B
Bruce E. Goldstein
Researcher at California Institute of Technology
Publications - 118
Citations - 5539
Bruce E. Goldstein is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Solar wind & Coronal mass ejection. The author has an hindex of 45, co-authored 118 publications receiving 5295 citations.
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Journal ArticleDOI
Solar wind observations over Ulysses' first full polar orbit
David J. McComas,B. L. Barraclough,Herbert O. Funsten,J. T. Gosling,E. Santiago-Muñoz,Ruth M. Skoug,Bruce E. Goldstein,Marcia Neugebauer,Pete Riley,André Balogh +9 more
TL;DR: In this article, the authors examined solar wind plasma and magnetic field observations from Ulysses' first full polar orbit in order to characterize the high-latitude solar wind under conditions of decreasing and low solar activity.
Journal Article
The Ulysses solar wind plasma experiment
S. J. Bame,David J. McComas,B. L. Barraclough,John L. Phillips,K. J. Sofaly,J. C. Chavez,Bruce E. Goldstein,R. K. Sakurai +7 more
TL;DR: The Ulysses solar wind plasma experiment, termed the Solar Wind Observations Over the Poles of the Sun (SWOOPS) as mentioned in this paper, includes measurements of the solar-wind global properties, the nonlinear MHD disturbances in the solar wind, and the internal state of the plasma.
Journal ArticleDOI
Ulysses solar wind plasma observations at high southerly latitudes.
John L. Phillips,S. J. Bame,W. C. Feldman,Bruce E. Goldstein,J. T. Gosling,C. M. Hammond,David J. McComas,Marcia Neugebauer,Earl Scime,Steven T. Suess +9 more
TL;DR: Solar wind plasma observations made by the Ulysses spacecraft through –80.2� solar latitude and continuing equatorward to –40.1� are summarized.
Journal ArticleDOI
A reexamination of rotational and tangential discontinuities in the solar wind
TL;DR: In this article, an analysis is made of interplanetary tangential and rotational solar wind discontinuities (TD and RD) and comparisons are made between the features of RDs and TDs.
Journal ArticleDOI
Ulysses observations of a recurrent high speed solar wind stream and the heliomagnetic streamer belt
S. J. Bame,Bruce E. Goldstein,J. T. Gosling,J. W. Harvey,David J. McComas,Marcia Neugebauer,John L. Phillips +6 more
TL;DR: In this paper, Ulysses encountered a recurrent high-speed stream, that may also have been observed at IMP 8 at 1 AU, and observed it a total of 14 times, once in each solar rotation through June 1993 at approximately 34 deg S. The source of the high speed stream is an equatorward extension of the south polar coronal hole.