'A year later: Solar, heliospheric, and magnetospheric disturbances in November 2004', Geomagnetism and Aeronomy, 卷 45, 編號 6, 頁 681-719.

TY - JOUR

T1 - A year later

T2 - Solar, heliospheric, and magnetospheric disturbances in November 2004

AU - Yermolaev, Yu I.

AU - Zelenyi, L. M.

AU - Zastenker, G. N.

AU - Petrukovich, A. A.

AU - Yermolaev, M. Yu

AU - Nikolaeva, N. S.

AU - Panasyuk, M. I.

AU - Kuznetsov, S. N.

AU - Myagkova, I. N.

AU - Murav'eva, E. A.

AU - Yushkov, B. Yu

AU - Veselovsky, I. S.

AU - Dmitriev, A. V.

AU - Zhukov, A. N.

AU - Yakovchouk, O. S.

AU - Kuznetsov, V. D.

AU - Chertok, I. M.

AU - Ishkov, V. N.

AU - Belov, A. V.

AU - Eroshenko, E. A.

AU - Yanke, V. G.

AU - Gaidash, S. P.

AU - Kanonidi, Kh D.

AU - Kuzin, S. V.

AU - Zhitnik, I. A.

AU - Ignat'ev, A. P.

AU - Slemzin, V. A.

AU - Sukhodrev, N. K.

AU - Shestov, S. A.

AU - Eselevich, M. V.

AU - Eselevich, V. G.

AU - Rudenko, G. V.

AU - Dvornikov, V. M.

AU - Sdobnov, V. E.

AU - Kravtsova, M. V.

AU - Bogod, V. M.

AU - Kotel'nikov, V. S.

AU - Pershakov, L. A.

AU - Beloglazov, M. I.

AU - Vlasov, V. I.

AU - Chashei, I. V.

AU - Kleimenova, N. G.

AU - Kozyreva, O. V.

AU - Kozlov, V. I.

AU - Parkhomov, V. A.

AU - Kugaenko, Yu A.

AU - Khisamov, R. Z.

AU - Yanchukovskii, V. L.

AU - Kudela, K.

PY - 2005/11

Y1 - 2005/11

N2 - A year after the extreme events on the Sun, in the heliosphere, and on the Earth in October-November 2003 [Veselovsky et al., 2004; Panasyuk et al., 2004; Yermolaev et al., 2005], a similar situation was also observed in November 2004. The main data observed when the strongest magnetic storm with Dst = -373 nT occurred on the Earth are presented in the paper prepared mainly by the participants of the last year's collaboration of native researchers of extreme events. The disturbance of the Sun, solar wind, and magnetosphere during the considered period was weaker than during the similar period in 2003 with respect to a number of parameters; nevertheless, the presented data indicate that the decline phase of solar cycle 23 is one of the most active intervals over the entire period of comprehensive studies of the solar-terrestrial coupling owing to the events that occurred in autumn 2003 and 2004.

AB - A year after the extreme events on the Sun, in the heliosphere, and on the Earth in October-November 2003 [Veselovsky et al., 2004; Panasyuk et al., 2004; Yermolaev et al., 2005], a similar situation was also observed in November 2004. The main data observed when the strongest magnetic storm with Dst = -373 nT occurred on the Earth are presented in the paper prepared mainly by the participants of the last year's collaboration of native researchers of extreme events. The disturbance of the Sun, solar wind, and magnetosphere during the considered period was weaker than during the similar period in 2003 with respect to a number of parameters; nevertheless, the presented data indicate that the decline phase of solar cycle 23 is one of the most active intervals over the entire period of comprehensive studies of the solar-terrestrial coupling owing to the events that occurred in autumn 2003 and 2004.

UR - http://www.scopus.com/inward/record.url?scp=30744456827&partnerID=8YFLogxK

M3 - 期刊論文

AN - SCOPUS:30744456827

SN - 0016-7932

VL - 45

SP - 681

EP - 719

JO - Geomagnetism and Aeronomy

JF - Geomagnetism and Aeronomy

IS - 6

ER -

A year later: Solar, heliospheric, and magnetospheric disturbances in November 2004

摘要

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