Zobrazeno 1 - 10
of 22
pro vyhledávání: '"R. T. Smyth"'
Autor:
J. C. Anderson, R. T. Smyth
Publikováno v:
Active and Passive Electronic Components, Vol 2, Iss 2, Pp 135-145 (1975)
Externí odkaz:
https://doaj.org/article/4e3f341891734dbdab324b48931c2872
Autor:
Phillip C. Stancil, Connor Ballance, James Babb, Brendan M. McLaughlin, R. T. Smyth, Alfred Müller, M. S. Pindzola
Publikováno v:
High Performance Computing in Science and Engineering '19 ISBN: 9783030667917
Our prime computational effort is to support current and future measurements of atomic photoionization cross-sections at various synchrotron radiation facilities, and ion-atom collision experiments, together with plasma, fusion and astrophysical appl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::feec4227256feda3cdb374319031f2fa
https://doi.org/10.1007/978-3-030-66792-4_3
https://doi.org/10.1007/978-3-030-66792-4_3
Publikováno v:
Delahaye, F, Ballance, C P, Smyth, R T & Badnell, N R 2021, ' Quantitative comparison of opacities calculated using the R-matrix and Distorted-Wave methods: Fe XVII ', Monthly Notices of the Royal Astronomical Society, vol. 508, no. 1, pp. 421-432 . https://doi.org/10.1093/mnras/stab2016
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 508 (1), pp.421-432. ⟨10.1093/mnras/stab2016⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 508 (1), pp.421-432. ⟨10.1093/mnras/stab2016⟩
We present here a detailed calculation of opacities for Fe~XVII at the physical conditions corresponding to the base of the Solar convection zone. Many ingredients are involved in the calculation of opacities. We review the impact of each ingredient
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::00bcb535e614c901a9543594baa15913
Publikováno v:
Smyth, R, Ramsbottom, C, Keenan, F, Ferland, G & Ballance, C 2019, ' Towards converged electron-impact excitation calculations of low-lying transitions in Fe II ', Monthly Notices of the Royal Astronomical Society, vol. 483, no. 1, pp. 654-663 . https://doi.org/10.1093/mnras/sty3198
Absorption and emission lines of the iron-peak species Fe II are prominent in the infrared, optical and ultraviolet spectra of a myriad of astrophysical sources, requiring extensive and highly reliable sets of atomic structure and collisional data fo
Autor:
Gary J. Ferland, Marios Chatzikos, Connor Ballance, A. Sarkar, Francis P. Keenan, P. A. M. van Hoof, R. T. Smyth, F. S. Guzmán, Catherine Ramsbottom
Understanding the Fe II emission from active galactic nuclei (AGNs) has been a grand challenge for many decades. The rewards from understanding the AGN spectra would be immense, involving both quasar classification schemes such as “Eigenvector 1”
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7fb9eda14740c0b236c2c2394aac50d5
Autor:
David Ennis, Gregory Hartwell, Ezekial A Unterberg, Cameron Samuell, R. T. Smyth, Stuart Loch, Tyler Abrams, Brian Victor, S.L. Allen, C.A. Johnson, David Maurer
A spectral survey of tungsten emission in the ultraviolet region has been completed in the DIII-D tokamak and the CTH torsatron to assess the potential benefit of UV emission for the diagnosis of gross W erosion. A total of 29 W I spectral lines are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::37e5c56025d990759545b7a99bd25a59
http://arxiv.org/abs/1912.07723
http://arxiv.org/abs/1912.07723
Publikováno v:
Babb, J F, Smyth, R T & McLaughlin, B M 2019, ' Radiative Association of Atomic and Ionic Carbon ', The Astrophysical Journal, vol. 884, no. 2, 155 . https://doi.org/10.3847/1538-4357/ab43cb
We present calculated cross sections and rate coefficients for the formation of the dicarbon cation (C$_2^+$) by the radiative association process in collisions of a C$(^3P)$ atom and a C$^+(^2P^o)$ ion. Molecular structure calculations for a number
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0a4e81ae538a07815094431599b3ee81
https://pure.qub.ac.uk/en/publications/radiative-association-of-atomic-and-ionic-carbon(3fbcc91a-11b2-4015-88d0-81cafef26848).html
https://pure.qub.ac.uk/en/publications/radiative-association-of-atomic-and-ionic-carbon(3fbcc91a-11b2-4015-88d0-81cafef26848).html
Publikováno v:
Smyth, R T, Ballance, C P & Ramsbottom, C A 2019, ' Level resolved photoionisation cross sections for Fe I ', The Astrophysical Journal, vol. 874, no. 2, 144 . https://doi.org/10.3847/1538-4357/ab0d25
Significant contributions to the UV opacity in the solar atmosphere have been found to stem from bound-free transitions in neutral iron. As such, accurate cross sections for the photoionisation process are required for a detailed and meaningful analy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::630dd357719163b879f7d31016c2142f
https://pure.qub.ac.uk/en/publications/level-resolved-photoionisation-cross-sections-for-fe-i(513b2ef4-9e86-4e9e-8fec-8bb5d9fbdeb8).html
https://pure.qub.ac.uk/en/publications/level-resolved-photoionisation-cross-sections-for-fe-i(513b2ef4-9e86-4e9e-8fec-8bb5d9fbdeb8).html
Publikováno v:
Babb, J, Smyth, R & McLaughlin, B 2019, ' Dicarbon formation in collisions of two carbon atoms ', The Astrophysical Journal, vol. 876, no. 1 . https://doi.org/10.3847/1538-4357/ab1088
Radiative association cross sections and rates are computed, using a quantum approach, for the formation of C$_2$ molecules (dicarbon) during the collision of two ground state C($^3$P) atoms. We find that transitions originating in the C$\;^1\Pi_g$,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7787bb29406beb79fa0043d858a3ca7b
Publikováno v:
Fernandez Menchero, L, Smyth, R, Ramsbottom, C & Ballance, C 2019, ' Spectroscopic diagnostics of low-ionized iron-peak elements: Electron-impact excitation of Ni3+ and photoionization of Ni2+. ', Monthly Notices of the Royal Astronomical Society, vol. 483, no. 2154, pp. 2154-2164 . https://doi.org/10.1093/mnras/sty3238
The spectra from Fe-peak elements may be used to determine the temperature and density of various astrophysical objects. Determination of these quantities is underpinned by the accuracy and the comprehensiveness of the underlying atomic structure and
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd767e0f588b2336b6ccdb46c5a88890
http://arxiv.org/abs/1809.05472
http://arxiv.org/abs/1809.05472