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  • 1
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    Heliospheric Plasma Sheet and Coronal Streamers (1997)
    In:  Other Sources
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    Publication Date: 2018-06-08
    Description: In-situ measurements of solar wind plasma and magnetic field between 0.3 and 1 AU are used to investigate the structure of the heliospheric plasma sheet, namely the region of enhanced plasma density that surrounds the helioshperic current sheet.
    Keywords: Solar Physics
    Type: Geophysical Research Letters
    Format: text
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    NASA TECHNICAL REPORTS
  • 2
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    Intermittency and extended self-similarity in the solar wind turbulence (1995)
    In:  Other Sources
    Details
    Publication Date: 2019-07-17
    Description: Using the satellite measurements of the velocity field in the interplanetary plasma. we present some analysis which show the presence of a self-similar intermittent state in the solar wind turbulence. We used the so called Extended Self-Similarity hypothesis, which is well visible in the solar wind turbulence, showing convincing evidences for the presence of universal anomalous scaling laws. Through the Extended Self-Similarity we are able to calculate the scaling exponents of the velocity structure functions with very small uncertainties, and we show that these scaling exponents are in very good agreement with the multifractal models describing intermittency in magnetohydrodynamic flows.
    Keywords: Solar Physics
    Type: ; 82
    Format: text
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    NASA TECHNICAL REPORTS
  • 3
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    On the nature of Alfven inward modes in the solar wind (1995)
    In:  Other Sources
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    Publication Date: 2019-07-17
    Description: Within the past decade there has been a remarkable production of papers both theoretical and observational that have shed some light on the intriguing and unsolved problem of the Alfvenic MHD turbulence in the solar wind. Although the scientific community has agreed upon many points which are at the basis of the temporal and radial evolution of the turbulence like the solar origin of most of the outward Alfven modes or the importance of non-linear interactions between outward and inward modes. there are still many open issues which are of fundamental importance for a complete understanding of the phenomenon. One of these key-issues is about the real nature of these inward modes. are they real propagating Alfven waves or rather static structures convected by the wind or a mixture of both? The present analysis represents an effort towards a better understanding of the nature and the role of these modes.
    Keywords: Solar Physics
    Type: ; 38
    Format: text
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