Ultrafast Hole Deformation Revealed by Molecular Attosecond Interferometry
Fitting the participation of different orbitals. Experimental (a) and fitting (b) yields of H22. (c) The fitting amplitudes of HOMO (blue lines), HOMO-1 (red lines), and HOMO-2 (green lines) for H22, shown in polar coordinate. (d–f) present the same for H30. For comparison, we present the fitting amplitudes of the three molecular orbitals for H24 (g), H28 (h), and H32 (i). The standard deviation of the fitting amplitudes is estimated to be less than 5%.