Modelling of the novel folded steel structures is therefore also shown to avoid much of the complexity normally encountered in folded structure analysis, such as characterisation of fold-line rotational stiffness or folding plasticity behaviours.
In a biomechanical study, Sairyo et al. reported that extension loading causes a more coronally oriented fracture line, while rotational loading causes a more sagittally oriented fracture line [10].
The latter stars exhibit weak helium lines, low rotational velocities, and excess amounts of gallium, strontium, yttrium, mercury, and platinum, as well as absences of such elements as aluminum and nickel.
So by analyzing the width of these lines, the rotational velocity of a star can be estimated.
Fig. 22 Rotational line profile of Aniline 0 0 origin in helium gas jet with estimated temperature from spectral calculation [61] Fig. 23 Spectra of helium clusters on Anthracene indicating the low temperatures achieved (less than 0.8 K) [21].
The rotational line P1(4) is not used for temperature derivation because there is a strong water vapor absorption line near it.
The N2 1PG (4-4) band emission partially overlaps a rotational line of the OH (8-4) band.
However, this resolution is not sufficient to resolve Λ-splitting effects for each rotational line.
Concentrations were determined using a combination of singular value decomposition matrix techniques and fitting of rotational line sequences.
Fourier transform spectroscopy has been used to record the absorption line shapes for rotational transitions in the Δv=0, b1Σg+←X3Σg− band of O2 in the presence of the noble gases.
In the low energy and momentum transfer region, at about 14.5 meV we observe a sharp line corresponding to rotational transitions between the ground para-J = 0 state and the ground ortho-J = 1 state without change of the translational state of the molecular centre of mass (CoM).
