We present results for the electron-impact excitation of highly-charged sulphur ions (S8+–S11+) obtained using the intermediate-coupling frame transformation R-matrix approach. A detailed comparison of the target structure has been made for the four ions to assess the uncertainty on collision strengths from the target structure. Effective collision strengths (Υs) are presented at temperatures ranging from 2 × 102(z + 1)2 K to 2 × 106(z + 1)2 K (where z is the residual charge of ions). Detailed comparisons for the Υs are made with the results of previous calculations for these ions, which will pose insight on the uncertainty in their usage by astrophysical and fusion modelling codes
Context. Sulfur emission lines in the soft X-ray and extreme-ultraviolet regions are obser...
Context. Astrophysical plasma codes are built on atomic databases. In the current atomic databases, ...
We present results for the electron-impact excitation of all Li-like ions from Be+ to Kr33+ which we...
We present results for the electron-impact excitation of highly-charged sulphur ions (S8+–S11+) obta...
We present results for the electron-impact excitation of highly-charged sulphur ions (S8+–S11+) obta...
Emission lines from ions in the Mg-like iso-electronic sequence can be used as reliable diagnostics ...
Context.$\ion{S}{v}$ emission lines have been observed in solar flares, solar upper atmospheres, qui...
Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for relia...
We have carried-out parallel intermediate-coupling frame transformation R-matrix calculations for el...
We present results for the electron-impact excitation of all Ne-like ions from Na+ to Kr26+ obtained...
We have carried-out parallel intermediate-coupling frame transformation R-matrix calculations for el...
We present results for the outer-shell electron-impact excitation of all Na-like ions from Mg+ to Kr...
R-matrix calculations of electron impact excitations have been done for several isoelectronic sequen...
We present results for the electron-impact excitation of all Ne-like ions from Na+ to Kr26+ obtained...
We present results for the outer-shell electron-impact excitation of all Na-like ions from Mg+ to Kr...
Context. Sulfur emission lines in the soft X-ray and extreme-ultraviolet regions are obser...
Context. Astrophysical plasma codes are built on atomic databases. In the current atomic databases, ...
We present results for the electron-impact excitation of all Li-like ions from Be+ to Kr33+ which we...
We present results for the electron-impact excitation of highly-charged sulphur ions (S8+–S11+) obta...
We present results for the electron-impact excitation of highly-charged sulphur ions (S8+–S11+) obta...
Emission lines from ions in the Mg-like iso-electronic sequence can be used as reliable diagnostics ...
Context.$\ion{S}{v}$ emission lines have been observed in solar flares, solar upper atmospheres, qui...
Aims. Emission lines from ions in the Be-like isoelectronic sequence can be used for relia...
We have carried-out parallel intermediate-coupling frame transformation R-matrix calculations for el...
We present results for the electron-impact excitation of all Ne-like ions from Na+ to Kr26+ obtained...
We have carried-out parallel intermediate-coupling frame transformation R-matrix calculations for el...
We present results for the outer-shell electron-impact excitation of all Na-like ions from Mg+ to Kr...
R-matrix calculations of electron impact excitations have been done for several isoelectronic sequen...
We present results for the electron-impact excitation of all Ne-like ions from Na+ to Kr26+ obtained...
We present results for the outer-shell electron-impact excitation of all Na-like ions from Mg+ to Kr...
Context. Sulfur emission lines in the soft X-ray and extreme-ultraviolet regions are obser...
Context. Astrophysical plasma codes are built on atomic databases. In the current atomic databases, ...
We present results for the electron-impact excitation of all Li-like ions from Be+ to Kr33+ which we...