Results 11 to 20 of about 355,580 (300)

Passage of intraseasonal waves in the subsurface oceans

open access: yesGeophysical Research Letters, 2007
This study exploits the coverage of ARGO (Array for Real‐time Geostrophic Oceanography) float data sets towards identifying passage of intraseasonal waves over the subsurface global oceans. ARGO, a new observing system, has provided an unprecedented data coverage and impact.
T. N. Krishnamurti   +4 more
openaire   +2 more sources

In Search of Subsurface Oceans Within the Uranian Moons. [PDF]

open access: yesJ Geophys Res Planets, 2021
AbstractThe Galileo mission to Jupiter discovered magnetic signatures associated with hidden subsurface oceans at the moons Europa and Callisto using the phenomenon of magnetic induction. These induced magnetic fields originate from electrically conductive layers within the moons and are driven by Jupiter's strong time‐varying magnetic field.
Cochrane CJ   +5 more
europepmc   +6 more sources

Tides in subsurface oceans with meridional varying thickness [PDF]

open access: yes, 2020
Tidal heating can play an important role in the formation and evolution of subsurface oceans of outer-planet moons. Up until now tidal heating has only been studied in subsurface oceans of spatially uniform thickness.
Vermeersen, B.   +5 more
core   +3 more sources

Protein Stability in Titan's Subsurface Water Ocean [PDF]

open access: yesAstrobiology, 2020
Models of Titan predict that there is a subsurface ocean of water and ammonia under a layer of ice. Such an ocean would be important in the search for extraterrestrial life since it provides a potentially habitable environment.
Kyle P, Martin   +3 more
openaire   +2 more sources

Platinum Group Element Traces of CAMP Volcanism Associated With Low‐Latitude Environmental and Biological Disruptions

open access: yesGeophysical Monograph Series, Page 263-304., 2021

Exploring the links between Large Igneous Provinces and dramatic environmental impact

An emerging consensus suggests that Large Igneous Provinces (LIPs) and Silicic LIPs (SLIPs) are a significant driver of dramatic global environmental and biological changes, including mass extinctions.
Jessica H. Whiteside   +3 more
wiley  

+5 more sources

Titan’s obliquity as evidence of a subsurface ocean? [PDF]

open access: yesAstronomy & Astrophysics, 2011
11 pages, 4 ...
Baland, Rose-Marie   +3 more
openaire   +4 more sources

Amplified Subsurface Signals of Ocean Acidification [PDF]

open access: yesGlobal Biogeochemical Cycles, 2023
AbstractWe evaluate the impact of anthropogenic carbon (Cant) accumulation on multiple ocean acidification (OA) metrics throughout the water column and across the major ocean basins using the GLODAPv2.2016b mapped product. OA is largely considered a surface‐intensified process caused by the air‐to‐sea transfer of Cant; however, we find that the partial
Andrea J. Fassbender   +5 more
openaire   +1 more source

Subsurface ocean warming preceded Heinrich Events

open access: yesNature Communications, 2022
AbstractAlthough the global environmental impact of Laurentide Ice-Sheet destabilizations on glacial climate during Heinrich Events is well-documented, the mechanism driving these ice-sheet instabilities remains elusive. Here we report foraminifera-based subsurface (~150 m water depth) ocean temperature and salinity reconstructions from a sediment core
Lars Max   +4 more
openaire   +3 more sources

Redox heterogeneity of subsurface waters in the Mesoproterozoic ocean [PDF]

open access: yesGeobiology, 2014
AbstractA substantial body of evidence suggests that subsurface water masses in mid‐Proterozoic marine basins were commonly anoxic, either euxinic (sulfidic) or ferruginous (free ferrous iron). To further document redox variations during this interval, a multiproxy geochemical and paleobiological investigation was conducted on the approximately 1000‐m ...
Sperling, E.A.   +9 more
openaire   +4 more sources

Reorientation of Sputnik Planitia implies a subsurface ocean on Pluto [PDF]

open access: yesNature, 2016
The deep nitrogen-covered Sputnik Planitia (SP; informal name) basin on Pluto is located very close to the longitude of Pluto's tidal axis[1] and may be an impact feature [2], by analogy with other large basins in the solar system[3,4]. Reorientation[5-7] due to tidal and rotational torques can explain SP's location, but requires it to be a positive ...
F. Nimmo   +74 more
openaire   +5 more sources

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