Results 121 to 130 of about 33,171 (317)

Revealing giant planet interiors beneath the cloudy veil

open access: yesNature Communications, 2020
Observations from the Juno and Cassini missions provide essential constraints on the internal structures and compositions of Jupiter and Saturn, resulting in profound revisions of our understanding of the interior and atmospheres of Gas Giant planets ...
Tristan Guillot, Leigh N. Fletcher
doaj   +1 more source

Corotation‐Bounce Resonance of Ions in Jupiter's Magnetosphere

open access: yesGeophysical Research Letters, Volume 52, Issue 3, 16 February 2025.
Abstract Banded energy distributions of H+, O++, S+++, and O+ or S++ ions between 100 eV and ∼20 keV are consistently observed in Jupiter's magnetosphere mapping to M‐shells between M = 10–20. The bands correspond to flux enhancements at similar speeds for different ion species, providing the first evidence of simultaneous bounce‐resonant acceleration ...
Y. Sarkango   +8 more
wiley   +1 more source

Modeling of Multimodal Effects in Two-port Ring-Resonator Circuits for Sensing Applications [PDF]

open access: yes, 2007
Multimodal effects in two-port ring-resonator circuits for sensing applications were modeled using a transfer matrix method and previously published rigorous 3-D modeling tools.
Hoekstra, H.J.W.M.   +2 more
core   +1 more source

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

open access: yes, 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.   +9 more
core   +2 more sources

Stronger Evidence of a Subsurface Ocean Within Callisto From a Multifrequency Investigation of Its Induced Magnetic Field

open access: yesAGU Advances, Volume 6, Issue 1, February 2025.
Abstract The magnetometer investigation of the Galileo mission used the phenomenon of magnetic induction to produce the most compelling evidence that subsurface oceans exist within our solar system. Although there is high certainty that the induced field measured at Europa is attributed to a global‐scale subsurface ocean, there is still uncertainty ...
Corey J. Cochrane   +4 more
wiley   +1 more source

Investigation of the small-scale structure and dynamics of Uranus' atmosphere [PDF]

open access: yes
This document constitutes the final technical report of the Uranus Analysis Program. Papers and/or abstracts resulting from this research are presented.
Eshleman, Von R., Hinson, David P.
core   +1 more source

Noise and resolution in IO interferometric sensing [PDF]

open access: yes, 2007
The paper presents a general theory for sensing devices, relating noise and device parameters to resolution of modal index changes. The theory is applied to optimise the length of a few integrated optics sensing devices, being a Mac-Zehnder ...
Hoekstra, H.J.W.M.   +3 more
core   +1 more source

Uranus Study Report: KISS [PDF]

open access: yes
Determining the internal structure of Uranus is a key objective for planetary science. Knowledge of Uranus's bulk composition and the distribution of elements is crucial to understanding its origin and evolutionary path. In addition, Uranus represents a poorly understood class of intermediate-mass planets (intermediate in size between the relatively ...
arxiv   +1 more source

Future Patterns of Compound Dry and Hot Summers and Their Link to Soil Moisture Droughts in Europe

open access: yesEarth's Future, Volume 13, Issue 2, February 2025.
Abstract Compound dry and hot extreme (CDHE) summers in Europe, like 2015, 2018 and 2022, have wide ranging impacts: heat exacerbates moisture shortages during dry periods whereas water demand rises. Current studies of CDHE are mostly conducted in observations or coarse‐resolution global climate model large ensembles.
Andrea Böhnisch   +4 more
wiley   +1 more source

Variations of brightness temperatures of Uranus and Neptune

open access: yesВісник Астрономічної школи, 2003
In this work variations of brightness temperatures of Uranus and Neptune were investigated. It is obtained, that in the microwave region of spectrum changes of temperature with time are not considerable.
V. M. Krushevs’ka   +2 more
doaj   +1 more source

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