0000000001301596

AUTHOR

N. Al-labady

showing 4 related works from this author

Line Identification of Atomic and Ionic Spectra of Holmium in the Near-UV. II. Spectra of Ho ii and Ho iii

2017

Fourier Transform spectra of holmium (Ho) in the UV spectral range from 31,530 to 25,000 cm−1 (317 to 400 nm) have been investigated, particularly focusing on the ionic lines. The distinction between the different degrees of ionization (I, II, and III) is based on differences in signal-to-noise ratios from two Ho spectra, which have been measured with different buffer gases, i.e., neon and argon. Based on 106 known Ho ii and 126 known Ho iii energy levels, 97 lines could be classified as transitions of singly ionized Ho and 9 lines could be classified as transitions of doubly ionized Ho. Of the 97 Ho ii lines, 6 have not been listed in the extant literature. Another 215 lines have been assi…

PhysicsArgon010504 meteorology & atmospheric sciencesAnalytical chemistrychemistry.chemical_elementIonic bondingAstronomy and Astrophysics01 natural sciencesSpectral lineNeonchemistryExtant taxonSpace and Planetary ScienceIonization0103 physical sciencesAtomic physicsHolmium010303 astronomy & astrophysics0105 earth and related environmental sciencesLine (formation)The Astrophysical Journal Supplement Series
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Line Identification of Atomic and Ionic Spectra of Holmium in the Near-UV. Part I. Spectrum of Ho i

2017

The Fourier Transform spectra of a Holmium hollow cathode discharge lamp have been investigated in the UV spectral range from 25,000 up to 31,530 cm−1 (317 to 400 nm). Two Ho spectra have been measured with neon and argon as buffer gases. Based on the intensity ratios from these two spectra, a distinction was made between atomic and ionic lines (ionic lines are discussed in an accompanying paper). Using the known Ho i energy levels, 71 lines could be classified as transitions of atomic Ho, 34 of which have not been published previously. Another 32 lines, which could not be classified, are listed in the literature and assigned as atomic Ho. An additional 370 spectral lines have been assigned…

PhysicsGas-discharge lampArgon010504 meteorology & atmospheric scienceschemistry.chemical_elementIonic bondingAstronomy and Astrophysics01 natural sciencesCathodeSpectral linelaw.invention010309 opticsNeonchemistrySpace and Planetary Sciencelaw0103 physical sciencesAtomic physicsHolmium0105 earth and related environmental sciencesLine (formation)The Astrophysical Journal Supplement Series
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Spectra of a Holmium in the near-UV. I. Ho I.

2017

The Fourier Transform spectra of a Holmium hollow cathode discharge lamp have been investigated in the UV spectral range from 25000 up to 31530cm^-1^ (317 to 400nm). Two Ho spectra have been measured with neon and argon as buffer gases. Based on the intensity ratios from these two spectra, a distinction was made between atomic and ionic lines (ionic lines are discussed in an accompanying paper). Using the known Ho I energy levels, 71 lines could be classified as transitions of atomic Ho, 34 of which have not been published previously. Another 32 lines, which could not be classified, are listed in the literature and assigned as atomic Ho. An additional 370 spectral lines have been assigned t…

observational astronomyUltraviolet astronomyAstrophysics and AstronomyPhysicsPhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsNatural SciencesSpectroscopyAtomic physicsInterdisciplinary Astronomy
researchProduct

Spectra of a Holmium in the near-UV. II.

2017

Fourier Transform spectra of Holmium (Ho) in the UV spectral range from 31530 to 25000cm^-1^ (317 to 400nm) have been investigated, particularly focusing on the ionic lines. The distinction between the different degrees of ionization (I, II, and III) is based on differences in signal-to-noise ratios from two Ho spectra, which have been measured with different buffer gases, i.e., neon and argon. Based on 106 known Ho II and 126 known Ho III energy levels, 97 lines could be classified as transitions of singly ionized Ho and 9 lines could be classified as transitions of doubly ionized Ho. Of the 97 Ho II lines, 6 have not been listed in the extant literature. Another 215 lines have been assign…

observational astronomyUltraviolet astronomyAstrophysics and AstronomyPhysicsNatural SciencesSpectroscopyAtomic physicsInterdisciplinary Astronomy
researchProduct