J/A+AS/105/77 J/A+AS/105/77 Atomic data and spectral line intensities for O V M Cornille J Dubau P Faucher F Bely-Dubau C Blancard Astron. Astrophys. Suppl. Ser. 105 77 1994 1994A&AS..105...77C atomic data line: identification Sun: corona Sun: X-rays, gamma rays X-rays: general The atomic data required to analyse low density coronal plasmas have been calculated and used to interpret X-ray spectra observed by the Flat Crystal Spectrometer of the SMM/NASA satellite in the 14-19 A wavelength range. The emission lines correspond mainly to Fe XVI, Fe XVII, Fe XVIII and some ones to O VII, O VIII.

Id. identification number corresponding to the following level --- Level level --- E energy level cm-1 Id.f1 final level of Ar1 --- Ar1 radiative transition probability (first of the two more important) s-1 Id.f2 Final level of Ar2 --- Ar2 radiative transition probability (second of the two more important) s-1 SAr Sum of all radiative probabilities from the level identified in the first two columns s-1 Tran. transition (with identification numbers of table1) --- LambdaObs observed wavelength from Phillips et al. (1982) 0.1nm Lambda1 observed wavelength from this work 0.1nm Lambda2 observed wavelength from Loulergue & Nussbaumer (1975) 0.1nm Ar1 radiative transition probability form this work s-1 Ar2 radiative transition probability form Loulergue & Nussbaumer (1975) s-1 Id. level identification number (form table1) --- Omega70 fine structure collision strength for an electron impact energy of 70 Ry --- Omega85 fine structure collision strength for an electron impact energy of 85 Ry --- Omega200 fine structure collision strength for an electron impact energy of 200 Ry --- Omega400 fine structure collision strength for an electron impact energy of 400 Ry --- Omega600 fine structure collision strength for an electron impact energy of 600 Ry --- Omega800 fine structure collision strength for an electron impact energy of 800 Ry --- Ts autoionizing level s of the transition (s -> f) --- Tf final level f of the transition (s -> f) --- Es energy of the corresponding captured electron Ry lambda wavelength 0.1nm F*2(sf) Fe XVI dielectronic satellite atomic data s-1 n_F*2(sf) relative importance of each F*2(sf) to this one of the strongest dielectronic line choosen as a reference line --- Level excited level --- Omega60 fine structure collision strength for an electron impact energy of 60 Ry --- Level excited level --- Id. level identification number (see table7) --- Omaga62 fine structure collision strength for an electron impact energy of 62 Ry --- Omaga93 fine structure collision strength for an electron impact energy of 93 Ry --- Omaga124 fine structure collision strength for an electron impact energy of 124 Ry --- Trans. Transition --- Lambda wavelength 0.1nm Epsilon62 line energy differential emissivity for an electron impact energy of 62 Ry ph/s/cm3 Epsilon93 line energy differential emissivity for an electron impact energy of 93 Ry ph/s/cm3 Epsilon124 line energy differential emissivity for an electron impact energy of 124 Ry ph/s/cm3 DE62/E relative energy differential emissivity for an electron impact energy of 62 Ry --- DE93/E relative energy differential emissivity for an electron impact energy of 93 Ry --- DE124/E relative energy differential emissivity for an electron impact energy of 124 Ry --- Trans. transition --- Lambda wavelength 0.1nm Epsilon60 most important inner-shell line energy differential emissivity for an electron impact energy of 60 Ry ph/s/cm3 DE60/E most important relative energy differential emissivity for an electron impact energy of 60 Ry --- CDS 1994May19 J_A+AS_105_77.xml