International audienceHelium-like ions provide the most important x-ray spectral diagnostics in high temperature fusion and astrophysical plasmas. We previously presented computed collision strengths for O VII including relativistic fine structure, levels up to the n = 4 complex and radiation damping of autoionizing resonances. We have extended this work to other He-like ions (N, Ne, Mg, Al, Si, S, Ca). The calculations are carried out using the Breit-Pauli R-matrix (BPRM) method with a 31-level eigenfunction expansion. Collision strengths for the principal lines important in x-ray plasma diagnostics, w, x, y and z, corresponding to the four transitions to the ground level 1s^2 (^1S_0) \longleftarrow 1s2p \big(^1P^o_1\big), 1s2p \big(^3P^o_...
Context. Spectral lines from N-like ions can be used to measure the temperature and density of vario...
Plasma models built on extensive atomic data are essential to interpreting observed cosmic spectra. ...
International audienceThe line ratios R and G of the three main lines of He-like ions (triplet: reso...
International audienceHelium-like ions provide the most important x-ray spectral diagnostics in high...
Helium-like ions provide the most important X-ray spectral diagnostics in high temperature fusion an...
Emission lines from highly-excited states (n ≥ 5) of H- and He-like ions have been detected in astro...
Emission lines from highly-excited states (n ≥ 5) of H- and He-like ions have been detected in astro...
Aims. Spectral lines of He-like ions are among the most prominent features in X-ray spectra from a l...
Aims. Spectral lines of He-like ions are among the most prominent features in X-ray spectra from a l...
Context. Many observed emission lines from space missions are due to highly charged H-like ions. An ...
Context. Many observed emission lines from space missions are due to highly charged H-like ions. An ...
Context. Electron impact excitation collision strengths are required for analysing and interpreting ...
Emission lines from ions in the Mg-like iso-electronic sequence can be used as reliable diagnostics ...
Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for relia...
We describe, and present the results of, a new large-scale R-matrix scattering calculation for the e...
Context. Spectral lines from N-like ions can be used to measure the temperature and density of vario...
Plasma models built on extensive atomic data are essential to interpreting observed cosmic spectra. ...
International audienceThe line ratios R and G of the three main lines of He-like ions (triplet: reso...
International audienceHelium-like ions provide the most important x-ray spectral diagnostics in high...
Helium-like ions provide the most important X-ray spectral diagnostics in high temperature fusion an...
Emission lines from highly-excited states (n ≥ 5) of H- and He-like ions have been detected in astro...
Emission lines from highly-excited states (n ≥ 5) of H- and He-like ions have been detected in astro...
Aims. Spectral lines of He-like ions are among the most prominent features in X-ray spectra from a l...
Aims. Spectral lines of He-like ions are among the most prominent features in X-ray spectra from a l...
Context. Many observed emission lines from space missions are due to highly charged H-like ions. An ...
Context. Many observed emission lines from space missions are due to highly charged H-like ions. An ...
Context. Electron impact excitation collision strengths are required for analysing and interpreting ...
Emission lines from ions in the Mg-like iso-electronic sequence can be used as reliable diagnostics ...
Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for relia...
We describe, and present the results of, a new large-scale R-matrix scattering calculation for the e...
Context. Spectral lines from N-like ions can be used to measure the temperature and density of vario...
Plasma models built on extensive atomic data are essential to interpreting observed cosmic spectra. ...
International audienceThe line ratios R and G of the three main lines of He-like ions (triplet: reso...