Effective collision strengths for electron impact excitation of fine-structure levels in Fe XI

被引:16
作者
Gupta, GP [1 ]
Tayal, SS
机构
[1] Clark Atlanta Univ, Dept Phys, Atlanta, GA 30314 USA
[2] Meerut Univ, Sanatan Sharam Coll, Dept Phys, Meerut 250001, Uttar Pradesh, India
关键词
atomic data; atomic processes;
D O I
10.1086/306612
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Collision strengths for transitions between the 3s(2)3p(4) P-3(2,1,0), D-1(2), and S-1(0) levels and from these levels to the 3s3p(5) (3)p(2,1,0,)degrees and (1)P(1)degrees levels of Fe XI are calculated using a semirelativistic R-matrix approach. The 38 fine-structure levels arising from the 20 LS 3s(2)3p(4) P-3, D-1, S-1, 3s3p(5) P-3 degrees, P-1 degrees, 3s(2)3p3(S-4 degrees)3d D-3 degrees, 3s(2)3p(3)((2)p degrees)3d P-1,P-3 degrees D-1,D-3 degrees, F-1,F-3 degrees, 3S(2)3p(3)(D-2 degrees)3d S-1,S-3 degrees, (1,3)p degrees, D-1,D-3 degrees, F-1,F-3 degrees states are included in our calculation. These target levels are represented by configuration-interaction wave functions. The relativistic effects are considered in the Breit-Pauli approximation by including one-body mass correction, Darwin term, and spin-orbit terms in the scattering equations. Complicated resonance structures are found to enhance the collision strengths significantly for many transitions in the threshold energy regions. Our collision strengths are compared with the available results of Bhatia & Doschek at 8.0, 16.0,and 24.0 ryd. The collision strengths are integrated over a Maxwellian distribution of electron energies to give effective collision strengths over a wide temperature range.
引用
收藏
页码:1078 / 1081
页数:4
相关论文
共 20 条
[1]   ATOMIC DATA FOR OPACITY CALCULATIONS .2. COMPUTATIONAL METHODS [J].
BERRINGTON, KA ;
BURKE, PG ;
BUTLER, K ;
SEATON, MJ ;
STOREY, PJ ;
TAYLOR, KT ;
YAN, Y .
JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS, 1987, 20 (23) :6379-6397
[2]   Atomic data and spectral line intensities for Fe XI [J].
Bhatia, AK ;
Doschek, GA .
ATOMIC DATA AND NUCLEAR DATA TABLES, 1996, 64 (02) :183-222
[3]   ELECTRON-IMPACT EXCITATION OF RESONANCE LINES OF ALKALI-LIKE POSITIVE-IONS [J].
BURGESS, A ;
SHEOREY, VB .
JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS, 1974, 7 (17) :2403-2416
[4]  
Clementi E., 1974, Atomic Data and Nuclear Data Tables, V14, P177, DOI 10.1016/S0092-640X(74)80016-1
[5]   Fine-structure energy levels and oscillator strengths of Fe XI [J].
Deb, NC ;
Tayal, SS .
ATOMIC DATA AND NUCLEAR DATA TABLES, 1998, 69 (01) :161-170
[6]   EXTREME ULTRAVIOLET-SPECTRA OF SOLAR ACTIVE REGIONS AND THEIR ANALYSIS [J].
DERE, KP .
SOLAR PHYSICS, 1982, 77 (1-2) :77-93
[7]   STELLAR CORONAL ABUNDANCES .2. THE FIRST IONIZATION-POTENTIAL EFFECT AND ITS ABSENCE IN THE CORONA OF PROCYON [J].
DRAKE, JJ ;
LAMING, JM ;
WIDING, KG .
ASTROPHYSICAL JOURNAL, 1995, 443 (01) :393-415
[8]  
DRAKE JJ, 1995, APJ, V443, P416
[10]   THE USE OF SPECTRAL EMISSION-LINES IN THE DIAGNOSTICS OF HOT SOLAR PLASMAS [J].
FELDMAN, U .
PHYSICA SCRIPTA, 1981, 24 (04) :681-711