Generalized Squashing Factors for Covariant Description of Magnetic Connectivity in the Solar Corona

By V. Titov. 2007

193 citations recorded by the source corpus.

The study of magnetic connectivity in the solar corona reveals a need to generalize the field line mapping technique to arbitrary geometry of the boundaries and systems of coordinates. Indeed, the global description of the connectivity in the corona requires the use of the photospheric and solar wind boundaries. Both are closed surfaces and therefore do not admit a global regular system of coordinates. At least two overlapping regular systems of coordinates for each of the boundaries are necessary in this case to avoid spherical-pole-like singularities in the coordinates of the footpoints. This implies that the basic characteristic of magnetic connectivity—the squashing degree or factor Q of elemental flux tubes, according to Titov and coworkers—must be rewritten in covariant form. Such a covariant expression of Q is derived in this work. The derived expression is very flexible and highly efficient for describing the global magnetic connectivity in the solar corona. In addition, a general expression for a new characteristic Q⊥, which defines a squashing of the flux tubes in the directions perpendicular to the field lines, is determined. This new quantity makes it possible to filter out the quasi-separatrix layers whose large values of Q are caused by a projection effect at the field lines nearly touching the photosphere. Thus, the value Q⊥ provides a much more precise description of the volumetric properties of the magnetic field structure. The difference between Q and Q⊥ is illustrated by comparing their distributions for two configurations, one of which is the Titov-Démoulin model of a twisted magnetic field.

Subfields: Artificial Intelligence, Astronomy and Astrophysics, Renewable Energy, Sustainability and the Environment

View Paper: https://www.semanticscholar.org/paper/598a14ca404d3193c4224867b6b6e91b970f6b3b

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Citations in the corpus

The standard flare model in three dimensions - III. Slip-running reconnection properties (2013, methodology): “This configuration is a signature of twisted flux tubes, as was shown analytically by Démoulin et al. (1996b) and Titov (2007).”
A MODEL FOR THE SOURCES OF THE SLOW SOLAR WIND (2010, methodology): “The topology of this mapping, as evidenced by structures such as separatrices and QSLs, is most easily seen by analyzing the squashing factor Q (Titov et al. 2002; Titov 2007).”
Three-dimensional magnetic reconnection regimes: a review (2011, background): “These gradients in the connectivity are characterised by the so-called squashing factor, Q (Titov et al., 2002; Titov, 2007), and regions with high values of Q are usually termed quasi-separatrix layers (or QSLs).”