2 edition of **Oscillator strengths and transition probabilities for 3288 lines of Fe I** found in the catalog.

Oscillator strengths and transition probabilities for 3288 lines of Fe I

Charles H. Corliss

- 377 Want to read
- 1 Currently reading

Published
**1968** by U.S. Dept. of Commerce, National Bureau of Standards; for sale by the Supt. of Docs., U.S. G.P.O. in Washington .

Written in English

- Iron -- Isotopes.,
- Iron -- Spectra -- Tables.

**Edition Notes**

Statement | [by] C.H. Corliss and J.L. Tech. |

Genre | Tables. |

Series | National Bureau of Standards monograph -- 108, NBS monograph -- 108. |

Contributions | Tech, J. L. |

The Physical Object | |
---|---|

Pagination | iii, 66 p. |

Number of Pages | 66 |

ID Numbers | |

Open Library | OL22948212M |

• For an electronic transition to occur an oscillating dipole must be induced by Oscillator strength (f): quantum mechanical model • As a result their oscillator strengths f and emission decay rate constants differ Size: 2MB. Ekberg, J. Wavelengths and transition probabilities of the 3d d 5 4p and 3d 5 4s-3d 5 4p transition arrays of Fe III. Astron. Astrophys. Suppl. Ser. , , 1– [Google Scholar] Corrégé, G.; Hibbert, A. The Oscillator Strengths of Fe II λ λ , Astrophys. J. Author: Peter Uylings, Ton Raassen. "Oscillator Strengths and Transition Probabilities from Breit-Pauli R-matrix Method: Ne IV", Sultana N. Nahar, Atomic Data Nuclear Data Tables , .

You might also like

Twelve Acts for inclosing the common fields in Warwickshire

Twelve Acts for inclosing the common fields in Warwickshire

Urban housing markets, housing supply, and the spatial structure of residential change

Urban housing markets, housing supply, and the spatial structure of residential change

Human society and the church of tomorow

Human society and the church of tomorow

Self-knowledge

Self-knowledge

Phase Transitions and Critical Phenomena/Volume 5B

Phase Transitions and Critical Phenomena/Volume 5B

Comparatively speaking

Comparatively speaking

Knowledge representation in neural networks

Knowledge representation in neural networks

conjurors box

conjurors box

Use of sedimentary structures for recognition of clastic environments. Edited by Monzer S. Shawa

Use of sedimentary structures for recognition of clastic environments. Edited by Monzer S. Shawa

comparative test of the flow of water in 8-inch concrete and vitrified clay sewer pipe

comparative test of the flow of water in 8-inch concrete and vitrified clay sewer pipe

Industrial co-operation and investment in Yugoslavia

Industrial co-operation and investment in Yugoslavia

Marine Corps manual.

Marine Corps manual.

Interviewing

Interviewing

Prevention of occupational cancer

Prevention of occupational cancer

Interventions in HIV transmission among IVDUs

Interventions in HIV transmission among IVDUs

Get this from a library. Oscillator strengths and transition probabilities Oscillator strengths and transition probabilities for 3288 lines of Fe I book lines of Fe I.

[Charles H Corliss; Jack L Tech]. Report of a homogeneous set of intensity-related data calculated for spectral lines of Fe I in the region from to angstroms. The quantities tabulated in the present monograph include log (g__), log (gf), gf,f,gA, and by: Full text of "Oscillator strengths and transition probabilities for lines of Fe I" See other formats.

Oscillator strengths and transition probabilities for lines of Fe I Item Preview remove-circle Share or Embed This Item. EMBED. EMBED (for hosted blogs and item tags) Want more.

Advanced embedding details, examples, and help. No_Favorite. share. An extensive set of oscillator strengths, line strengths, and radiative decay rates for the allowed and forbidden transitions in Fe XIX is presented.

They correspond to fine structure levels of total angular momenta 0≤J≤8 of even and odd parities with 2≤n≤10, 0≤l≤9, 0≤L≤10, and (2S+1)=1, 3, : Sultana Nurun Nahar. Particular attention is given to the lines in the ultraviolet spectrum. The oscillator strengths are calculated for 33 Fe II lines observed in the solar spectrum between λ and nm.

For each line, the emission transition probability Aki, the line strength S, and (for allowed lines) the absorption oscillator strength fik are given, together with the spectroscopic Oscillator strengths and transition probabilities for 3288 lines of Fe I book.

Oscillator strengths and transition probabilities for the fine-structure transitions have been calculated using nonorthogonal orbitals in the multiconfiguration Hartree-Fock : Sultana Nurun Nahar.

We present calculations of the oscillator strengths of Fe II λλ,which are the strongest observed lines in the emission spectrum of the B and D Weigelt blobs of η Carinae.

