Nomenclature C = chord length, m C T = thrust coefficient f = flapping frequency, Hz h tip = plunge amplitude at the wing tip, m k = ωC∕U ∞ , reduced frequency l span = wingspan, m Re = U ∞ C∕ν, Reynolds number r z = z-directional distance away from the wing tip, m S wing = wing area, m 2 St = fh tip ∕U ∞ , Strouhal number U ∞ = freestream velocity, m∕s ν = kinematic viscosity of fluid, m 2 ∕s ...

1 The Cassini cameras have captured the opposition effect in Saturn’s rings with a high 2 radial resolution at phase angles down to 0.01 in the entire main ring system. We de3 rive phase functions from 0.01 to 25 of phase angle in the Wide-Angle Camera clear 4 filters with a central wavelength λcl=0.611 μm and phase functions from 0.001 o to 25 of 5 phase angle in the Narrow-Angle and Wide-Angl...

mas·hyy saturated soil liquefaction during earthquakes, shnakhthshdhyy phenomenon that many researchers in the past three decades has attracted. more research on the liquefaction of saturated soils has focused mas·hyy the natural soils are rarely composed of clean sands, and mixed with clay or silt soils, which is why the study has important ghyrkhmyry and paste. despite numerous studies on the...

Phase-retrieval from measured phaseless field data is of interest for various applications including electromagnetic dosimetry, electromagnetic compatibility investigations, near-field to far-field transformations and antenna diagnostics. In this study two phaseretrieval methods, namely the adjoint field method and the phase angle gradient method, are compared using 3D numerical test cases. The...

We show how the neutrino mixing angles and oscillation phase can be predicted from tri-bimaximal neutrino mixing, corrected by charged lepton mixing angles which are related to quark mixing angles via quark-lepton unification. The tribimaximal neutrino mixing can naturally originate from the see-saw mechanism via constrained sequential dominance (CSD), where CSD can result from the vacuum align...

Introduction: SELENE Spectral Profiler (SP) obtains Lunar Visible to NIR spectral data at spatial resolution of 500 m [1]. Since brightness of lunar surface depends on the viewing geometry, we have to correct these data to the values under certain standard observation geometry prior to the detailed analysis by an adequate phase curve. Although many researchers had proposed photo-metric models a...

The algebra of generalized linear quantum canonical transformations is examined in the perspective of Schwinger’s unitary-canonical operator basis. Formulation of the quantum phase problem within the theory of quantum canonical transformations and in particular with the generalized quantum action-angle phase space formalism is established and it is shown that the conceptual foundation of the qu...