3 Kinetic Description of Corona and Solar Wind

 3.1 Basic energetics of coronal expansion
 3.2 Collisional conditions in the corona and solar wind
 3.3 The exospheric paradigm and related models
 3.4 The failure to heat chromosphere or corona by collisions
 3.5 Dissipation of plasma waves in solar corona and solar wind
 3.6 Basics of Vlasov–Boltzmann theory
 3.7 Vlasov–Boltzmann equation and fluid theory

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