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Synthetic Line Profiles for Pulsating Red Giants
Pulsation influences atmospheric structures of variable AGB stars (Miras) considerably. Spectral lines of the CO...
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Ultrafast Variability of Line Profiles in Spectra of γ Ori
High time-resolution (∆T~2 min) observations of the B2V star γ Ori on the 2-m telescope at the Terskol Peak Observatory are presented. Regular...
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Regularities in the Behavior of the Line Profiles in Neon Emission Spectra in an Alternating Electric Field
A computer simulation of the spectral line profiles of the neon atom in an alternating circularly polarized electric field is carried out....
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Thermodynamic Profiles of Galaxy Clusters and Groups
The thermodynamic profiles of galaxy clusters and groups are an important probe of the growth of structure in the universe. The structure of the...
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Canonical and Experimental Plasma Pressure Profiles in Tokamaks
AbstractThe statement that the so-called canonical plasma pressure profile is in good agreement with experimental data was the motivating basis for...
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New interactions between various soliton solutions, including bell, kink, and multiple soliton profiles, for the (2+1)-dimensional nonlinear electrical transmission line equation
In this work, we investigate the (2+1)-dimensional nonlinear electrical transmission line model (NETLM) and propose a modified generalized Riccati...
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A Theoretical Method for Calculating the Line Profiles in Atomic Emission Spectra in Alternating Electric Fields
A unified approach is developed for calculating the profiles of the spectral lines of atoms in an alternating electric field on the basis of...
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The Influence of Resonant Absorption on the Fe Emission Line Profiles of Accreting Black Holes
Diffuse plasma existing above an accretion disc can affect the X-ray spectrum by iron K...
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Measuring Stellar Magnetic Fields from Profiles of Near-Infrared Lines
We have obtained high resolution (R = 29 000) spectra in the 15625–15665 Å region for the magnetic chemically peculiar star HD176232 and the...
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Rotation Profiles of Coronal Bright Points Inside and Outside of Coronal Holes
The rotation of the solar corona is not a fully resolved issue. Coronal holes (CHs) reveal sometimes more rigid, but in other cases more differential...
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Analysis of Emission Line Widths of [CII] 158μm
A study of [CII] 158 μm emission line profiles observed with Herschel PACS for 379 galaxies is presented. Emission line widths are compared to [CII]...
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Self-Similar Finite-Time Blowups with Smooth Profiles of the Generalized Constantin–Lax–Majda Model
We show that the a -parameterized family of the generalized Constantin–Lax–Majda model, also known as the Okamoto–Sakajo–Wunsch model, admits exact...
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Exploring the temperature effect on line-scan profile of a pitch structure under electron irradiation
Scanning electron microscope (SEM) is widely used in imaging rather than for thermometry. In this work, the temperature-dependent line-scan profile...
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Entanglement harvesting for different gravitational wave burst profiles with and without memory
In the present article, we study how different gravitational wave (GW) burst profiles in linearized gravity, with and without the asymptotic memory,...
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Construction of Texture Feature Profiles Using Whole Core Images
AbstractStudying images of a whole core (a sample of rock extracted from a well) is in demand in modern geophysics. The subject area determines the...
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The Scale Similarity of Solar Proton Time Profiles in the 23rd Solar Cycle
AbstractWe discussed the scale similarity (scaling) of solar proton time profiles in the 23rd solar cycles. In order to define of scaling...
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Thermodynamic Profiles of Galaxy Clusters and Groups
The thermodynamic profiles of galaxy clusters and groups are an important probe of the growth of structure in the universe. The structure of the...
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Search for Ultrafast Variability of Line Profiles in the Spectrum of ε Per A
The results of observations at high temporal resolution (∆T~4 min) of the B0.5V star ε Per A on the 2-m telescope of the Terskol Observatory are...
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Luminosity dependent cyclotron line in Swift J1626.6−5156
We studied the timing and spectral properties of the Be/X-ray pulsar Swift J1626.6−5156 using the NICER observations of its 2021 outburst. The most...
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Bell-Shaped Refractive Index Profiles of Multimode Optical Fibers and Method for Calculating Their Optical Properties
AbstractOptical properties of multimode fibers with refractive index profiles represented by a wide class of bell-shaped analytical functions are...
