By V. L. Bychkov (auth.), Viacheslav Shevelko, Hiro Tawara (eds.)
The booklet is a accomplished variation which considers the interactions of atoms, ions and molecules with charged debris, photons and laser fields and displays the current knowing of atomic strategies akin to electron seize, goal and projectile ionisation, photoabsorption and others taking place in so much of laboratory and astrophysical plasma resources together with many-photon and many-electron procedures. the fabric includes chosen papers written by means of top scientists in a variety of fields.
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Physics. Hung. Acad. Sci. KFKI-1987–10/D, (1987) 13. I. Grigorjev, Ball Lightning (YarGU publishers, Yaroslavl, 2006) (In Russian) 14. M. Stenhoff, Ball Lightning. An Unsolved Problem in Atmospheric Physics (Kluwer, New York, 1999) 15. V. Bychkov, A. Nikitin, G. Dijkhuis, in The Atmosphere and Ionospher: Dynamics, Processes and Monitoring, ed. by V. Bychkov, G. Golubkov, A. Nikitin (Springer, Heidelberg, 2010), pp. 201–373 16. M. Smirnov, Phys. Rep. 152, 178 (1987) 17. M. Smirnov, Problem of Ball Lightning (Nauka, Moscow, 1988) (In Russian) 18.
70, 1589 (2008) Chapter 2 Unravelling the Mysteries of Matter Surrounding Supermassive Black Holes A. Muller ¨ and S. Schippers Abstract Uncertainties of atomic data can compromise the interpretation of astronomical observations. Here, we discuss the case of low-temperature dielectronic recombination of iron ions in connection with X-ray spectra from active galactic nuclei, and we explain how new dielectronic recombination rate coefficients from storage-ring experiments have helped to remove previous inconsistencies in the astrophysical modeling of such spectra.
If these DR data are used for the astrophysical modeling of PP, inconsistencies arise. Such inconsistencies have been noted by Netzer  and Kraemer et al.  in the astrophysical modeling of X-ray spectra from AGN. On the basis of their model calculations, these authors have suspected that the DR rate coefficients for iron ions with an open M-shell (Fe1C –Fe15C ) from the widely used compilation of Arnaud and Raymond  are much too low in the PP temperature range. 3 shows the observed X-ray spectrum from an AGN in the wavelength range of the unresolved transition array (UTA) associated with 2p !