![PDF] The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/290d452a55be3047dfac8e8096a5ad5ca1708c97/6-Figure4-1.png "PDF] The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy | Semantic Scholar")
PDF] The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy | Semantic Scholar
IS spectral density functions of kappa distribution plasma for a... | Download Scientific Diagram
Entropy | Free Full-Text | Statistical Uncertainties of Space Plasma Properties Described by Kappa Distributions | HTML
![Nebular and auroral emission lines of [Cl iii] in the optical spectra of planetary nebulae | PNAS](https://www.pnas.org/cms/10.1073/pnas.070590597/asset/3bbe67ea-3bc7-44a7-a378-952ffa8a8686/assets/graphic/pq0705905001.jpeg "Nebular and auroral emission lines of [Cl iii] in the optical spectra of planetary nebulae | PNAS")
Nebular and auroral emission lines of [Cl iii] in the optical spectra of planetary nebulae | PNAS
Electron Kappa Distributions in Astrophysical Nebulae - ScienceDirect
![PDF] The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/290d452a55be3047dfac8e8096a5ad5ca1708c97/6-Figure3-1.png "PDF] The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy | Semantic Scholar")
PDF] The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy | Semantic Scholar
Can the Kappa-distributed Electron Energies Account for the Intensity Ratios of O ii Lines in Photoionized Gaseous Nebulae? - IOPscience
Generation of Kappa Distributions in Solar Wind at 1 au
A Case for Electron-Astrophysics | SpringerLink
Kappa Distributions by George Livadiotis - Ebook | Scribd
Understanding Kappa Distributions: A Toolbox for Space Science and Astrophysics | SpringerLink
Introduction to special section on Origins and Properties of Kappa Distributions: Statistical Background and Properties of Kappa Distributions in Space Plasmas - Livadiotis - 2015 - Journal of Geophysical Research: Space Physics - Wiley Online Library
Electron Kappa Distributions in Astrophysical Nebulae - ScienceDirect
Kappa distributions, in arbitrary normalized units, for different k... | Download Scientific Diagram
Can the Kappa-distributed Electron Energies Account for the Intensity Ratios of O ii Lines in Photoionized Gaseous Nebulae? - IOPscience
Diffuse Radio Emission from Galaxy Clusters | SpringerLink
Origins and Properties of Kappa Distributions: Journal of Geophysical Research: Space Physics
![Nebular and auroral emission lines of [Cl iii] in the optical spectra of planetary nebulae | PNAS](https://www.pnas.org/cms/10.1073/pnas.070590597/asset/73a5662f-5d07-4713-b4ad-57ca3f66b7b6/assets/graphic/pq0705905004.jpeg "Nebular and auroral emission lines of [Cl iii] in the optical spectra of planetary nebulae | PNAS")
Nebular and auroral emission lines of [Cl iii] in the optical spectra of planetary nebulae | PNAS
A Case for Electron-Astrophysics | SpringerLink
Kappa distribution functions approach a thermal Maxwellian core at... | Download Scientific Diagram
![PDF] The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy | Semantic Scholar](https://d3i71xaburhd42.cloudfront.net/290d452a55be3047dfac8e8096a5ad5ca1708c97/4-Table1-1.png "PDF] The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy | Semantic Scholar")
PDF] The continuum emission spectrum of Hf 2-2 near the Balmer limit and the ORL versus CEL abundance and temperature discrepancy | Semantic Scholar
The abundance discrepancy factor and t 2 in nebulae: are non-thermal electrons the culprits?
Ashkbiz Danehkar's Astrophysics Pages - Presentations and Outreach
