Results 1 to 10 of about 6,084,559 (245)

Collision Strengths and Effective Collision Strengths for Allowed Transitions among the n ≤ 5 Degenerate Levels of Atomic Hydrogen [PDF]

open access: yesAtoms, 2018
We report calculations of collision strengths and effective collision strengths for 26 allowed transitions among the n≤ 5 degenerate levels of atomic hydrogen for which the close-coupling (CC) and Born approximations have been used. Results are listed
Kanti M. Aggarwal   +2 more
doaj   +5 more sources

Collision strengths and effective collision strengths for Ne-like Ge [PDF]

open access: yesCanadian Journal of Physics, 2017
We have carried out a calculation of 241 levels for Ne-like Ge (Z = 36) to calculate electron impact collision strengths and effective collision strengths belonging to 1s22s22p5nl, 1s22s12p6nl (n = 3, 4, 5, 6; l = s, p, d, f, g, and h) configurations, which have been calculated by the fully relativistic flexible atomic code (FAC).
Wessameldin S Abdelaziz
exaly   +4 more sources

Effective collision strengths for transitions of Ni XVII

open access: yesJournal of Physics: Conference Series, 2009
Electron impact excitation collision strengths are required for the analysis and interpretation of stellar observations. This calculation aims to provide fine structure effective collision strengths for the Nixvii ion using a method which includes contributions from resonances. A DARC calculation has been performed, involving 37 Jπ states.
C E Hudson   +2 more
exaly   +3 more sources

COLLISION STRENGTHS AND EFFECTIVE COLLISION STRENGTHS FOR TRANSITIONS WITHIN THE GROUND-STATE CONFIGURATION OF S III

open access: yesAstrophysical Journal, 2012
We have carried out a 29-state R-matrix calculation in order to calculate collision strengths and effective collision strengths for the electron impact excitation of S III. The recently developed parallel RMATRX II suite of codes have been used, which perform the calculation in intermediate coupling.
M P Scott, C A Ramsbottom
exaly   +4 more sources

Effective collision strengths for transitions in Fe X [PDF]

open access: yesAstronomy & Astrophysics, 2003
Effective collision strengths for transitions among the lowest 97 fine-structure levels belonging to the (1s 2 2s 2 2p 6 ) 3s 2 3p 2 ,3 s3p 3 ,3 s 2 3p3d, 3p 4 ,3 s3p 2 3d and 3s 2 3d 2 configurations of Fe XIII have been calculated using the fully relativistic Dirac Atomic R-matrix Code (DARC) of Norrington & Grant (2004).
Keenan, Francis, Aggarwal, Kanti
openaire   +4 more sources

Effective collision strengths for O II

open access: yesAstrophysical Journal, 1993
Accurate electron collisional excitation strengths Ω, from 11 state R-matrix calculations performed in LSπ coupling, are convoluted with a Maxwellian velocity distribution to obtain effective collision strengths γ for a range of temperatures 5×10 3 K to 10 6 K for electron excitation of singly ionized atomic oxygen.
Brenda M. McLaughlin, Kenneth L. Bell
exaly   +2 more sources

Toward Autonomous UAV Swarm Navigation: A Review of Trajectory Design Paradigms [PDF]

open access: yesSensors
The development of efficient and reliable trajectory-planning strategies for swarms of unmanned aerial vehicles (UAVs) is an increasingly important area of research, with applications in surveillance, search and rescue, smart agriculture, defence ...
Kaleem Arshid   +4 more
doaj   +2 more sources

Effective collision strengths for transitions in O III

open access: yesAstrophysical Journal, Supplement Series, 1993
Effective collision strengths for transitions among 26 LS-coupled states of the (1s 2 ) 2s 2 2p 2 , 2s2p 3 , 2p 4 , 2s 2 2p3s, 2s 2 2p3p, and 2s 2 2p3d configurations of O III are reported in a wide electron temperature range of 2500-200,000 K. Collision strengths for these transitions have been computed at energies below 13.1 Ry in a fine mesh of ...
K M Aggarwal
exaly   +2 more sources

Collision Strengths of Astrophysical Interest for Multiply Charged Ions

open access: yesAtoms, 2023
The electron impact excitation and ionization processes are crucial for modeling the spectra of different astrophysical objects, from atmospheres of late-type stars to remnants of supernovae and up to the light emission from neutron star mergers, to name
Stephan Fritzsche   +3 more
doaj   +1 more source

Effective collision strengths for Si II [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1989
Collision strengths are presented for electron impact excitation among the eight lowest LS states (corresponding to 15 levels including the splitting of the doublet and quartet terms) of Si II calculated using the R-matrix method. These collision strengths are used to deduce effective collision strengths, adopting a Maxwellian electron energy ...
P. L. Dufton, A. E. Kingston
openaire   +2 more sources

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