T
T. S. Horbury
Researcher at Imperial College London
Publications - 32
Citations - 1851
T. S. Horbury is an academic researcher from Imperial College London. The author has contributed to research in topics: Solar wind & Heliosphere. The author has an hindex of 22, co-authored 32 publications receiving 1771 citations. Previous affiliations of T. S. Horbury include Queen Mary University of London.
Papers
More filters
Journal ArticleDOI
The heliospheric magnetic field over the South polar region of the sun.
André Balogh,David J. Southwood,R. J. Forsyth,T. S. Horbury,Edward J. Smith,Bruce T. Tsurutani +5 more
TL;DR: Magnetic field measurements from the Ulysses space mission showed that the structure and properties of the three-dimensional heliosphere were determined by the fast solar wind flow and magnetic fields from the large coronal holes in the polar regions of the sun.
Journal ArticleDOI
Properties of magnetohydrodynamic turbulence in the solar wind as observed by Ulysses at high heliographic latitudes
Bruce E. Goldstein,Edward J. Smith,André Balogh,T. S. Horbury,Melvyn L. Goldstein,D. A. Roberts +5 more
TL;DR: The Ulysses mission as mentioned in this paper provides an opportunity to study the evolution of magnetohydrodynamic (MHD) turbulence in pure high-speed solar wind streams, and the results constrain current theories of MHD turbulence in the solar wind.
Journal Article
Properties of Magnetohydrodynamic Turbulence in the Solar Wind as Observed
TL;DR: The Ulysses mission as discussed by the authors provides an opportunity to study the evolution of magnetohydrodynamic (MHD) turbulence in pure high-speed solar wind streams, and the results constrain current theories of MHD turbulence in the solar wind.
Journal ArticleDOI
Three spacecraft observations of solar wind discontinuities
TL;DR: In this paper, the Tsurutani-Smith method was used to detect rotational magnetic field discontinuities from inter-spacecraft timings of three spacecraft, Geotail, Wind and IMP 8, during 5 days when they were between 6 × 104 and 4 × 105 km.
Journal ArticleDOI
Heliospheric magnetic field polarity inversions at high heliographic latitudes
TL;DR: The heliospheric magnetic field over the poles of the sun has been examined to identify intervals when the polarity of the magnetic field deviates significantly from the calculated Parker spiral as mentioned in this paper.