The phrase "atomic lines and" is correct and usable in written English.
It can be used in contexts related to physics, chemistry, or any discussion involving atomic structures or spectra.
Example: "The study focused on the atomic lines and their significance in understanding the behavior of different elements."
Alternatives: "atomic spectra and" or "atomic transitions and".
Self-formation of Si atomic lines and dimer vacancy chains on the β-SiC(100) surface is taking place at the phase transition between the 3×2 (Si-rich) and c(4×2) surface reconstructions.
Optical emission spectroscopy of atomic lines and molecular vibrational bands in N2, H2/N2 and Ar/N2 plasmas at steel nitriding conditions have been reported as an application of this diagnostic to plasma nitriding.
The narrow features are atomic lines and the broad features between 5 and 20 μm marked as AIB are due to aromatic compounds.
As a PPN, IRAS 01005+7910 does not emit atomic lines, and thus provides a good platform to search for fulleranes.
This class of over 300 interstellar absorption bands seen in the spectra of background stars have too broad a profile to be due to atomic lines, and are most likely of molecular or solid-state origin.
Several reactive groups such as N2 second positive, ( {text{N}}_{ 2}^ ) first negative and second-order systems, atomic oxygen, helium atomic lines and OH line were observed at the helium emission spectrum.
We will introduce concepts such as atomic lines, line and continuum emission, ionization balance, and emission measure distributions, with emphasis on how they are used to understand the coronae of solar like stars.
The electron temperature of (3600 ± 300) K was estimated by measuring the relative line intensities of zinc atomic lines at 334.50 nm and 472.21 nm.
A broaden 7.51 μm band with a FWHM of 0.1 μm and two narrow atomic lines that are interpreted as H I and [Ne VI] lines can reasonably fit the observations.
The basic philosophy of the package is to provide access to the innards of atomic line databases, and to have flexible tools to interactively compare with the observed data.
The emission intensities of lines related to C1Πu XA1Σg+ transition, are compared with the intensities of Hα, Hβ and Hγ atomic lines.