Fe I OSCILLATOR STRENGTHS FOR TRANSITIONS FROM HIGH-LYING EVEN-PARITY LEVELS E. Den Hartog1, M. Ruffoni2, J. Lawler1, J. Pickering2, K. Lind3 and N. Brewer1 1Department of Physics, University of Wisconsin, Madison, WIUSA 2Blackett Laboratory, Imperial College London, London SW7 2BW, UK 3Department of Physics and Astronomy, Uppsala University, Box Cited by: I.

Introduction. The oscillator strengths (/-values) and transition proba- bilities can be computed from the measurement Oscillator strengths and transition probabilities for 3288 lines of Fe I book the amount of total absorption f0 (nk)dv by graphical integration of the line contours. In the study of the pressure broadening of spectral lines if the integrated absorption coefficients of Cited by: 1.

The electric dipole transition probabilities, oscillator strengths and lifetimes have been calculated using the weakest bound electron potential model theory (WBEPMT) for singly ionized magnesium.

In the calculations both multiplet and fine structure transitions are by: J. () e C. Corliss and J. Tech, Oscillator strengths and transition probabilities for lines of Fe I, Nat. Bur. Std. Monograph no. parison yields no further insight into the cause of the heated mixture of Ar and Fe(CO), of known compo- discrepancy.

by: Fe I Oscillator Strengths 49 desired accuracy. Oscillator strengths for heavy elements are better calculated using semiempirical methods. A goo daccount earlier of theoretical att deerive mpts togfvaluecsan be found in Crossley () and Führ et al. Semi-empirical Oscillator Strengths The most extensive w thoe serk onmi-empirical sotsrencilglatths is or Kubryucz &.

Full text of "Oscillator strengths for ultraviolet lines of Fe I" See other formats. Key Words: Transition probabilities, oscillator strengths, the weakest bound electron potential model theory, atomic ﬂuorine.

Introduction Determination of physical parameters such as oscillator strengths, transition probabilities and atomic lifetimes are very important in research areas where atomic data is widely used.

Hence, the. the new lifetimes to obtain accurate values of oscillator strengths (and transition probabilities). Comparison with previous experiments shows that 22 of the analyzed transitions have no earlier log ()gf-values and for 63 transitions the accuracy of the log (gf)s are improved compared with existing measurements in the literature.

by: Determination of absolute oscillator strengths from lifetime data would be of value in the quantitative interpretation of astrophysical spectra. D.C., ). 19) C.

Corliss and J. Tech, Oscillator strengths and transition probabilities for lines of Fe I, Nat. Bur. Std. Monograph (U.S. Government Printing Office, Washington, D Cited by: Charro and Martin have calculated E2 line strengths for n p − n ′ f, n f − n ′ p forbidden transitions, oscillator strengths for E2-forbidden spectral lines of sodium-isoelectronic ions, from K IX to Cs XLV, transition probabilities for E2 spectral lines between levels with Δ l = 0 of the Na isoelectronic sequence, from Si IV (Z = 14 Author: Yasin Gökçe, Gültekin Çelik, Murat Yıldız.

@article{osti_, title = {Energy levels, oscillator strengths, line strengths, and transition probabilities in Si-like ions of La XLIII, Er LIV, Tm LV, and Yb LVI}, author = {Chen, Zhan-Bin and Ma, Kun and Wang, Hong-Jian and Wang, Kai and Liu, Xiao-Bin and Zeng, Jiao-Long}, abstractNote = {Detailed calculations using the multi.

There is an on-going need for accurate oscillator strengths to be used in astrophysical applications, particularly in plasma diagnostics and in the modelling of stellar atmospheres and the interstellar medium.

There are several databases in regular use which contain some of the required data, although often insufficiently complete, and sometimes not sufficiently by: 3. We present the FERRUM Project, an international collaboration aiming at a production and evaluation of oscillator strengths (transition probabilities) of selected spectral lines of singly ionized iron group elements, that are of astrophysical relevance.

The results obtained include measurements and calculations of permitted and forbidden lines of Fe II. Journal Article: Oscillator strengths and transition probabilities for allowed and forbidden transitions in Fe XIX. Abstract. I have been asked by the Chairman of the Conference to say something about future laboratory work on Fe II.

In a way it is impossible to make a specification of the future experimental program at the laboratories, where measurements of atomic parameters of Fe II are in : Sveneric Johansson.

In spectroscopy, oscillator strength is a dimensionless quantity that expresses the probability of absorption or emission of electromagnetic radiation in transitions between energy levels of an atom or molecule.

The oscillator strength can be thought of as the ratio between the quantum mechanical transition rate and the classical absorption/emission rate of a single electron oscillator with.

They recalculated the Opacity Project multiplet gf-values to oscillator strengths and transition probabilities of individual lines. For completeness, the authors added resonance lines of Ne I, Ar I, Fe I, and Fe II ions which are not coveredmore».

