Influence of Electron-Impact Multiple Ionization on Equilibrium and Dynamic Charge State Distributions: A Case Study Using Iron
arXiv:1410.4850 · doi:10.1088/0004-637X/800/1/68
Abstract
We describe the influence of electron-impact multiple ionization (EIMI) on the ionization balance of collisionally ionized plasmas. We are unaware of any previous ionization balance calculations that have included EIMI, which is usually assumed to be unimportant. Here, we incorporate EIMI cross-section data into calculations of both equilibrium and non-equilibrium charge-state distributions (CSDs). For equilibrium CSDs, we find that EIMI has only a small effect and can usually be ignored. However, for non-equilibrium plasmas the influence of EIMI can be important. In particular, we find that for plasmas in which the temperature oscillates there are significant differences in the CSD when including versus neglecting EIMI. These results have implications for modeling and spectroscopy of impulsively heated plasmas, such as nanoflare heating of the solar corona.
arXiv commentSubmitted to the Astrophysical Journal
References in corpus (21)
- Ionization balance for optically thin plasmas: rate coefficients for all atoms and ions of the elements H to Ni
- On Solving the Coronal Heating Problem
- A new approach to analyzing solar coronal spectra and updated collisional ionization equilibrium calculations. II. Additional ionization rate coefficients
- Dielectronic recombination data for dynamic finite-density plasmas I. Goals and methodology
- Collisional Ionization Equilibrium for Optically Thin Plasmas. I. Updated Recombination Rate Coefficients for Bare though Sodium-like Ions
- Ionization Equilibrium Timescales in Collisional Plasmas
- Modeling of iron K lines: radiative and Auger decay data for Fe II-Fe IX
- Hinode X-Ray Telescope Detection of Hot Emission from Quiescent Active Regions: A Nanoflare Signature?
- Evidence of widespread hot plasma in a non-flaring coronal active region from Hinode/XRT
- Non-equilibrium of Ionization and the Detection of Hot Plasma in Nanoflare-heated Coronal Loops
- Diagnosing the time-dependence of active region core heating from the emission measure: I. Low-frequency nanoflares
- Dielectronic recombination of Fe 3p^q ions: a key ingredient for describing X-ray absorption in active galactic nuclei
- The Role of Diffusive Shock Acceleration on Non-Equilibrium Ionization in Supernova Remnants
- Decay Properties of K-Vacancy States in Fe X-Fe XVII
- Hydrodynamic Simulations of Merging Galaxy Clusters: Non-Equilibrium Ionization State and Two-Temperature Structure
- H to Zn Ionization Equilibrium for the Non-Maxwellian Electron kappa-distributions: Updated Calculations
- Are Chromospheric Nanoflares a Primary Source of Coronal Plasma?
- Diagnosing the time-dependence of active region core heating from the emission measure: II. Nanoflare trains
- Storage Ring Cross Section Measurements for Electron Impact Ionization of Fe^11+ Forming Fe^12+ and Fe^13+
- Assessment of the Fluorescence and Auger Data Base used in Plasma Modeling
- Storage Ring Cross Section Measurements for Electron Impact Single and Double Ionization of Fe^13+ and Single Ionization of Fe^16+ and Fe^17+
Cited by in corpus (5)
- A Simple Method for Modeling Collision Processes in Plasmas with a Kappa Energy Distribution
- Electron-Impact Multiple Ionization Cross Sections for Atoms and Ions of Helium through Zinc
- X-ray Spectra from Plasmas with High-Energy Electrons: kappa-distributions and e-e Bremsstrahlung
- A Suzaku X-ray study of the mixed-morphology supernova remnant Kes 69 and searching for its gamma-ray counterpart
- The NuSTAR View of Perseus: the ICM and a Peculiar Hard Excess