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Bruce T. Tsurutani
Researcher at California Institute of Technology
Publications - 623
Citations - 33600
Bruce T. Tsurutani is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Solar wind & Interplanetary magnetic field. The author has an hindex of 85, co-authored 605 publications receiving 30358 citations. Previous affiliations of Bruce T. Tsurutani include University of Concepción & National Institute for Space Research.
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What is a geomagnetic storm
Walter D. Gonzalez,J. A. Joselyn,Yohsuke Kamide,H. W. Kroehl,Gordon Rostoker,Bruce T. Tsurutani,Vytenis M. Vasyliunas +6 more
TL;DR: In this article, an attempt is made to define a geomagnetic storm as an interval of time when a sufficiently intense and long-lasting interplanetary convection electric field leads, through a substantial energization in the magnetosphere-ionosphere system, to an intensified ring current sufficiently strong to exceed some key threshold of the quantifying storm time Dst index.
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Postmidnight chorus: A substorm phenomenon
TL;DR: In this paper, the post-midnight chorus was detected in the midnight sector of the magnetosphere in conjunction with magnetospheric substorms and the characteristics of these emissions such as their frequency time structure, emission frequency with respect to the local equatorial electron gyrofrequency, intensity-time variation, and the average intensity were investigated.
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Origin of interplanetary southward magnetic fields responsible for major magnetic storms near solar maximum (1978–1979)
TL;DR: In this article, simultaneous ISEE-3 field and plasma data were used to examine interplanetary phenomena associated with 10 major magnetic storms detected from August 16, 1978, to December 28, 1979, in a study of Gonzalez and Tsurutani (1987), and, in particular, to determine the origins of the southward magnetic fields which caused the storms.
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Interplanetary origin of geomagnetic storms
TL;DR: In this article, the authors examined the effects of a combination of a long-duration southward sheath magnetic field, followed by a magnetic cloud Bs event, and showed that double, and sometimes triple, IMF Bs events are important causes of such events.
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Corotating solar wind streams and recurrent geomagnetic activity: A review
Bruce T. Tsurutani,Bruce T. Tsurutani,Walter D. Gonzalez,Alicia L. Clúa de Gonzalez,Fernando L. Guarnieri,Nat Gopalswamy,Manuel Grande,Yohsuke Kamide,Yoshiya Kasahara,Gang Lu,Ian R. Mann,Robert L. McPherron,Finn Søraas,Vytenis M. Vasyliunas +13 more
TL;DR: In this paper, it was shown that geomagnetic storms associated with high-speed streams/CIRs will have the same initial, main, and recovery phases as those associated with ICME-related magnetic storms but that the interplanetary causes are considerably different.