True 3-D displays for avionics and mission crewstations
Elizabeth A. Sholler, Frederick M. Meyer, et al.
SPIE AeroSense 1997
Digital computer calculations in SCF MO approximation on the two lowest excited states of BH, 1σ22σ23σ4σ, 3Σ+ and 1Σ+, from 2.0 a.u. out to dissociation are reported. As shown previously by Grimaldi and coworkers [1], these are stable Rydberg states, but it is now shown that the 3Σ+ potential curve on increasing the interatomic distance R goes over a maximum and then becomes a repulsion curve dissociating to normal atoms. The changing characteristics of the 2σ, 3σ and 4σ orbitals as a function of R are described and discussed. Copyright © 1971 John Wiley & Sons, Inc.
Elizabeth A. Sholler, Frederick M. Meyer, et al.
SPIE AeroSense 1997
Xikun Hu, Wenlin Liu, et al.
IEEE J-STARS
S. Cohen, T.O. Sedgwick, et al.
MRS Proceedings 1983
Robert W. Keyes
Physical Review B