Solar wind variation with the cycle

I. S. Veselovsky, A. V. Dmitriev, A. V. Suvorova, M. V. Tarsina

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

The cyclic evolution of the heliospheric plasma parameters is related to the time-dependent boundary conditions in the solar corona. "Minimal" coronal configurations correspond to the regular appearance of the tenuous, but hot and fast plasma streams from the large polar coronal holes. The denser, but cooler and slower solar wind is adjacent to coronal streamers. Irregular dynamic manifestations are present in the corona and the solar wind everywhere and always. They follow the solar activity cycle rather well. Because of this, the direct and indirect solar wind measurements demonstrate clear variations in space and time according to the minimal, intermediate and maximal conditions of the cycles. The average solar wind density, velocity and temperature measured at the Earth's orbit show specific decadal variations and trends, which are of the order of the first tens per cent during the last three solar cycles. Statistical, spectral and correlation characteristics of the solar wind are reviewed with the emphasis on the cycles.

Original languageEnglish
Pages (from-to)423-429
Number of pages7
JournalJournal of Astrophysics and Astronomy
Volume21
Issue number3-4
DOIs
StatePublished - 2000

Keywords

  • Solar activity cycle
  • Solar wind

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