By Y. Hahn, A. Pradhan, H. Tawara, H.L. Zhang

ISBN-10: 3540653473

ISBN-13: 9783540653479

Interactions of photons and electrons with atoms, molecules, and ions are basic simple procedures in a large choice of impartial or ionized gases in nature or laboratory. the information at the move sections or comparable amounts for these approaches are eagerly wanted in lots of fields of program akin to astrophysics, atmospheric technology, plasma technological know-how, radiation physics and chemistry, and so forth. also they are vital in figuring out actual or chemical houses of atoms, molecules, and their ions. quantity I/17 presents go part information and comparable quantitative info at the collisions of photons with atoms, electrons with atoms, and electrons with atomic ions.

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Extra resources for Collisions of Electrons with Atomic Ions (Landolt-Börnstein: Numerical Data and Functional Relationships in Science and Technology - New Series Elementary Particles, Nuclei and Atoms)

Example text

The Iron Project (IP) [93H1] is mostly devoted to calculating reliable collisional data for all iron ions using the most accurate method, the Breit-Pauli R-matrix closecoupling method, with relativistic fine structure effects. The effective, or maxwellian-averaged, collision strengths tabulated in this section are mostly taken from the collective efforts by the IP. Because this is an on-going endeavor, data for some iron ions by the IP are currently not available. For some of these ions data calculated by the RDW method are also tabulated.

1 Excitation [Ref. p. 3–96 Table 1 (continued) Ion Ref. 2 95S3 Schoning Data Rating (Rb-like) 4s − 5f, 5s − 4f CDW N = 51 Xe iv Transitions Ω B Ω,Υ C (Sb-like) CC 5s2 5p3 ; J-levels Effective collision strengths, wavelengths, and A-values At electron temperatures around 10000 K the elements in a plasma source are in low ionization stages and low levels of excitation. In astronomy such sources are often “nebular” plasmas such as found in supernova remnants, diffuse and planetary nebulae, stellar atmospheres, active galactic nuclei, and the interstellar medium.

1 Excitation [Ref. p. 64 − 1 Landolt-B¨ ornstein New Series I/17B Ref. p. 92 + 0 Excitation data for iron ions Electron-impact excitation data for iron ions are very important for astrophysical and other plasam modeling applications. The Iron Project (IP) [93H1] is mostly devoted to calculating reliable collisional data for all iron ions using the most accurate method, the Breit-Pauli R-matrix closecoupling method, with relativistic fine structure effects. The effective, or maxwellian-averaged, collision strengths tabulated in this section are mostly taken from the collective efforts by the IP.

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Collisions of Electrons with Atomic Ions (Landolt-Börnstein: Numerical Data and Functional Relationships in Science and Technology - New Series Elementary Particles, Nuclei and Atoms) by Y. Hahn, A. Pradhan, H. Tawara, H.L. Zhang


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