Results 81 to 90 of about 34,434 (269)

Effective Temperature Of Uranus [PDF]

, 1976
NASA NGR 09-015-047, NGR 22-007-270, NGR 44-012 ...
Fazio, G. G., Low, F. J., Trafton, L., Traub, W. A., Wright, Edward L.   +4 more
core   +1 more source

Information on Judgment Invariance Influences Contributors' Opting‐In Behavior in Sequential Collaboration

Journal of Behavioral Decision Making, Volume 39, Issue 1, January 2026.
ABSTRACT Sequential collaboration describes an aggregation process intensively researched for numerical judgments which is characterized by a first contributor creating a judgment that is subsequently adjusted or maintained by following contributors.
Vincent Eric Fischer, Maren Mayer, Joachim Kimmerle   +2 more
wiley   +1 more source

Asymmetry in Uranus' High Energy Proton Radiation Belt

Geophysical Research Letters
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, A. Masters, S. Zomerdijk‐Russell   +2 more
doaj   +1 more source

Evolution and Magnitudes of Candidate Planet Nine [PDF]

, 2016
The recently renewed interest in a possible additional major body in the outer solar system prompted us to study the thermodynamic evolution of such an object. We assumed that it is a smaller version of Uranus and Neptune.
Linder, Esther F., Mordasini, Christoph
core   +2 more sources

Structure of Jupiter's High‐Latitude Storms: Folded Filamentary Regions Revealed by Juno

Journal of Geophysical Research: Planets, Volume 131, Issue 1, January 2026.
Abstract Sprawling, turbulent cloud formations dominate the meteorology of Jupiter's mid‐to‐high latitudes, known as Folded Filamentary Regions (FFRs). A multi‐wavelength characterization by Juno reveals the spatial distribution, vertical structure, and energetics of the FFRs.
L. N. Fletcher, Z. Zhang, S. Brown, F. A. Oyafuso, J. H. Rogers, M. H. Wong, A. Mura, G. Eichstädt, G. S. Orton, S. Brueshaber, R. Sankar, C. Li, S. M. Levin, F. Biagiotti, T. Guillot, A. P. Ingersoll, D. Grassi, C. J. Hansen, S. Bolton, J. H. Waite   +19 more
wiley   +1 more source

The Upper Atmosphere of Uranus from Stellar Occultations. II. Revised Temperatures in the Upper Stratosphere and Lower Thermosphere

The Planetary Science Journal
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, Michael J. Person, Paul Withers, Richard G. French, Chanita Tubthong   +4 more
doaj   +1 more source

Earth-based Stellar Occultation Predictions for Jupiter, Saturn, Uranus, Neptune, Titan, and Triton: 2023–2050

The Planetary Science Journal, 2023
In support of studies of decadal-timescale evolution of outer solar system atmospheres and ring systems, we present detailed Earth-based stellar occultation predictions for Jupiter, Saturn, Uranus, Neptune, Titan, and Triton for 2023–2050,
Richard G. French, Damya Souami
doaj   +1 more source

Astrometry of the main satellites of Uranus: 18 years of observations

, 2015
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., Assafin, M., Benedetti-Rossi, G., Braga-Ribas, F., Camargo, J. I. B., Dias-Oliveira, A., Gomes-Júnior, A. R., Magalhães, F. P., Neto, D. N. da Silva, Vieira-Martins, R.   +9 more
core   +3 more sources

Jovian Planets [PDF]

, 1998
This resource includes pictures, diagrams and brief details about the four outer giant planets: Jupiter, Uranus, Saturn and Neptune. Educational levels: Primary elementary, Intermediate elementary, Middle school, High school, Informal ...

core   +1 more source

Uranus' Long‐Term Thermospheric Cooling Is Unlikely to Be Primarily Driven by the Solar Wind

Geophysical Research Letters, Volume 52, Issue 24, 28 December 2025.
Abstract Over the last 40 yrs, Uranus' thermospheric temperature has decreased by ∼8 K/yr. Here we show that this is less likely to be driven by solar wind kinetic power than previously thought. We determine that the solar wind kinetic power at Uranus has been increasing since the start of solar cycle 24 in 2009, while Uranus's thermospheric ...
Jamie M. Jasinski, Henrik Melin, James A. Sinclair, Sophia Zomerdijk‐Russell, Nick Achilleos, Carol Paty   +5 more
wiley   +1 more source