@article{osti_, title = {Fine-structure calculations of energy levels, oscillator strengths, and transition probabilities for sulfur-like iron, Fe XI}, author = {Abou El-Maaref, A., E-mail: [email protected] and Ahmad, Mahmoud and Allam, S. H.}, abstractNote = {Energy levels, oscillator strengths, and transition probabilities for transitions among the 14 LS states belonging to.

The solar neutral iron spectrum. II: Profile synthesis of representative Fe I fraunhofer lines ‘Oscillator Strengths and Transition Probabilities for Lines of Fe i ’, N.B.S. MonographWashington, D.C. (U.S E. F.:‘Oscillator Strengths of Weak Fe i Resonance Lines Measured by Combined Hook and Absorption Techniques Cited by: Wavelengths, energy levels, and E1 transition parameters (oscillator strengths, transition probabilities, and line strengths) have been computed for fine-structure levels.

The calculations have been divided into two main groups, with even and odd parity. The odd-parity group contains 90 levels while the even-parity group has 92 by: 4. This banner text can have markup. web; books; video; audio; software; images; Toggle navigation. "Atomic Data from the IRON Project VII.

Radiative Transition Probabilities for Fe II", Sultana N. Nanar, A&A() "Atomic Data For Opacities Calculations.

XX: Photoionization cross sections and oscillator strengths for Fe II", Sultana N. Nahar and Anil K. Pradhan J. Phys. B 27, () Oscillator strengths and transition probabilities for allowed and forbidden transitions in Fe XIX. Journal Article Nahar, Sultana N., E-mail: [email protected] - Atomic Data and Nuclear Data Tables.

An extensive set of oscillator strengths, line strengths, and radiative decay rates for the allowed and forbidden transitions in Fe.

Vol NIST monograph Modified airy function and WKB solutions to the wave equation -- by Ghatak, A. K Oscillator strengths and transition probabilities for lines of Fe I --by Corliss, C. H.; Tech, J. texts. eye Effect of mortar properties on strength of masonry.

of our transition probability data book series [ll, During the last two decades, many new oscillator- strength calculations and measurements have been per- formed for various spectra of the light elements. Thus, it was only a matter of time until the amount of this new, and inCited by: 2.

The transition wavelengths, transition probabilities, line strengths, and absorption oscillator strengths for 2s 2 2p–2s2p 2 electric dipole (E1) transitions are calculated.

Both valence and core-valence correlation effects were accounted for through single-double multireference (SD-MR) expansions to increasing sets of active : Indu Khatri, Arun Goyal, Avnindra Kumar Singh, Man Mohan. the absorption lines formed by the radiative processes, such as the photo-excitations reported here.

Radiative transitions are obtained from a total of fine structure levels of O II with n ≤ 10, l ≤ 9, and 1/2 ≤ J ≤ 17/2. For spectral analysis oscillator strengths, line strengths, and transition probabilities.

"Oscillator Strengths and Transition Probabilities from Breit-Pauli R-matrix Method: Ne IV", Sultana N. Nahar, Atomic Data Nuclear Data Tables() (Elsevier report on download of the paper in ) Buy Transition probability and oscillator strength by perturbation theory: 1s3pÂ¹, Â³P=1s3dÂ¹, Â³D transition in helium isoelectronic sequence (International journal of quantum chemistry.

[Offprint]) on FREE SHIPPING on qualified orders. These books were structured in a manner similar to the energy level volumes and contained both the transition probabilities and the equivalent expressions of oscillator strength and line strength, since different user commu-nities work with different quantities.

Both experimental and theoretical sources of data were utilized. Among the properties discussed are oscillator strengths for resonance lines, magnetic dipole hyperfine structure constants, lifetimes of metastable states, transition probabilities of intercombination lines, and level structure of rare earth elements.

New results are presented for the 3s 2 3p 2 3 P J – 3s3p 3 5 S 2 transitions in silicon-like. the oscillator strengths, pdf probabilities, and other quantities given in NBS Monograph for lines of Fe!.

For each of the quantities listed in that monograph, a simple transformation ex pression can be written that is based on the correct ing equation given above in .ASD contains data on more than spectra download pdf about Å to µm, with more t energy levels andlines, 73, of which have transition probabilities.

In Version 5, a new Web interface for retrieval of ionization energies and total binding energies of ground states of all atomic spectra has been added.Abstract X-ray emission from neon-like Ebook XVII has ebook observed in a plethora of celestial sources including stellar atmospheres, galaxy clusters, elliptical galaxies, and supernova remnants.

Two of the strongest lines emitted from Fe XVII are the 3d to 2p transitions located at and angstroms and known as 3C and 3D, respectively.