Sentence examples for i emission from inspiring English sources

As a consequence of the change of the neutral gas to metal ratio the estimated effective electron temperature, Te, changes from ~ 2 eV as estimated from Ar I emission to ~ 0.3 0.6 eV as indicated by W I emission.

Atmospheric dissemination involves three processes: (i) emission from a source, (ii) transport and survival in the atmosphere via the circulation of air masses and (iii) deposition back to the Earth's surface through impaction, turbulent airflows or precipitation.

The proposed mechanism involves: (i) emission of X-ray photons by Hg nanoparticles upon laser exposure, leading to neutron release from D2O, (ii) initiation of Hg → Au transmutation by the capture of neutrons.

An increase in Ar I intensity as Ar percentage increases in an Ar/N2 mixture is observed, while the effect on N2+ emission has a decrease, just the reverse of Ar I emission profile.

Lightcurves of the high excitation Bowen/HeII emission lines and a red continuum at λc ∼ 6000 Å were obtained through narrow interference filters with ULTRACAM, and these were cross-correlated with simultaneous RXTE X-ray lightcurves.

The atomic parameters of Ar I emission lines are taken from the National Institute of Standards and Technology NISTT) database [48].

The aim was to compare (i) emissions among the sites in relation to substrate characteristics and (ii) emissions before and after sludge loading in the STRB.

(i) Emissions reductions achieved by shutting down an existing source or curtailing production or operating hours may be generally credited for offsets if they meet the requirements in paragraphs IV.C.3.i.1.

All HWP used in NRW: For quantification of wood volumes, see III; emissions reduction was calculated using the substitution factor SFMa =1.50 tC/tC.

There is little doubt that changes in counts detected in the myocardium reflect a component of counts that originated from I emissions in the lungs.

The second mirror is aperiodic Mg/SiC multilayer, also a bi-functional mirror with high reflectivity for He-II emission line (30.4 nm) but suppressing He-I emission line (58.4 nm) in astronomy observation, which will replace the traditional combination of periodic multilayer and the fragile film filter.