Answers are grounded in this paper and cite their sources.
Measurements of electron densities and population densities of excited states of neutral helium are presented for afterglows in the C stellarator. Electron densities range from 10¹¹ to 3×{}10¹³ cm^-3, and electron temperatures range from 0.04 to 1 eV. Semiempirical cross-section formulas for transitions among excited levels are deduced by comparing observed excited-state population densities with solutions of detailed transition-rate equations. The agreement between computed and measured values is good, when the assumed cross sections are comparable with impact-parameter approximation results; the agreement is poor - especially at low electron densities and temperatures - when classical cross sections are assumed.
No takes yet. Share an insight, caveat, or question.
Johnson et al. (1969) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: