Results 71 to 80 of about 34,434 (269)
To use accumulated resources of UkrVO digital archive, analysis of the available photographic plates containing images of Uranus and Neptune was conducted.
Yu. Protsyuk +6 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
Tropospheric Composition and Circulation of Uranus with ALMA and the VLA [PDF]
We present Atacama Large Millimeter/submillimeter Array (ALMA) and Very Large Array (VLA) spatial maps of the Uranian atmosphere taken between 2015 and 2018 at wavelengths from 1.3 mm to 10 cm, probing pressures from ∼1 to ∼50 bar at spatial resolutions ...
E. Molter +6 more
semanticscholar +1 more source
Since the Voyager fly-bys of Uranus and Neptune, improved gravity field data have been derived from long-term observations of the planets' satellite motions, and modified shape and solid-body rotation periods were suggested. A faster rotation period (-40
Anderson +47 more
core +1 more source
Abstract Hydropower is considered essential in meeting the increasing demand in low carbon energy in the context of climate change. Greenhouse gas emissions (GHG) by hydroelectric reservoirs have nevertheless become a major concern to the energy sector.
Maud Demarty +4 more
wiley +1 more source
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
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
Auroral emissions from Uranus and Neptune
Uranus and Neptune possess highly tilted/offset magnetic fields whose interaction with the solar wind shapes unique twin asymmetric, highly dynamical, magnetospheres.
L. Lamy
semanticscholar +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
Dynamics of the giant planets of the solar system in the gaseous proto-planetary disk and relationship to the current orbital architecture [PDF]
We study the orbital evolution of the 4 giant planets of our solar system in a gas disk. Our investigation extends the previous works by Masset and Snellgrove (2001) and Morbidelli and Crida (2007, MC07), which focussed on the dynamics of the Jupiter ...
Alessandro Morbidelli +6 more
core +4 more sources

