On the Influence of the Ionization-Recombination Processes on Hydrogen Plasma Polytropic Index
arXiv:2008.03565 · doi:10.3847/1538-4357/ac0629
Abstract
The polytropic (adiabatic) index for pure hydrogen plasma is analytically calculated as function of reciprocal temperature and degree of ionization. Additionally, the polytropic index is graphically represented as a function of temperature and density. It is concluded that the partially ionized hydrogen plasma cannot be exactly polytropic. The calculated deviations from the mono-atomic value 5/3 are measurable. The analytical result for pure hydrogen plasma is a test example how this approach can be extended for arbitrary gas cocktail.
arXiv comment5 pages, 4 figures, 32 refs
References in corpus (19)
- Physics of Solar Prominences: I - Spectral Diagnostics and Non-LTE Modelling
- CHIANTI - an atomic database for emission lines - Paper XV: Version 9, improvements for the X-ray satellite lines
- Partially Ionized Plasmas in Astrophysics
- The Internal Energy for Molecular Hydrogen in Gravitationally Unstable Protoplanetary Disks
- Three-Dimensional Radiation-Hydrodynamics Calculations of the Envelopes of Young Planets Embedded in Protoplanetary Disks
- Evidence of thermal conduction suppression in a solar flaring loop by coronal seismology of slow-mode waves
- Formation of quasi-periodic slow magnetoacoustic wave trains by the heating/cooling misbalance
- Reconstructing the Solar Wind From Its Early History To Current Epoch
- Simulation of homologous and cannibalistic Coronal Mass Ejections produced by the emergence of a twisted flux rope into the Solar Corona
- The polytropic index of solar coronal plasma in sunspot fan loops and its temperature dependence
- Non-equilibrium calcium ionisation in the solar atmosphere
- Does solar structure vary with solar magnetic activity?
- Time-dependent hydrogen ionisation in the solar chromosphere. I: Methods and first results
- On the Dissociation Equilibrium of H2 in Very Cool, Helium-Rich White Dwarf Atmospheres
- Self-consistent 3D radiative MHD simulations of coronal rain formation and evolution
- Magnetohydrostatic solar prominences in near-potential coronal magnetic fields
- Theory of warm ionized gases: equation of state and kinetic Schottky anomaly
- Sound Absorption in Partially Ionized Hydrogen Plasma and Heating Mechanism of Solar Chromosphere
- Slow magnetosonic wave absorption by pressure induced ionization-recombination dissipation