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Marubashi, K. (1997) Interplanetary Magnetic Flux Ropes and Solar Filaments, Coronal Mass Ejections. In: Crooker, N., Joselyn, J. and Feynman, J., Eds., Geophysical Monograph Series 99, AGU, Washington DC, 147-156.
https://doi.org/10.1029/GM099p0147

has been cited by the following article:

• TITLE: Thermodynamic Interpretation of Electron Density and Temperature Description in the Solar Corona

  AUTHORS: Daniel B. Berdichevsky, Jenny M. Rodríguez Gómez

  KEYWORDS: Solar Corona, Density, Temperature and Polytropic Anomalous Index

  JOURNAL NAME: Advances in Aerospace Science and Technology, Vol.7 No.3, September 30, 2022

  ABSTRACT: We reach a thermodynamic interpretation of the CODET model and its accurate electron density and temperature prediction, grounded on the physics of hydro magnetism in global equilibrium. The thermodynamic interpretation finds consistency with the model of a magneto-matter medium possessing a 3-D Langmuir structure. That medium is diamagnetic in the context of ideal magnetohydrodynamic (MHD). It is shown that this magneto-matter has unusual characteristics consistent with assuming that the low quiescent solar corona possesses a nature-state, non yet studied. It is further noticed that this is wholly consistent with the CODET model prediction of a polytropic anomalous index for the electron gas of the Sun’s corona. Constitutive properties are derived from this novel state of nature, like magnetic permeability properties and non-dispersive acoustic speed. This non-dispersive acoustic speed is also expected to predict the observed equilibration time for the 1.1 to 1.3R⊙ quiescent corona during the solar minimum from 2008 to 2009.