Results 111 to 120 of about 11,862 (238)
Abstract Convection‐permitting regional climate models (CP‐RCMs) often outperform coarser‐resolution models in simulating precipitation, but assessing their accuracy across resolutions and configurations remains challenging. This study evaluates the performance and sensitivity of different configurations of the sixth version of the Canadian Regional ...
Kim Lahaie +3 more
wiley +1 more source
THE WAVE PRINCIPLE OF THE DISTRIBUTION OF SUBSTANCE IN SOLAR SYSTEM
The wave principle of planet system formation and systems of satellites of Jupiter, Saturn and Uranus in the Solar system are considered.
V. A. Smirnov
doaj +1 more source
Uranus and Neptune missions: A study in advance of the next Planetary Science Decadal Survey
The ice giant planets, Uranus and Neptune, represent an important and relatively unexplored class of planet. Most of our detailed information about them comes from fleeting looks by the Voyager 2 spacecraft in the 1980s.
M. Hofstadter +17 more
semanticscholar +1 more source
Soft X‐Ray Emission From Saturn's Magnetosheath II: Solar Wind Driving
Abstract Saturn's magnetosphere is dominated by Enceladus‐sourced neutrals, which spread throughout the system into the magnetosheath. The neutrals can charge exchange with highly charged solar wind ions, causing soft X‐ray emission (<2 ${< } 2$ keV) upon de‐excitation of the ion.
D. Naylor +4 more
wiley +1 more source
Uranus orbiter and probe mission : Project Upsilon [PDF]
Project Upsilon is a proposed NASA Flagship Class, Uranus Orbiter and Probe mission concept to investigate Uranus' planetary magnetic field and atmosphere.
Lu, Jason Yunhe
core +3 more sources
Combination of Density‐Based Spatial Clustering With Grid Search Using Nash Equilibrium
This paper introduces a novel clustering approach that enhances the traditional Density‐Based Spatial Clustering of Applications with Noise (DBSCAN) algorithm by integrating a grid search method and Nash Equilibrium principles and addresses the ...
Uranus Kazemi, Seyfollah Soleimani
doaj +1 more source
Can Radio Occultations Constrain Uranus or Neptune’s Internal Rotation Periods?
The shapes of fluid planets bear the signatures of rotational flattening and atmospheric flows. Precise knowledge of their shapes and wind profiles may therefore reveal their interior rotation rates.
Christopher R. Mankovich +4 more
doaj +1 more source
Tilting Uranus via Secular Spin-Orbit Resonance with Planet 9
Uranus' startlingly large obliquity of 98 degrees has yet to admit a satisfactory explanation. The most widely accepted hypothesis involving a giant impactor that tipped Uranus onto its side encounters several difficulties with regards to the Uranus ...
Lu, Tiger, Laughlin, Gregory
core +1 more source
RESEARCHES OF LONG-TERM VARIATIONS IN URANUS AND NEPTUNE SPECTRA
The results of long-term spectral observations of Solar System giant planets Uranus and Neptune are presented here. Data were obtaining in period 2002-2012 at the peak Terskol Observatory (Northern Caucasus, Russia) using 2-meter Ritchey-Chretien ...
Yu. Kuznyetsova +5 more
doaj +1 more source
The authors here perform ab initio calculations to investigate in the heat transport properties of water at extreme pressure and temperature conditions, typically found in the interior of ice giants such as Uranus and Neptune.
Federico Grasselli +2 more
doaj +1 more source

