Atomic data for x-ray astrophysics
The available atomic data used for interpreting and modeling x-ray observations are
reviewed. The applications for these data can be divided into several levels of detail …
reviewed. The applications for these data can be divided into several levels of detail …
[HTML][HTML] Excitation and ionization by electron impact
O Bely, H Van Regemorter - … and Astrophysics, vol. 8, p. 329, 1970 - adsabs.harvard.edu
Excitation and Ionization by Electron Impact ADS Classic is now deprecated. It will be completely
retired in October 2019. This page will automatically redirect to the new ADS interface at that …
retired in October 2019. This page will automatically redirect to the new ADS interface at that …
Physical properties of solar chromospheric plages: II: Chromospheric plage models
RA Shine, JL Linsky - Solar Physics, 1974 - Springer
We propose chromospheric models of plages to explain profiles of the Ca ii H, K, λ l8498, λ
8542, and λ 8662 lines described in Paper I. These models are consistent with boundary …
8542, and λ 8662 lines described in Paper I. These models are consistent with boundary …
Clocking femtosecond collisional dynamics via resonant x-ray spectroscopy
QY Van den Berg, EV Fernandez-Tello, T Burian… - Physical review …, 2018 - APS
Electron-ion collisional dynamics is of fundamental importance in determining plasma
transport properties, nonequilibrium plasma evolution, and electron damage in diffraction …
transport properties, nonequilibrium plasma evolution, and electron damage in diffraction …
Measured cross sections for ionisation of C3+, N4+ and O5+ ions with contribution due to excitation-autoionisation
DH Crandall, RA Phaneuf… - Journal of Physics B …, 1979 - iopscience.iop.org
Measured cross sections for electron impact ionisation of Li-like ions of C 3+, N 4+ and O 5+
are reported for energies from threshold to 1500 eV. For electron energies from near …
are reported for energies from threshold to 1500 eV. For electron energies from near …
Resonance-line transfer with partial redistribution. II-The solar MG II lines
RW Milkey, D Mihalas - … Journal, vol. 192, Sept. 15, 1974, pt. 1 …, 1974 - adsabs.harvard.edu
Line profiles for the Mg II h and k lines have been calculated, accounting for the partial
frequency redistribution of photons. These profiles are compared with the complete …
frequency redistribution of photons. These profiles are compared with the complete …
X-ray emission from thin plasmas-Collisional ionization for atoms and ions of H to Zn
I Urdampilleta, JS Kaastra, M Mehdipour - Astronomy & Astrophysics, 2017 - aanda.org
Every observation of astrophysical objects involving a spectrum requires atomic data for the
interpretation of line fluxes, line ratios, and ionization state of the emitting plasma. One of the …
interpretation of line fluxes, line ratios, and ionization state of the emitting plasma. One of the …
Excitation of atomic positive ions by electron impact
RJW Henry - Physics Reports, 1981 - Elsevier
Excitation of atomic positive ions by electron impact - ScienceDirect Skip to main contentSkip
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Electron impact ionization of multicharged ions
DH Crandall - Physica Scripta, 1981 - iopscience.iop.org
The available literature on electron impact ionization of ions of charge+ 3 or greater is
reviewed. Several easily used formulae are presented-the classical result, the Lotz formula …
reviewed. Several easily used formulae are presented-the classical result, the Lotz formula …
[HTML][HTML] The solar hydrogen Lyman-beta and Lyman-alpha lines-Disk center observations from OSO 8 compared with theoretical profiles
P Gouttebroze, P Lemaire, JC Vial… - … Part 1, vol. 225, Oct. 15 …, 1978 - adsabs.harvard.edu
The solar hydrogen Lyman-beta and Lyman-alpha lines - Disk center observations f ADS
Classic is now deprecated. It will be completely retired in October 2019. This page will …
Classic is now deprecated. It will be completely retired in October 2019. This page will …