Results 31 to 40 of about 25,199 (146)
Aim: The Impact of surface conditioning protocol i.e., Sandblasting (SB), Bioactive glasses particles (BAGPs), and Phthalocyanine (Pc) activated via low-level laser therapy (LLLT) on the surface roughness (Ra) and shear bond strength (SBS) of hybrid ...
Rana Sulaiman Al-Hamdan +2 more
doaj +1 more source
Recent years have seen increased reports of disruptive behavior at live music events, leading many to question the capacity of audiences to regulate their behavior. This matters both for positive audience experience and for crowd safety. Whilst some previous studies have examined violence in music audiences, there is almost no research looking at the ...
Harry M. Lewis +8 more
wiley +1 more source
Measurements made by Voyager 2 during its flyby of Uranus in 1986 found warm stratospheric and hot thermospheric temperatures that cannot be explained by solar energy alone.
William R. Saunders +4 more
doaj +1 more source
Strong Tidal Dissipation at Uranus?
Geophysical estimates of paleo heat fluxes on the Uranian moons Miranda and Ariel are in the range of 25–75 mW m ^−2 . For a canonical Uranus dissipation factor Q = 18,000, expected equilibrium tidal heating rates for these satellites are less than 6 mW ...
Francis Nimmo
doaj +1 more source
With the development of aerospace science and technology, more and more probes are expected to be deployed around extraterrestrial planets. In this paper, some special orbits around Jupiter, Saturn, Uranus, and Neptune are discussed and analyzed.
Biao Yang +7 more
doaj +1 more source
Astrometry of the main satellites of Uranus: 18 years of observations
We determine accurate positions of the main satellites of Uranus: Miranda, Ariel, Umbriel, Titania, and Oberon. Positions of Uranus, as derived from those of these satellites, are also determined. The observational period spans from 1992 to 2011.
Andrei, A. H. +9 more
core +3 more sources
NMR 15N spin‐relaxation rates are a primary source of information for deciphering protein conformational dynamics, but they require unreasonable experimental times when their 1H‐15N 2D spectra are highly congested. We propose an ultra‐selective method, SNIPER, that greatly accelerates data collection of individual residues. This allows characterization
Wiktor Adamski +3 more
wiley +1 more source
Selection of a common communication link geometry for Saturn, Uranus and Titan [PDF]
Mission analysis link parametrics, considering a Pioneer baseline, are developed through launch energies, flyby radii, and trip time calculations. Projected is also a 1979 Jupiter Uranus opportunity for a derivative Mariner to fly to Uranus by using the ...
Hendricks, T.
core +1 more source
Early Dynamical Evolution of the Solar System: Pinning Down the Initial Condition of the Nice Model [PDF]
In the recent years, the "Nice" model of solar system formation has attained an unprecedented level of success in reproducing much of the observed orbital architecture of the solar system by evolving the planets to their current locations from a more ...
Batygin, Konstantin, Brown, Michael E.
core +3 more sources
Asymmetry in Uranus' High Energy Proton Radiation Belt
Uranus is one of the least explored planets in our solar system, it exhibits a unique magnetic field structure which was observed by NASA's Voyager 2 mission nearly 50 years ago.
M. Acevski +2 more
doaj +1 more source

