Number density structures in the inner heliosphere

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Stansby, D.; Horbury, T. S.;
  • Related identifiers: doi: 10.1051/0004-6361/201732567
  • Subject: Physics - Space Physics | Physics - Plasma Physics
    arxiv: Physics::Space Physics | Astrophysics::Solar and Stellar Astrophysics

The origins and generation mechanisms of the slow solar wind are still unclear. Part of the slow solar wind is populated by "number density structures", discrete patches of increased number density that are frozen in to and move with the bulk solar wind. In this paper w... View more
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