Angular distribution of discontinuity normals of the interplanetary magnetic field

K. Lukács, G. Erdős

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

High time resolved (6 s) magnetic field data from the Helios-1 and Ulysses spacecrafts were used to investigate MHD discontinuities in the heliosphere. The identification of discontinuities was based on the rotation of the field vectors relative to the distance to the plasma in which the vectors were supposed to be frozen. In order to obtain the real thickness of the discontinuity transition region, the surface normal of discontinuities were calculated by both the minimum variance and cross-product methods. We found an anisotropy in the angular distribution of the discontinuity surface normals in the heliosphere where the average interplanetary magnetic field is close to radial. It is an indirect evidence that most of the discontinuities are tangential rather than rotational ones. This result is also supported by the fact that the Minimum Variance and Cross-Product methods gave similar results for the determination of the surface normals.

Original languageEnglish
Pages (from-to)1055-1058
Number of pages4
JournalAstronomische Nachrichten
Volume334
Issue number9
DOIs
Publication statusPublished - Nov 2013

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interplanetary magnetic fields
discontinuity
angular distribution
magnetic field
heliosphere
Helios 1
products
distribution
spacecraft
anisotropy
plasma
magnetic fields

Keywords

  • Interplanetary medium
  • Magnetic fields
  • Magnetohydrodynamics (MHD)
  • Solar wind
  • Waves

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Angular distribution of discontinuity normals of the interplanetary magnetic field. / Lukács, K.; Erdős, G.

In: Astronomische Nachrichten, Vol. 334, No. 9, 11.2013, p. 1055-1058.

Research output: Contribution to journalArticle

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