J/AZh/81/33            Excitation of PtI transitions             (Smirnov, 2004)

Excitation of PtI transitions ending at the levels of the main term. Smirnov Yu.M. <Astron. Zh. 81, 33 (2004)> =2004AZh....81...33S 2004AZh....81...33S =2004ARep...48...29S 2004ARep...48...29S
ADC_Keywords: Atomic physics Abstract: We have experimentally studied the excitation of transitions of the platinum atom ending in levels of the 3D main term. The atoms were excited by a 30 eV monoenergetic electron beam. The lines studied are located at wavelengths of 204-367nm. The largest of the measured excitational cross sections exceed 10-16cm2. The optical-excitation functions measured at electron energies of 0-200eV have complex structures. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table.dat 79 46 Excitational cross sections of the platinum atom -------------------------------------------------------------------------------- Byte-by-byte Description of file: table.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 F7.3 0.1nm Lambda Spectral line wavelength 10- 35 A26 --- Trans Type of transition 37- 39 A3 --- J Inner quantum number 43- 47 I5 cm-1 Elow Energy of low level 49- 53 I5 cm-1 Eup Energy of upper level 54 A1 --- Rem [*] Mark two near levels for which common cross section is given 56- 61 F6.2 10-18cm+2 Q30 ? Excitational cross section for an electron energy of 30eV 64- 69 F6.2 10-18cm+2 Qmax ? Maximum of optical excitation function cross section 72- 75 F4.1 eV E(Qmax) ? Position of maximum Qmax 78- 79 I2 --- OEFnum ? Number of optical excitation function --------------------------------------------------------------------------------
(End) Veta Avedisova (INASAN) 17-Dec-2004
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line